{
    "count": 106,
    "next": "http://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=%22Volcanoes%22",
    "previous": null,
    "results": [
        {
            "id": 5675,
            "url": "http://svs.gsfc.nasa.gov/5675/",
            "result_type": "Visualization",
            "release_date": "2026-09-24T14:00:00-04:00",
            "title": "US-India Satellite Captures Time-Lapse Video of Volcanic Eruption",
            "description": "Video of Krasheninnikov eruption starting on December 25, 2025 and ending on August 17, 2026. || nisar_volcano_annotated.00500_print.jpg (1024x576) [507.7 KB] || nisar_volcano_annotated.00500_searchweb.png (320x180) [128.6 KB] || nisar_volcano_annotated.00500_thm.png (80x40) [7.0 KB] || nisar_volcano_annotated.mp4 (3840x2160) [30.0 MB] || nisar_volcano_annotated.mp4.hwshow [189 bytes] || ",
            "hits": 634
        },
        {
            "id": 5669,
            "url": "http://svs.gsfc.nasa.gov/5669/",
            "result_type": "Visualization",
            "release_date": "2026-08-10T15:15:00-04:00",
            "title": "GEOS Aerosols (2025)",
            "description": "Aerosols are tiny solid or liquid particles that float in the atmosphere and can travel long distances, affecting air quality and visibility far from their sources. This visualization still, captured for August 19, 2025 (20:00 UTC), is based on NASA's Goddard Earth Observing System (GEOS) model. The GEOS model delivers realistic, high-resolution weather and aerosol data that enable customized environmental prediction and advances in AI research.",
            "hits": 171
        },
        {
            "id": 14985,
            "url": "http://svs.gsfc.nasa.gov/14985/",
            "result_type": "Produced Video",
            "release_date": "2026-05-13T09:00:00-04:00",
            "title": "TESS Reveals Dazzling Night Sky",
            "description": "This view of the whole sky was constructed from 96 TESS sectors. By the end of September 2025, when the last image of this mosaic was captured, TESS had discovered 679 exoplanets (blue dots) and 5,165 candidates (orange dots). The glowing arc running through the center is the plane of the Milky Way. The Large Magellanic Cloud can be seen along the bottom edge just left of center. Black areas within the oval indicate regions TESS has not yet imaged.Credit: NASA/MIT/TESS and Veselin Kostov (University of Maryland College Park)Alt text: Oval projection of the TESS night sky with exoplanet markersImage description: This oval view of the night sky features a U-shaped band of greyish white running downward from top left to bottom center and then upward to top right. The left side of the U is brighter than the right. Blue and orange dots speckle the image, representing confirmed and candidate exoplanets, respectively. Along the oval’s equator, there are a few black lines and blocks of the sky that are a slightly different shade than the rest of the image. There is an empty black block in the upper left. || TESS_both_bin4_planets-Half.jpg (7740x3900) [11.9 MB] || TESS_both_bin4_planets.jpg (15480x7800) [51.2 MB] || TESS_both_bin4_planets.png (15480x7800) [107.6 MB] || TESS_both_bin4_planets-Half_searchweb.png (320x180) [90.2 KB] || TESS_both_bin4_planets-Half_thm.png (80x40) [5.6 KB] || ",
            "hits": 216
        },
        {
            "id": 5613,
            "url": "http://svs.gsfc.nasa.gov/5613/",
            "result_type": "Visualization",
            "release_date": "2026-02-04T00:00:00-05:00",
            "title": "Shifting Distribution of Land Temperature Anomalies, 1964-2025",
            "description": "The change in the distribution of land temperature anomalies over the years 1951 to 2025.",
            "hits": 382
        },
        {
            "id": 5572,
            "url": "http://svs.gsfc.nasa.gov/5572/",
            "result_type": "Visualization",
            "release_date": "2025-08-08T14:00:02-04:00",
            "title": "GEOS Aerosols",
            "description": "Aerosols are tiny solid or liquid particles that float in the atmosphere and can travel long distances, affecting air quality and visibility far from their sources. This visualization covers the period from August 1 to September 14, 2024, and is based on NASA's Goddard Earth Observing System (GEOS) model, which delivers realistic, high-resolution weather and aerosol data that enable customized environmental prediction and advances in AI research.",
            "hits": 441
        },
        {
            "id": 5552,
            "url": "http://svs.gsfc.nasa.gov/5552/",
            "result_type": "Visualization",
            "release_date": "2025-06-23T09:00:00-04:00",
            "title": "Science On A Sphere: Aerosols in the Air",
            "description": "NASA merges observations, advanced models and computing power to monitor aerosols in the atmosphere. Aerosols are tiny invisible solid or liquid particles that float in the atmosphere and can travel long distances affecting air quality and visibility far from their source. These particles come from natural and human sources and include black carbon (orange/red), sea salt (cyan), dust (magenta) and sulfates (green).",
            "hits": 389
        },
        {
            "id": 5519,
            "url": "http://svs.gsfc.nasa.gov/5519/",
            "result_type": "Visualization",
            "release_date": "2025-03-18T17:05:00-04:00",
            "title": "Surface Water and Ocean Topography (SWOT) Vertical Gravity Gradient",
            "description": "No description available.",
            "hits": 150
        },
        {
            "id": 5452,
            "url": "http://svs.gsfc.nasa.gov/5452/",
            "result_type": "Visualization",
            "release_date": "2025-01-10T11:00:00-05:00",
            "title": "Shifting Distribution of Land Temperature Anomalies, 1964-2024",
            "description": "The change in the distribution of land temperature anomalies over the years 1964 to 2024. This version is in Celsius, a Fahrenheit version is also available. || GISTEMPDist_2024_C.00850_print.jpg (1024x576) [45.7 KB] || GISTEMPDist_2024_C.00850_searchweb.png (320x180) [13.7 KB] || GISTEMPDist_2024_C.00850_thm.png [2.1 KB] || GISTEMPDist_2024_C.mp4 (3840x2160) [21.1 MB] ||",
            "hits": 240
        },
        {
            "id": 5217,
            "url": "http://svs.gsfc.nasa.gov/5217/",
            "result_type": "Visualization",
            "release_date": "2024-12-09T10:00:00-05:00",
            "title": "Northern California Fires in September 2020",
            "description": "This visualization shows the lightning over California on August 16 and 17, 2020 that caused 38 separate fires to ignite. These eventually combined into the August  Complex fire, the first recorded gigafire in California history, which burned until November 12 consuming 1,614 square miles (4,180 square kilometers). As the lightning fades, a series of images shows the smoke emanating from the fires on September 8 of that year. The visible smoke is followed by a series showing the Aerosol Optical Depth (a unitless quantitative metric of how much smoke is present in the atmosphere) as the smoke particles were transported across the Western US and Canada over a 10 day period. || geoxo_fires_v049_2024-02-21_0939.04321_print.jpg (1024x576) [185.9 KB] || geoxo_fires_v049_2024-02-21_0939.04321_searchweb.png (320x180) [78.6 KB] || geoxo_fires_v049_2024-02-21_0939.04321_thm.png (80x40) [5.6 KB] || geoxo_fires_v049_2024-02-21_0939_p30_1080p30.mp4 (1920x1080) [101.5 MB] || geoxo_fires_v049_2024-02-21_0939_1080p60.mp4 (1920x1080) [110.3 MB] || composite (3840x2160) [0 Item(s)] || composite (3840x2160) [0 Item(s)] || geoxo_fires_v049_2024-02-21_0939_2160p60.mp4 (3840x2160) [333.3 MB] || geoxo_fires_v049_2024-02-21_0939_p30_2160p30.mp4 (3840x2160) [322.9 MB] || geoxo_fires_v049_2024-02-21_0939_p30_2160p30.mp4.hwshow || ",
            "hits": 116
        },
        {
            "id": 31241,
            "url": "http://svs.gsfc.nasa.gov/31241/",
            "result_type": "Hyperwall Visual",
            "release_date": "2024-09-23T00:00:00-04:00",
            "title": "East African Rift Valley Volcanoes",
            "description": "Volcanic, tectonic, erosional and sedimentary landforms are all evident in this elevation model image of a region along the East African Rift at Lake Kivu. The area shown covers parts of Congo, Rwanda and Uganda.Lake Kivu, in the lower left of the image, lies within the East African Rift, an elongated tectonic pull-apart depression in Earth's crust. The rift extends to the northeast as a smooth lava- and sediment-filled trough. Two volcanic complexes are seen in the rift. The one closer to the lake is the Nyiragongo volcano, which erupted in January 2002, sending lava toward the lake shore and through the city of Goma. East of the rift, even more volcanoes are seen. These are the Virunga volcano chain, which is the home of the endangered mountain gorillas. Note that the terrain surrounding the volcanoes is much smoother than the eroding mountains that cover most of this view, such that topography alone is a good indicator of the extent of the lava flows.Elevation data used in this image was acquired by the Shuttle Radar Topography Mission aboard Space Shuttle Endeavour, launched on Feb. 11, 2000. The mission used the same radar instrument that comprised the Spaceborne Imaging Radar-C/X-Band Synthetic Aperture Radar (SIR-C/X-SAR) that flew twice on Endeavour in 1994. || ",
            "hits": 290
        },
        {
            "id": 14652,
            "url": "http://svs.gsfc.nasa.gov/14652/",
            "result_type": "Produced Video",
            "release_date": "2024-08-15T17:00:00-04:00",
            "title": "Exploring Volcanoes with NASA’s GEODES Team",
            "description": "Enjoy this music video of NASA’s GEODES team exploring lunar-like landscapes.Complete transcript available.Music credit: “Aerial” by Ben Cosgrove” and \"Volcano\" by Ben Cosgrove. Used with permission from the artist.Watch this video on the NASA Goddard YouTube channel. || ExploringVolcanoes_Thumbnail_print.jpg (1024x576) [185.0 KB] || ExploringVolcanoes_Thumbnail.png (1280x720) [1.2 MB] || ExploringVolcanoes_Thumbnail_searchweb.png (320x180) [106.5 KB] || ExploringVolcanoes_Thumbnail_thm.png (80x40) [8.4 KB] || ExploringVolcanoes_720.mp4 (1280x720) [67.0 MB] || EXPLORING_VOLCANOES_Captions_Final.en_US.srt [2.1 KB] || EXPLORING_VOLCANOES_Captions_Final.en_US.vtt [2.0 KB] || ExploringVolcanoes.mp4 (1920x1080) [471.1 MB] || ",
            "hits": 59
        },
        {
            "id": 31277,
            "url": "http://svs.gsfc.nasa.gov/31277/",
            "result_type": "Hyperwall Visual",
            "release_date": "2024-04-12T00:00:00-04:00",
            "title": "Gravity waves from Hunga Tonga Eruption",
            "description": "Gravity waves caused by the Hunga Tonga-Hunga Ha′apai volcanic eruption can be seen in Geostationary satellite data by taking the difference between subsequent images. Global images are acquired every 10 minutes by the GOES and Himawari weather satellite imagers. Calculating the difference between two subsequent images reveals circular gravity waves spreading out from the eruption center. || ",
            "hits": 114
        },
        {
            "id": 5211,
            "url": "http://svs.gsfc.nasa.gov/5211/",
            "result_type": "Visualization",
            "release_date": "2024-01-12T11:00:00-05:00",
            "title": "Shifting Distribution of Land Temperature Anomalies, 1963-2023",
            "description": "The change in the distribution of land temperature anomalies over the years 1963 to 2023. This version is in Celsius, a Fahrenheit version is also available. || 2023_GISTEMP_Dist_C.00899_print.jpg (1024x576) [38.5 KB] || 2023_GISTEMP_Dist_C.00899_searchweb.png (320x180) [13.9 KB] || 2023_GISTEMP_Dist_C.00899_thm.png (80x40) [2.3 KB] || 2023_GISTEMP_Dist_C.mp4 (3840x2160) [22.3 MB] || 2023_GISTEMP_Dist_C.mp4.hwshow || ",
            "hits": 94
        },
        {
            "id": 5065,
            "url": "http://svs.gsfc.nasa.gov/5065/",
            "result_type": "Visualization",
            "release_date": "2023-05-31T00:00:00-04:00",
            "title": "Shifting Distribution of Land Temperature Anomalies, 1962-2022",
            "description": "The change in the distribution of land temperature anomalies over the years 1962 to 2022. This version is in Celsius, a Fahrenheit version is also available. || GISTEMPDist2022_C.00890_print.jpg (1024x576) [49.0 KB] || GISTEMPDist2022_C.00890_searchweb.png (320x180) [18.8 KB] || GISTEMPDist2022_C.00890_thm.png (80x40) [2.5 KB] || GISTEMPDist2022_C.mp4 (3840x2160) [17.1 MB] || GISTEMPDist2022_C.webm (3840x2160) [4.2 MB] || ",
            "hits": 148
        },
        {
            "id": 14346,
            "url": "http://svs.gsfc.nasa.gov/14346/",
            "result_type": "Produced Video",
            "release_date": "2023-05-30T10:00:00-04:00",
            "title": "Skywatchers Delight! Venus Will Dazzle In The Night Sky Next Weekend! NASA’s Upcoming DAVINCI Mission Will Take The Plunge into Venus’s Hellish Atmosphere Live Shots",
            "description": "Quick link to EDITED BROLL for the live shotsQuick link to pre-recorded interview with DR. JIM GARVIN / DAVINCI Principal InvestigatorAdditional still images of Venus from NASA's Magellan  and Mariner missions. Credit: NASA/JPLLearn more about VENUS  here!!Quick link to pre-recorded interview with MATT GARRISONQuick link to pre-recorded interview with DR LINDSAY HAYS || VENUS.jpeg (1800x720) [220.3 KB] || VENUS_print.jpg (1024x409) [85.9 KB] || VENUS_searchweb.png (320x180) [64.2 KB] || VENUS_thm.png (80x40) [7.4 KB] || ",
            "hits": 93
        },
        {
            "id": 14282,
            "url": "http://svs.gsfc.nasa.gov/14282/",
            "result_type": "Produced Video",
            "release_date": "2023-05-17T11:00:00-04:00",
            "title": "Spitzer, TESS Find Potential Earth-Size World Covered in Volcanoes",
            "description": "LP 791-18 d, illustrated here in an artist's concept, is an Earth-size world about 90 light-years away. The gravitational tug from a more massive planet in the system, shown as a blue disk in the background, may result in internal heating and volcanic eruptions – as much as Jupiter’s moon Io, the most geologically active body in the solar system. Astronomers discovered and studied the planet using data from NASA’s Spitzer Space Telescope and TESS (Transiting Exoplanet Survey Satellite) along with many other observatories.Credit: NASA’s Goddard Space Flight Center/Chris Smith (KBRwyle) || LP79118d_BeautyShot.jpg (2048x1152) [130.9 KB] || LP79118d_Temperate_Earth_BeautyShot_Full.jpg (5760x3240) [2.2 MB] || LP79118d_Temperate_Earth_BeautyShot_Full.png (5760x3240) [12.4 MB] || LP79118d_BeautyShot_searchweb.png (320x180) [59.9 KB] || LP79118d_BeautyShot_thm.png (80x40) [5.1 KB] || ",
            "hits": 80
        },
        {
            "id": 14321,
            "url": "http://svs.gsfc.nasa.gov/14321/",
            "result_type": "Produced Video",
            "release_date": "2023-05-11T15:00:00-04:00",
            "title": "Cosmic Cycles 5: Planetary Fantasia",
            "description": "This video includes music from a synthesized orchestra provided by composer Henry Dehlinger.Music credit: “Planetary Fantasia\" from Cosmic Cycles: A Space Symphony by Henry Dehlinger.  Courtesy of the composer.Watch this video on the NASA Goddard YouTube channel. || Cosmic_Cycles_Planetary_Fantasia_V2_print.jpg (1024x576) [60.4 KB] || Cosmic_Cycles_Planetary_Fantasia_V2.jpg (3840x2160) [465.1 KB] || Cosmic_Cycles_Planetary_Fantasia_V2_searchweb.png (320x180) [40.9 KB] || Cosmic_Cycles_Planetary_Fantasia_V2_thm.png (80x40) [5.2 KB] || Cosmic_Cycles_Planetary_Fantasia.webm (1920x1080) [98.0 MB] || Cosmic_Cycles_Planetary_Fantasia.mp4 (1920x1080) [415.1 MB] || Cosmic_Cycles-Planetary_Fantasia_Online_50mbps.mp4 (1920x1080) [3.5 GB] || Cosmic_Cycles-Planetary_Fantasia_Online_ProRes_1920x1080_2997.mov (1920x1080) [10.9 GB] || ",
            "hits": 189
        },
        {
            "id": 40459,
            "url": "http://svs.gsfc.nasa.gov/gallery/cosmic-cycles5-planetary-fantasia/",
            "result_type": "Gallery",
            "release_date": "2023-05-03T00:00:00-04:00",
            "title": "Cosmic Cycles 5 Planetary Fantasia",
            "description": "Earth’s siblings, the other planets were created at the birth of the solar system. They give us a glimpse of the variety possible in the universe and how rare Earth is. As we explore these other worlds, we fuel our adventurous spirit and discover new wonders at every turn: riverbeds on Mars, volcanoes on Jupiter’s moon Io, auroras on Saturn, and sulfuric-acid clouds on Venus.",
            "hits": 23
        },
        {
            "id": 14223,
            "url": "http://svs.gsfc.nasa.gov/14223/",
            "result_type": "Produced Video",
            "release_date": "2022-10-20T06:00:00-04:00",
            "title": "NOAA and NASA Continue Mission to Monitor Extreme Weather and EnhanceForecasts with JPSS-2 Launching Nov. 1 Live Shots",
            "description": "Associated cut b-roll and pre-recorded interview will be added on Friday, Oct 28th by 4:00 p.m. ET || Screen_Shot_2022-10-19_at_5.13.17_PM.png (3250x1072) [3.1 MB] || Screen_Shot_2022-10-19_at_5.13.17_PM_print.jpg (1024x337) [80.1 KB] || Screen_Shot_2022-10-19_at_5.13.17_PM_searchweb.png (320x180) [93.3 KB] || Screen_Shot_2022-10-19_at_5.13.17_PM_thm.png (80x40) [10.5 KB] || ",
            "hits": 32
        },
        {
            "id": 14214,
            "url": "http://svs.gsfc.nasa.gov/14214/",
            "result_type": "Produced Video",
            "release_date": "2022-09-20T00:00:00-04:00",
            "title": "How NASA Sees the Life Cycle of Volcanic Island Hunga Tonga-Hunga Ha’apai",
            "description": "Complete transcript available. || HHTH_Final.00001_print.jpg (1024x576) [78.9 KB] || Thumbnail.png (2838x1588) [5.2 MB] || HHTH_Final.00001_searchweb.png (320x180) [66.5 KB] || HHTH_Final.00001_thm.png (80x40) [5.0 KB] || HHTH_Final.webm (1920x1080) [43.1 MB] || HHTH_Final.mp4 (1920x1080) [779.2 MB] || HHTH_Audio_otter_ai.en_US.srt [7.7 KB] || HHTH_Audio_otter_ai.en_US.vtt [7.7 KB] || ",
            "hits": 126
        },
        {
            "id": 14134,
            "url": "http://svs.gsfc.nasa.gov/14134/",
            "result_type": "Produced Video",
            "release_date": "2022-05-02T13:00:00-04:00",
            "title": "NASA Simulation Suggests Some Volcanoes Might Warm Climate, Destroy Ozone Layer",
            "description": "Watch this video on the NASA Goddard YouTube channel.Music is \"Good Omens\" by Count Zero and Rohan Stevenson and \"Blue Moons\" by Gresby Race Nash of Universal Production Music || 14134_thumb.jpg (1920x1080) [450.5 KB] || volcanism_14134.00242_searchweb.png (320x180) [71.1 KB] || volcanism_14134.00242_thm.png (80x40) [5.5 KB] || volcanism_14134.mp4 (1920x1080) [377.7 MB] || volcanism_14134.webm (1920x1080) [27.0 MB] || volcanism_14134_caption.en_US.srt [4.9 KB] || volcanism_14134_caption.en_US.vtt [4.7 KB] || ",
            "hits": 86
        },
        {
            "id": 31171,
            "url": "http://svs.gsfc.nasa.gov/31171/",
            "result_type": "Hyperwall Visual",
            "release_date": "2021-12-14T00:00:00-05:00",
            "title": "How do we know for sure about Atmospheric Aerosols?",
            "description": "Dr. Brent Holben explains how NASA's program of global ground-based sun photometers measure aerosols at the surface and why those measurements are so vital to understanding the Earth's processes at the 2021 United Nations Climate Change Conference.   Also available on YouTube || COP26_NASA_Hyperwall_Presentation_Atmospheric_Aerosols.02500_print.jpg (1024x576) [112.3 KB] || COP26_NASA_Hyperwall_Presentation_Atmospheric_Aerosols.02500_searchweb.png (320x180) [81.8 KB] || COP26_NASA_Hyperwall_Presentation_Atmospheric_Aerosols.02500_thm.png (80x40) [7.0 KB] || COP26_NASA_Hyperwall_Presentation_Atmospheric_Aerosols.mp4 (1280x720) [135.7 MB] || COP26_NASA_Hyperwall_Presentation_Atmospheric_Aerosols.webm (1280x720) [110.7 MB] || AERONET-COP26-talk2021.en_US.srt [19.2 KB] || AERONET-COP26-talk2021.en_US.vtt [19.0 KB] || ",
            "hits": 70
        },
        {
            "id": 4920,
            "url": "http://svs.gsfc.nasa.gov/4920/",
            "result_type": "Visualization",
            "release_date": "2021-08-04T17:00:00-04:00",
            "title": "Earth System Observatory",
            "description": "An animated graphic showing the areas of focus for NASA's Earth System Observatory. || EarthSystemObservatory_9.00001_print.jpg (1024x576) [158.4 KB] || EarthSystemObservatory_9.00001_searchweb.png (320x180) [72.0 KB] || EarthSystemObservatory_9.00001_web.png (320x180) [72.0 KB] || EarthSystemObservatory_9.00001_thm.png (80x40) [6.4 KB] || EarthSystemObservatory_9.mp4 (1920x1080) [44.9 MB] || EarthSystemObservatory_9.webm (1920x1080) [4.6 MB] || EarthSystemObservatory_4K_9.mp4 (3840x2160) [47.6 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || EarthSystemObservatory_9.mp4.hwshow [220 bytes] || earth-system-observatory-4k-movie.hwshow [329 bytes] || ",
            "hits": 63
        },
        {
            "id": 40413,
            "url": "http://svs.gsfc.nasa.gov/gallery/earth-science-playlist/",
            "result_type": "Gallery",
            "release_date": "2020-04-01T00:00:00-04:00",
            "title": "Earth Science Playlist",
            "description": "No description available.",
            "hits": 4
        },
        {
            "id": 13526,
            "url": "http://svs.gsfc.nasa.gov/13526/",
            "result_type": "Infographic",
            "release_date": "2020-01-24T10:00:00-05:00",
            "title": "What Makes an Exoplanet Habitable?",
            "description": "Explore this infographic to learn more about the many different factors that make a planet potentially habitable. Complete text transcript available.Machine readable version available.Credit: NASA Goddard Space Flight Center || Infographic_24x70_inset.jpg (1920x1080) [201.2 KB] || Habitability_Infographic_CROP_print.jpg (1024x702) [120.2 KB] || Habitability_Infographic_CROP.png (6667x4573) [1.7 MB] || Habitability_Infographic_FULL_24x70_2024Update.png (6667x19500) [5.4 MB] || Habitability_Infographic_CROP_searchweb.png (320x180) [47.0 KB] || Habitability_Infographic_CROP_thm.png (80x40) [5.7 KB] || ",
            "hits": 198
        },
        {
            "id": 31050,
            "url": "http://svs.gsfc.nasa.gov/31050/",
            "result_type": "Hyperwall Visual",
            "release_date": "2019-08-14T00:00:00-04:00",
            "title": "Landsat View of a Disappearing Glacier in Iceland",
            "description": "Ice loss from 1973 to 2019 || Iceland_glacier_00000_print.jpg (1024x576) [104.7 KB] || Iceland_glacier_00000_searchweb.png (320x180) [93.2 KB] || Iceland_glacier_00000_thm.png (80x40) [6.6 KB] || Iceland_glacier_1080p30_2.mp4 (1920x1080) [25.4 MB] || Iceland_glacier_720p30.mp4 (1280x720) [12.6 MB] || Iceland_glacier_720p30.webm (1280x720) [4.1 MB] || Iceland_glacier_1080p30_h265-TEST.mp4 (1920x1080) [3.8 MB] || 5760x3240_16x9_30p (5760x3240) [128.0 KB] || Iceland_glacier_2160p30.mp4 (3840x2160) [81.4 MB] || ",
            "hits": 53
        },
        {
            "id": 30977,
            "url": "http://svs.gsfc.nasa.gov/30977/",
            "result_type": "Hyperwall Visual",
            "release_date": "2019-03-29T00:00:00-04:00",
            "title": "Nighttime Views of the 2018 Kilauea Eruption",
            "description": "An animation of Landsat-8 truecolor and nighttime imagery shows the prograssion of the East Rift Zone eruption. || kilauea_2018_east_rift_zone_20180712_print.jpg (1024x576) [70.6 KB] || kilauea_2018_east_rift_zone_20180712.png (3840x2160) [1.8 MB] || kilauea_2018_east_rift_zone_20180712_searchweb.png (320x180) [45.1 KB] || kilauea_2018_east_rift_zone_20180712_thm.png (80x40) [3.8 KB] || kilauea_2018_east_rift_zone_720p.mp4 (1280x720) [2.7 MB] || kilauea_2018_east_rift_zone_720p.webm (1280x720) [1.9 MB] || ",
            "hits": 106
        },
        {
            "id": 4726,
            "url": "http://svs.gsfc.nasa.gov/4726/",
            "result_type": "Visualization",
            "release_date": "2019-03-27T00:00:00-04:00",
            "title": "New Island forms in Tonga (Updated)",
            "description": "This visualization shows the evolution Tonga's new island between January 2015 and March 2018. || Tonga_evolutn.1300_print.jpg (1024x576) [129.1 KB] || Tonga_evolutn.1300_searchweb.png (320x180) [84.2 KB] || Tonga_evolutn.1300_web.png (320x180) [84.2 KB] || Tonga_evolutn_Wcredits_1080p30.mp4 (1920x1080) [43.0 MB] || Tonga_evolutn_Wcredits_1080p30_h265.mp4 (1920x1080) [17.9 MB] || Tonga_evolutn_Wcredits_1080p30.webm (1920x1080) [5.8 MB] || Tonga_evolutn_Wcredits_2160p30_h265.mp4 (3840x2160) [50.9 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || Tonga_evolutn_Wcredits_2160p30.mp4 (3840x2160) [140.4 MB] || Tonga_evolutn_Wcredits_1080p30_h265.mp4.hwshow || ",
            "hits": 126
        },
        {
            "id": 30988,
            "url": "http://svs.gsfc.nasa.gov/30988/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-08-29T00:00:00-04:00",
            "title": "Earth System Diagram",
            "description": "Diagram showing parts of the Earth system. || earth_system_diagram_print.jpg (1024x574) [115.6 KB] || earth_system_diagram.png (4104x2304) [1.2 MB] || earth_system_diagram_searchweb.png (320x180) [63.5 KB] || earth_system_diagram_thm.png (80x40) [6.6 KB] || earth_system_diagram.hwshow [208 bytes] || ",
            "hits": 313
        },
        {
            "id": 13025,
            "url": "http://svs.gsfc.nasa.gov/13025/",
            "result_type": "Produced Video",
            "release_date": "2018-08-01T09:00:00-04:00",
            "title": "NASA Scientist Reveals Greenland's Geologic Past",
            "description": "A new map of Greenland's geothermal heat flux is helping to reveal the path of the North American tectonic plate over geologic time. Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music Provided by Killer Tracks: \"Valfri\" by James Alexander Dorman || FACEBOOK_720_13025_Greenland_Hotspot_MASTER_facebook_720.mp4 (1280x720) [173.9 MB] || Greenland_Tectonic_Preview_print.jpg (1024x576) [383.0 KB] || Greenland_Tectonic_Preview.jpg (3840x2160) [3.0 MB] || Greenland_Tectonic_Preview_searchweb.png (320x180) [136.6 KB] || Greenland_Tectonic_Preview_thm.png (80x40) [8.8 KB] || TWITTER_720_13025_Greenland_Hotspot_MASTER_twitter_720.mp4 (1280x720) [28.6 MB] || 13025_Greenland_Hotspot_MASTER.webm (960x540) [53.0 MB] || YOUTUBE_1080_13025_Greenland_Hotspot_MASTER_youtube_1080.mp4 (1920x1080) [228.2 MB] || YOUTUBE_1080_13025_Greenland_Hotspot_MASTER_youtube_1080_Output.en_US.srt [2.5 KB] || YOUTUBE_1080_13025_Greenland_Hotspot_MASTER_youtube_1080_Output.en_US.vtt [2.5 KB] || YOUTUBE_4K_13025_Greenland_Hotspot_MASTER_youtube_4k.mp4 (3840x2160) [543.3 MB] || 13025_Greenland_Hotspot_MASTER_youtube_hq.mov (3840x2160) [1.3 GB] || 13025_Greenland_Hotspot_MASTER.mov (3840x2160) [6.3 GB] || ",
            "hits": 71
        },
        {
            "id": 4635,
            "url": "http://svs.gsfc.nasa.gov/4635/",
            "result_type": "Visualization",
            "release_date": "2018-06-15T11:00:00-04:00",
            "title": "Visualizations of Hunga Tonga Hunga Ha'apai and the Martian Landscape",
            "description": "In early 2015, a volcanic eruption in the Kingdom of Tonga created a new island informally known as Hunga Tonga Hunga Ha'apai (HTHH).  The subsequent evolution of the new island was previously described in \"The Birth of a New Island\" available here.  Below are additional visualizations, including an updated view of the island's appearance in March 2018 as well as some visualizations of the martian surface. Results of this study can enhance our understanding of numerous small volcanic landforms on Mars whose formation may have been in shallow-water environments during epochs when persistent surface water was present.The complete  visualization of \"Using Earth to understand how water may have affected volcanoes on Mars\" is available here.Learn more about the evolution of Earth's newest island and how it could reveal new information about the presence of water on Mars: https://agupubs.onlinelibrary.wiley.com/doi/full/10.1002/2017GL076621 || ",
            "hits": 51
        },
        {
            "id": 12932,
            "url": "http://svs.gsfc.nasa.gov/12932/",
            "result_type": "Produced Video",
            "release_date": "2018-06-08T14:00:00-04:00",
            "title": "Using Earth to Understand How Water May Have Affected Volcanoes on Mars",
            "description": "This scientific data visualization shows the evolution of the newly-erupted island in the Kingdom of Tonga. Results of this study can enhance our understanding of numerous small volcanic landforms on Mars whose formation may have been in shallow-water environments during epochs when persistent surface water was present.Learn more about the evolution of Earth's newest island and how it could reveal new infomration about the presence of water on Mars: Monitoring and Modeling the Rapid Evolution of EArth's Newest Volcanic Island: Hunga Tonga Hunga Ha'apai (Tonga) Using High Spatial Resolution Satellite Observations Authors: J.B. Garvin, D.A. Slayback, V. Ferrini, J. Frawley, C. Giguere, G.R. Asrar, K. AndersonPages: 3445-3452  l   First Published: 26 March 2018- Volumetric erosion for new hydromagmatic island is approximately 0.0026km3/year- Demostrated first meter-scale documentation of landscapes and topography for a new volcanic island over its initial stages of evolution (approximately 3 years)- Satellite-based measurements of news island predict lifetime of up to approximately 42 years || ",
            "hits": 35
        },
        {
            "id": 12819,
            "url": "http://svs.gsfc.nasa.gov/12819/",
            "result_type": "Produced Video",
            "release_date": "2018-06-05T09:50:00-04:00",
            "title": "NASA's Worldview – Two Decades of Earth Data",
            "description": "Two decades of planetary change are available to explore in NASA's Worldview.  Detailed views of volcanoes fuming, hurricanes flooding, dams being built, and wildfires sweeping across landscapes are just some of the data accessible.  Worldview users can even create data animations at the touch of a button and easily share imagery, giving NASA's worldwide audience the ability to interactively view their world their way and interactively explore almost 20 years of planetary change. Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music: Natural Time Cycles by Laurent Dury || Hurricane_Katrina_print.jpg (1024x576) [183.3 KB] || Hurricane_Katrina.png (1920x1080) [3.0 MB] || Hurricane_Katrina_thm.png (80x40) [8.1 KB] || Hurricane_Katrina_searchweb.png (180x320) [111.0 KB] || TWITTER_720_MODIS18years_29.97_V10_twitter_720.mp4 (1280x720) [36.2 MB] || MODIS18years_29.97_V10.webm (960x540) [66.0 MB] || MODIS18years_29.97_V10_appletv_subtitles.m4v (1280x720) [96.9 MB] || MODIS18years_29.97_V10_large.mp4 (1920x1080) [169.2 MB] || MODIS18years_29.97_V10_appletv.m4v (1280x720) [96.9 MB] || YOUTUBE_720_MODIS18years_29.97_V10_youtube_720.mp4 (1280x720) [280.9 MB] || FACEBOOK_720_MODIS18years_29.97_V10_facebook_720.mp4 (1280x720) [226.7 MB] || YOUTUBE_1080_MODIS18years_29.97_V10_youtube_1080.mp4 (1920x1080) [307.0 MB] || MODIS18years_Captions.en_US.vtt [1.8 KB] || MODIS18years_Captions.en_US.srt [1.8 KB] || CH28_MODIS18years_29.97_V10_ch28.mov (1280x720) [1.6 GB] || MODIS18years_29.97_V10_lowres.mp4 (480x272) [22.8 MB] || MODIS18years_29.97_V10.mov (1920x1080) [2.3 GB] || ",
            "hits": 71
        },
        {
            "id": 30962,
            "url": "http://svs.gsfc.nasa.gov/30962/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-05-31T00:00:00-04:00",
            "title": "Sulfur Dioxide Leaks from Kilauea",
            "description": "This series of images, created using data from the Ozone Mapping Profiler Suite (OMPS) sensor on the Suomi National Polar-orbiting Partnership (NPP) satellite, shows elevated concentrations of sulfur dioxide from Hawaii's Kilauea volcano on May 5, 2018. || hawaii_omp_so2.png (1920x1080) [299.9 KB] || hawaii_omp_so2_print.jpg (1024x576) [49.1 KB] || hawaii_omp_so2_searchweb.png (320x180) [31.7 KB] || hawaii_omp_so2_thm.png (80x40) [3.7 KB] || sulfur-dioxide-leaks-from-kilauea-data.hwshow [290 bytes] || ",
            "hits": 44
        },
        {
            "id": 30964,
            "url": "http://svs.gsfc.nasa.gov/30964/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-05-31T00:00:00-04:00",
            "title": "Kilauea Continues to Erupt",
            "description": "On May 14, 2018, at 10:41 AM local time (20:41 Universal Time), the Operational Land Imager (OLI) on Landsat 8 acquired a natural-color image of Hawaii’s Kilauea volcano. || kilauea_continues_print.jpg (1024x682) [280.7 KB] || kilauea_continues.png (4860x3240) [26.3 MB] || kilauea_continues_searchweb.png (320x180) [123.7 KB] || kilauea_continues_thm.png (80x40) [8.0 KB] || kilauea-continues-to-erupt.hwshow [284 bytes] || ",
            "hits": 91
        },
        {
            "id": 30965,
            "url": "http://svs.gsfc.nasa.gov/30965/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-05-31T00:00:00-04:00",
            "title": "The Infrared Glow of Kilauea’s Lava Flows",
            "description": "The Operational Land Imager (OLI) on Landsat 8 acquired the data for this false-color view of the lava flow as it appeared on the night of May 23, 2018. || IR_leilani_print.jpg (1024x574) [95.3 KB] || IR_leilani.png (4104x2304) [3.5 MB] || IR_leilani_searchweb.png (320x180) [44.9 KB] || IR_leilani_thm.png (80x40) [2.7 KB] || the-infrared-glow-of-kilaueas-lava-flows.hwshow [284 bytes] || ",
            "hits": 51
        },
        {
            "id": 30973,
            "url": "http://svs.gsfc.nasa.gov/30973/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-05-27T00:00:00-04:00",
            "title": "Aoba (Ambae) Volcano Eruption, Vanuatu",
            "description": "Activity for Aoba (Ambae) volcano has increased in recent months and is now in a minor eruption state. A restricted area of risk which is 3km around the active vent has been established as the volcano began to become more active in March and early April 2018.  At that time the volcano began to emit more and sustained volcanic ash or/ and gases. Vanuatu’s Council of Ministers has declared a state of emergency on Ambae due to the heavy ash fall which has contaminated water and food supplies for the island’s nearly 11,000 inhabitants, who are in the process of being evacuated from the island. || ",
            "hits": 27
        },
        {
            "id": 12784,
            "url": "http://svs.gsfc.nasa.gov/12784/",
            "result_type": "Produced Video",
            "release_date": "2018-05-21T12:00:00-04:00",
            "title": "Martian Clues on a Baby Island",
            "description": "A young volcanic island on Earth may hold clues to former islands on Mars. || Tonga_v60_vis.0780_16x9.jpg (1024x576) [123.5 KB] || Tonga_v60_vis.0780_16x9_print.jpg (1024x576) [123.6 KB] || Tonga_v60_vis.0780_16x9_searchweb.png (320x180) [96.3 KB] || Tonga_v60_vis.0780_16x9_thm.png (80x40) [7.7 KB] || ",
            "hits": 45
        },
        {
            "id": 12880,
            "url": "http://svs.gsfc.nasa.gov/12880/",
            "result_type": "Produced Video",
            "release_date": "2018-03-05T00:00:00-05:00",
            "title": "Cosmic Designs and The Planets",
            "description": "Greetings and welcome to “Cosmic Designs” a performance by the National Philharmonic presented in partnership with NASA’s Goddard Space Flight Center.“Cosmic Designs” is a voyage that blends together science and art. The pursuit of knowledge and the creative drive for artistic expression are inherent to the human condition. The melding of NASA imagery and symphonic music we present here showcases the imagination that underpins both and highlights how inspiring the combination can be. || CD_Intro_Image_print.jpg (1024x567) [135.2 KB] || CD_Intro_Image.png (2918x1618) [5.8 MB] || CD_Intro_Image_searchweb.png (320x180) [103.7 KB] || CD_Intro_Image_web.png (320x177) [101.8 KB] || CD_Intro_Image_thm.png (80x40) [7.6 KB] || 1.CosmicDesigns_Title_1080.mov (1920x1080) [1.0 GB] || 1.CosmicDesigns_Title_1080.mp4 (1920x1080) [35.9 MB] || 1.CosmicDesigns_Title_1080.webm (1920x1080) [3.3 MB] || 1.CosmicDesigns_Title_4K.mov (3840x2160) [4.3 GB] || 1.CosmicDesigns_Title_4K.mp4 (3840x2160) [55.1 MB] || ",
            "hits": 122
        },
        {
            "id": 4602,
            "url": "http://svs.gsfc.nasa.gov/4602/",
            "result_type": "Visualization",
            "release_date": "2017-12-11T10:00:00-05:00",
            "title": "New island forms in Tonga",
            "description": "This visualization shows the change in the island of Hunga Tonga Hunga Ha'apa between January 2015 and September 2017.This video is also available on our YouTube channel. || Tonga_v60_vis.0780_print.jpg (1024x576) [123.5 KB] || Tonga_v60_vis.0780_searchweb.png (320x180) [76.8 KB] || Tonga_v60_vis.0780_thm.png (80x40) [6.0 KB] || new_island_vis (1920x1080) [0 Item(s)] || Tonga_v60_vis_1080p30.mp4 (1920x1080) [33.3 MB] || Tonga_v60_vis_1080p30.webm (1920x1080) [5.1 MB] || Tonga_4k_final2_1080p30.mp4 (1920x1080) [34.3 MB] || new_island_vis (3840x2160) [0 Item(s)] || Tonga_4k_final2_2160p30.mp4 (3840x2160) [52.0 MB] || Tonga_v60_vis_1080p30.mp4.hwshow [187 bytes] || ",
            "hits": 70
        },
        {
            "id": 12715,
            "url": "http://svs.gsfc.nasa.gov/12715/",
            "result_type": "Produced Video",
            "release_date": "2017-09-21T10:00:00-04:00",
            "title": "Baseball Hits an Eclipse",
            "description": "One of the best places to view the 2017 Total Solar Eclipse was at a ballpark in Keizer, Oregon.  Here, NASA Goddard and the Lunar Reconnaissance Orbiter mission partnered with the Salem-Keizer Volcanoes Minor League Baseball team for an \"EclipseFest\" that featured the first ever \"Eclipse Delay\" in baseball history.  This video shows what took place at the event.Music provided by KillerTracks: \"Dayz On The Road\" - Billy Lincoln, Thomas Dean Pugh-Fields; \"Take Me Out to the Ball Game\" - Harry Edwards; \"The World Is Wide Enough\" - Roger Rodes SendrosWatch this video on the NASA.gov Video YouTube channel. || Volcanoes2Thumnail.jpg (1920x1080) [854.8 KB] || Volcanoes2Thumnail_searchweb.png (320x180) [142.0 KB] || Volcanoes2Thumnail_thm.png (80x40) [9.0 KB] || Baseball-Hits-An-Eclipse-YouTubeHD.mp4 (1920x1080) [420.1 MB] || Baseball-Hits-An-Eclipse-Facebook.mp4 (1280x720) [320.0 MB] || Baseball-Hits-An-Eclipse-MASTER.mov (1920x1080) [3.4 GB] || Baseball-Hits-An-Eclipse-Facebook.webm (1280x720) [31.0 MB] || Baseball-Hits-An-Eclipse-Captions.en_US.srt [4.7 KB] || Baseball-Hits-An-Eclipse-Captions.en_US.vtt [4.7 KB] || ",
            "hits": 51
        },
        {
            "id": 4582,
            "url": "http://svs.gsfc.nasa.gov/4582/",
            "result_type": "Visualization",
            "release_date": "2017-07-27T18:00:00-04:00",
            "title": "Aerosol Optical Thickness Updating Forecast",
            "description": "The atmosphere is made up of gases like oxygen, nitrogen, and water vapor, but it also contains tiny particles called aerosols. Aerosols come from both natural and human sources and include things like sea salt, dust, soot, and sulfates. Aerosols often contribute to air pollution and poor visibility. Once they are in the atmosphere, they can travel long distances, affecting air quality far from their source. Aerosols also absorb or reflect energy (light), influencing temperatures in the atmosphere and on the ground. Satellites measure aerosols by how much light can pass through them. A thick layer of aerosols will block the ground from view, while a thin layer allows enough light through to see the ground. The measurement is called aerosol optical thickness.The GEOS model is built on satellite data and provides a forecast of aerosol optical thickness (among other things). This animation shows a daily updated 10-day forecast of aerosol optical thickness from GEOS. The date and timestamp are in the lower left corner. In general, brighter colors are thick aerosols, while dull darker colors are thin aerosols. Blue represents sea salt (sea salt extinction aerosol optical thickness, 550 nm). Winds blowing across the ocean kicks up ocean spray, which includes sea salt. In the animation, pale blue to white colors reflect stormy conditions. Individual large storms like tropical cyclones (hurricanes, typhoons) are visible as swirling circles of thick sea salt. Red represents dust (dust extinction aerosol optical thickness, 550 nm). The Saharan Desert of northern Africa is the largest source of dust, but dust can be seen across the globe. Saharan dust often interacts with tropical cyclones.Green represents the sum of aerosol optical thickness for organic carbon, black carbon, and sulfate. Organic and black carbon come from burning biomass or fossil fuels. Sources include fires, power plants, vehicles, and other combustion engines that run on fossil fuel. Sulfate particles come mostly from burning fossil fuels, but also from volcanoes. || gmao_aerosols_print.jpg (1024x576) [201.6 KB] || gmao_aerosols_searchweb.png (320x180) [108.3 KB] || gmao_aerosols.00001_thm.png (80x40) [7.0 KB] || gmao_aerosols.mp4 (1920x962) [16.2 MB] || gmao_aerosols.webm (1920x962) [1.5 MB] || latest-wdates (2239x1123) [0 Item(s)] || latest-nodates (2239x1123) [0 Item(s)] || gmao_aerosols.mp4.hwshow [191 bytes] || ",
            "hits": 72
        },
        {
            "id": 40323,
            "url": "http://svs.gsfc.nasa.gov/gallery/applied-science/",
            "result_type": "Gallery",
            "release_date": "2017-03-30T00:00:00-04:00",
            "title": "Applied Science",
            "description": "Discovering innovative and practical uses of Earth observations\n\nappliedsciences.nasa.gov",
            "hits": 19
        },
        {
            "id": 12518,
            "url": "http://svs.gsfc.nasa.gov/12518/",
            "result_type": "Produced Video",
            "release_date": "2017-02-17T11:00:00-05:00",
            "title": "ATom Postcard - Kona, Hawaii",
            "description": "Atmospheric scientist Jack Dibb of the University of New Hampshire sent a video postcard from the Hawaii leg of the Atmospheric Tomography or ATom mission. On its second worldwide tour, the ATom team flew into Kona, Hawaii, to study small particles like sulfate and nitrate in the atmosphere. Volcanoes like Kilauea, in Hawaii, constantly release sulfate particles, which can oxidize to make sulfuric acid, a component of acid rain.  Complete transcript available. || LARGE_MP4-12518_ATom2_Hawaii_large.00007_print.jpg (1024x576) [66.6 KB] || LARGE_MP4-12518_ATom2_Hawaii_large.00007_searchweb.png (320x180) [62.6 KB] || LARGE_MP4-12518_ATom2_Hawaii_large.00007_thm.png (80x40) [4.3 KB] || LARGE_MP4-12518_ATom2_Hawaii_large.mp4 (1920x1080) [91.6 MB] || WEBM-12518_ATom2_Hawaii.webm (960x540) [33.1 MB] || APPLE_TV-12518_ATom2_Hawaii_appletv.m4v (1280x720) [42.7 MB] || APPLE_TV-12518_ATom2_Hawaii_appletv_subtitles.m4v (1280x720) [42.8 MB] || NASA_PODCAST-12518_ATom2_Hawaii_ipod_sm.mp4 (320x240) [17.0 MB] || ATom2_Hawaii.en_US.srt [1.6 KB] || ATom2_Hawaii.en_US.vtt [1.6 KB] || NASA_TV-12518_ATom2_Hawaii.mpeg (1280x720) [299.3 MB] || YOUTUBE_HQ-12518_ATom2_Hawaii_youtube_hq.mov (1920x1080) [252.3 MB] || ",
            "hits": 22
        },
        {
            "id": 12482,
            "url": "http://svs.gsfc.nasa.gov/12482/",
            "result_type": "Produced Video",
            "release_date": "2017-01-12T13:00:00-05:00",
            "title": "NASA to Explore Volcanoes, Coral Reefs, and Snowpacks",
            "description": "Complete transcript available. || EarthEx2.00450_print.jpg (1024x576) [110.8 KB] || EarthEx2.00450_searchweb.png (320x180) [61.7 KB] || EarthEx2.00450_thm.png (80x40) [5.3 KB] || EarthEx2.mp4 (1920x1080) [72.4 MB] || EarthEx2.webm (1920x1080) [7.9 MB] || EarthEx2.mov (3840x2160) [3.5 GB] || EarthEx2.en_US.srt [1.2 KB] || ",
            "hits": 23
        },
        {
            "id": 12392,
            "url": "http://svs.gsfc.nasa.gov/12392/",
            "result_type": "Produced Video",
            "release_date": "2016-10-17T03:00:00-04:00",
            "title": "Ultraviolet Mars Reveals Cloud Formation",
            "description": "Ultraviolet images from NASA's Mars Atmosphere and Volatile Evolution mission, MAVEN, were used to make this movie of rapid cloud formation on Mars. Watch this video on the NASA.gov Video YouTube channel. || MarsCloudsUltravioletPreview.jpg (800x800) [87.2 KB] || MarsCloudsUltravioletPreview_searchweb.png (320x180) [83.3 KB] || MarsCloudsUltravioletPreview_thm.png (80x40) [6.8 KB] || IUVS3CloudMovie.mov (800x800) [8.4 MB] || IUVS3CloudMovie_large.mp4 (800x800) [11.1 MB] || IUVS3CloudMovie.webm (960x540) [4.3 MB] || ",
            "hits": 47
        },
        {
            "id": 30800,
            "url": "http://svs.gsfc.nasa.gov/30800/",
            "result_type": "Hyperwall Visual",
            "release_date": "2016-08-29T12:00:00-04:00",
            "title": "Highlighting National Parks on the National Park Service Centennial",
            "description": "Grand Canyon from the ISS, photo by NASA astronaut Jeff Williams || grandcanyon_ISS_jsc2016e073419.jpg (6000x2460) [1.7 MB] || grandcanyon_ISS_jsc2016e073419_searchweb.png (320x180) [60.4 KB] || grandcanyon_ISS_jsc2016e073419_thm.png (80x40) [4.8 KB] || grandcanyon_ISS_jsc2016.key [2.1 MB] || grandcanyon_ISS_jsc2016.pptx [1.5 MB] || nps-centennial-grand-canyon.hwshow [225 bytes] || ",
            "hits": 58
        },
        {
            "id": 12246,
            "url": "http://svs.gsfc.nasa.gov/12246/",
            "result_type": "Produced Video",
            "release_date": "2016-05-19T11:00:00-04:00",
            "title": "Tracking Volcanic Ash",
            "description": "NASA satellite data could help reduce flights sidelined by volcanic eruptions. || c-1024.jpg (1024x576) [93.6 KB] || c-1280.jpg (1280x720) [126.2 KB] || c-1920.jpg (1920x1080) [192.8 KB] || c-1024_print.jpg (1024x576) [95.2 KB] || c-1024_searchweb.png (320x180) [50.6 KB] || c-1024_web.png (320x180) [50.6 KB] || c-1024_thm.png (80x40) [16.7 KB] || ",
            "hits": 60
        },
        {
            "id": 12181,
            "url": "http://svs.gsfc.nasa.gov/12181/",
            "result_type": "Produced Video",
            "release_date": "2016-03-22T16:56:00-04:00",
            "title": "Mars Gravity Map",
            "description": "Scientists have used small fluctuations in the orbits of three NASA spacecraft to map the gravity field of Mars. || c-1024.jpg (1024x576) [238.0 KB] || c-1280.jpg (1280x720) [324.9 KB] || c-1920.jpg (1920x1080) [504.9 KB] || c-1024_print.jpg (1024x576) [251.2 KB] || c-1024_searchweb.png (320x180) [97.5 KB] || c-1024_web.png (320x180) [97.5 KB] || c-1024_thm.png (80x40) [7.0 KB] || ",
            "hits": 90
        },
        {
            "id": 30706,
            "url": "http://svs.gsfc.nasa.gov/30706/",
            "result_type": "Hyperwall Visual",
            "release_date": "2015-10-28T12:00:00-04:00",
            "title": "Io in Motion",
            "description": "Io a moon of Jupiter in motion || io_in_motion_grid_1280x720_print.jpg (1024x576) [42.0 KB] || io_in_motion_grid_1280x720_searchweb.png (180x320) [31.9 KB] || io_in_motion_grid_1280x720_web.png (320x180) [31.9 KB] || io_in_motion_grid_1280x720_thm.png (80x40) [3.0 KB] || io_in_motion_grid_1280x720.mp4 (1280x720) [2.2 MB] || io_in_motion_grid_1280x720.webm (1280x720) [1.7 MB] || io_in_motion_grid_4096x2304.mp4 (4104x2304) [15.3 MB] || 4104x2304_16x9_30p (4104x2304) [0 Item(s)] || io_in_motion_grid.key [4.3 MB] || io_in_motion_grid.pptx [2.8 MB] || ",
            "hits": 155
        },
        {
            "id": 11692,
            "url": "http://svs.gsfc.nasa.gov/11692/",
            "result_type": "Produced Video",
            "release_date": "2014-12-18T11:00:00-05:00",
            "title": "Young Lava On The Moon",
            "description": "The moon, our companion in space, bears the scars of ancient asteroid impacts and lava flows. Such flows resulted in the large, dark spots on the moon’s surface that we see today. Scientists thought the moon's last volcanoes erupted at least 1 billion years ago. But new observations by NASA's Lunar Reconnaissance Orbiter (LRO) spacecraft have revealed dozens of geologic structures, called irregular mare patches, scattered across the lunar landscape. In these unusual areas, averaging 500 meters in diameter, smooth mounds sit next to blocky terrain. Unlike the rest of the moon, the structures have almost no craters, suggesting that they’re the remnants of recent lava flows that occurred within the last 100 million years. If true, this means the moon could be hotter inside than expected. Watch the video to learn more. || ",
            "hits": 67
        },
        {
            "id": 11685,
            "url": "http://svs.gsfc.nasa.gov/11685/",
            "result_type": "Produced Video",
            "release_date": "2014-11-25T11:00:00-05:00",
            "title": "Cloud Transformation",
            "description": "Volcanoes can spew lava, ash and smoke when they erupt. But even when they aren't erupting, gases can leak from their vents and form tiny particles in the atmosphere known as volcanic aerosols. Although smaller than a human hair, these particles can have a large effect on the properties of nearby clouds. A new study using NASA and European Space Agency satellite data has shown that volcanic aerosols can decrease the size of water droplets that make up clouds. The result may not seem significant, but clouds composed of smaller droplets tend to be brighter and reflect more sunlight back into space. This can affect weather patterns, such as altering winds and where rain falls. Watch the video to learn more. || ",
            "hits": 34
        },
        {
            "id": 11684,
            "url": "http://svs.gsfc.nasa.gov/11684/",
            "result_type": "Produced Video",
            "release_date": "2014-11-20T11:00:00-05:00",
            "title": "The Erupting Peninsula",
            "description": "Explorer Stepan Krasheninnikov first pointed it out in 1755: there may not be another land mass on Earth where so many volcanoes and hot springs are crammed into so little space. Situated along the Pacific Coast of Russia, the Kamchatka Peninsula is part of the Ring of Fire, one of the most geologically active zones on the planet. More than 300 volcanoes dot the peninsula, including 29 active ones. The volcanoes are as diverse—in shape, size, geologic formations, and eruptive styles—as they are numerous. The logistics of maintaining ground-based sensors in this rugged region make satellites a necessity for monitoring the volcanoes. In September 2014, the USGS-NASA Landsat 8 satellite captured six clear images of Kamchatka's often cloudy east coast. The images were stitched into a mosaic, providing a seamless look at five volcanoes with plumes of steam, gas, or ash rising from their summits. Watch the video for a tour of the mosaic. || ",
            "hits": 42
        },
        {
            "id": 10183,
            "url": "http://svs.gsfc.nasa.gov/10183/",
            "result_type": "Produced Video",
            "release_date": "2014-11-13T13:00:00-05:00",
            "title": "How Do Active Volcanoes Change Clouds?",
            "description": "NASA Goddard Space Flight Center scientist Andrew Sayer talks about how emissions from volcanoes can affect clouds.This video provides an overview of research published in the Journal of Atmospheric Chemistry and Physics Research:Systematic satellite observations of the impact of aerosols from passive volcanic degassing on local cloud propertiesJournal of Atmospheric Chemistry and Physics, October 9, 2014 || ",
            "hits": 45
        },
        {
            "id": 10916,
            "url": "http://svs.gsfc.nasa.gov/10916/",
            "result_type": "Produced Video",
            "release_date": "2014-03-06T00:00:00-05:00",
            "title": "Hello Paradise",
            "description": "Depending on your definition, there are 2,000 to 400,000 islands in the world. Some rival the size of continents—Greenland and Indonesia—while others barely stick a kilometer or two of beach out of the sea. Together they shelter unique plant and animal species and nearly 500 million humans. Some islands are formed by volcanism, with molten rock emerging from Earth's interior to build seafloor mountains that eventually rise above the water surface. Others are chunks of continental crust that became surrounded by water when sea levels rose at the end of the last Ice Age. Life itself has created a few, from artificial islands made by humans to sandbar-topped reefs built by corals. With the space station and a fleet of satellites, NASA has seen all of them. Check out the images for a look at five islands viewed from orbit. || ",
            "hits": 37
        },
        {
            "id": 11455,
            "url": "http://svs.gsfc.nasa.gov/11455/",
            "result_type": "Produced Video",
            "release_date": "2014-03-04T00:00:00-05:00",
            "title": "Io Erupts",
            "description": "En route to the icy worlds inhabiting the outer regions of our solar system, NASA’s New Horizons spacecraft zipped past Jupiter, catching Io, the planet’s third-largest moon, enduring a volcanic explosion. Locked in a perpetual tug of war between the imposing gravity of Jupiter and the smaller, consistent pulls of its neighboring moons, Io’s distorted orbit causes it to flex as it swoops around the gas giant. The stretching causes friction and intense heat in Io’s interior, sparking massive eruptions across its surface. Images snapped by the spacecraft’s high-resolution telescopic camera in March 2007 show a 200-mile-high plume spewing from Tvashtar volcano in Io’s northern hemisphere. Watch the video to see it for yourself. || ",
            "hits": 102
        },
        {
            "id": 11446,
            "url": "http://svs.gsfc.nasa.gov/11446/",
            "result_type": "Produced Video",
            "release_date": "2014-01-30T00:00:00-05:00",
            "title": "Spectacular Sarychev",
            "description": "On June 12, 2009, a fortuitous orbit of the International Space Station (ISS) made it possible for an astronaut on board to capture Sarychev Volcano in the early stages of eruption. The volcano is located on the northwestern end of Matua Island, which is part of the Kuril Islands, a chain of 56 islands northeast of Japan. The eruption sent a plume of brown-colored ash and white steam rising into the atmosphere. The plume was so immense that it cast a large shadow on the island. Sarychev is one of the most active volcanoes in the Kuril Island chain. Prior to June 12, the last explosive eruption occurred in 1989, with eruptions in 1986, 1976, 1954, and 1946 also producing lava flows. Watch the video to see how the eruption looked from space. || ",
            "hits": 69
        },
        {
            "id": 30476,
            "url": "http://svs.gsfc.nasa.gov/30476/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-11-01T15:00:00-04:00",
            "title": "Mount Etna",
            "description": "Twin volcanic plumes—one of ash, one of gas—rose from Sicily’s Mount Etna on the morning of October 26, 2013. L’Istituto Nazionale di Geofisica e Vulcanologia (INGV) Osservatorio Etneo (National Institute of Geophysics and Volcanology Etna Observatory) reported that Etna was experiencing its first paroxysm in six months. Multiple eruption columns are common at Etna, a result of complex plumbing within the volcano. The Northeast Crater, one of several on Etna’s summit, was emitting the ash column, while the New Southeast Crater was simultaneously venting mostly gas.This natural-color image collected by Landsat 8 shows the view from space at 11:38 a.m. local time. The towering, gas-rich plume cast a dark shadow over the lower, ash-rich plume and Etna’s northwestern flank. Relatively fresh lava flows (less than a century or so old) are dark gray; vegetation is green; and the tile-roofed buildings of Bronte and Biancavilla lend the towns an ochre hue. || ",
            "hits": 34
        },
        {
            "id": 30307,
            "url": "http://svs.gsfc.nasa.gov/30307/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-21T12:00:00-04:00",
            "title": "Iceland Volcano Eruption Eyjafjallajökull",
            "description": "Iceland’s Eyjafjallajökull Volcano produced its second major ash plume of 2010 beginning on May 7. When the first ash eruption began on April 14, air travel across most of Europe was shut down, but by the time of the second eruption, forecasters were better prepared to predict the spread of volcanic ash. Despite some airport closures and flight cancellations, most air passengers completed their journeys with minimal delay.Among the key pieces of information that a computer model must have to predict the spread of ash is when the eruption happened, how much ash was ejected, and how high the plume got. The Multi-angle Imaging SpectroRadiometer (MISR) aboard NASA’s Terra satellite collected data on ash height when it passed just east of the Eyjafjallajökull Volcano mid-morning on May 7. || ",
            "hits": 39
        },
        {
            "id": 30308,
            "url": "http://svs.gsfc.nasa.gov/30308/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-21T12:00:00-04:00",
            "title": "Puyehue-Cordon Caulle Volcanic Complex, Chile",
            "description": "On June 4, 2011, a fissure opened in Chile's Puyehue-CordÃ³n Caulle Volcanic Complex, sending ash 45,000 feet (14,000 meters) into the air. This image, taken on June 11, 2011, shows the path of the volcanic ash plume. Winds blowing from the west carried the plume downwind, across Argentina and eventually reaching the South Atlantic Ocean. Clear skies allow the snow-covered Andes Mountains to be seen just north and south of the erupting volcano. The opposite is true for areas downwind of the volcano beneath the highest concentrations of volcanic ash. It is hard for even the tiniest bit of sunlight to penetrate the thick plume as revealed by the dark shadow cast on the earth's surface directly south of the plume. The width of the plume increases with increasing distance from the volcano as particulates disperse in the atmosphere. The zigzag path of the plume over Argentina suggests shifts in wind direction. East of the Andes, heavier volcanic ash sediment has settled on the land below, blanketing large portions of Argentina. It appears that some of the settled ash has been picked up again, this time by surface winds that may eventually carry the sediment out to sea. A high resolution image acquired 6 weeks later  shows ash covering the mountain slopes and pumice floating in lakes. || ",
            "hits": 46
        },
        {
            "id": 30336,
            "url": "http://svs.gsfc.nasa.gov/30336/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-21T12:00:00-04:00",
            "title": "Exploring Mars",
            "description": "Since our first close-up picture of Mars in 1965, spacecraft voyages to the Red Planet have revealed a world strangely familiar, yet different enough to challenge our perceptions of what makes a planet work. Every time we feel close to understanding Mars, new discoveries send us straight back to the drawing board.Over the past several decades, spacecraft have shown us that Mars is rocky, cold, and desolate beneath its hazy, pink sky. We've discovered that today's Martian wasteland hints at a formerly volatile world where volcanoes once raged and flash floods rushed over the land.Among our many discoveries about Mars, one stands out above all others: the evidence for past surface water on Mars. Water is key because almost everywhere we find water on Earth, we find life. With our robotic spacecraft, we've found evidence that liquid water once flowed in ancient Martian environments that could have supported microbial life. Armed with that knowledge, we now can seek signs of whether such life actually arose. Is there any evidence of life in the planet's past? If so, could any of these tiny living creatures still exist today? Imagine how exciting it would be to answer, \"Yes!!\" || ",
            "hits": 66
        },
        {
            "id": 30338,
            "url": "http://svs.gsfc.nasa.gov/30338/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-21T12:00:00-04:00",
            "title": "Rotating Mars",
            "description": "Since our first close-up picture of Mars in 1965, spacecraft voyages to the Red Planet have revealed a world strangely familiar, yet different enough to challenge our perceptions of what makes a planet work. Every time we feel close to understanding Mars, new discoveries send us straight back to the drawing board. Over the past several decades, spacecraft have shown us that Mars is rocky, cold, and desolate beneath its hazy, pink sky. We've discovered that today's Martian wasteland hints at a formerly volatile world where volcanoes once raged and flash floods rushed over the land. Among our many discoveries about Mars, one stands out above all others: the evidence for past surface water on Mars. Water is key because almost everywhere we find water on Earth, we find life. With our robotic spacecraft, we've found evidence that liquid water once flowed in ancient Martian environments that could have supported microbial life. Armed with that knowledge, we now can seek signs of whether such life actually arose. Is there any evidence of life in the planet's past? If so, could any of these tiny living creatures still exist today? Imagine how exciting it would be to answer, \"Yes!!\" || ",
            "hits": 138
        },
        {
            "id": 30188,
            "url": "http://svs.gsfc.nasa.gov/30188/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-17T12:00:00-04:00",
            "title": "Mount Etna Deformation",
            "description": "This animation depicts a time-series of ground deformation at Mount Etna Volcano between 1992 and 2001. The deformation results from changes in the volume of a shallow chamber centered approximately 5 km (3 miles) below sea level. The accumulation of magma in this chamber results in the inflation, or expansion, of the volcano, while the release of magma from the chamber results in deflation or contraction. || ",
            "hits": 41
        },
        {
            "id": 30189,
            "url": "http://svs.gsfc.nasa.gov/30189/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-17T12:00:00-04:00",
            "title": "Simulated Flight over Mount Rainier",
            "description": "This simulated flight combines radar topography and visible images of Mount Rainier in Washington state. The volcano last erupted about 150 years ago and numerous large floods and debris flows have originated on its slopes during the last century. Today the volcano is heavily mantled with glaciers and snowfields. More than 100,000 people live on young volcanic mudflows less than 10,000 years old and, consequently, are within the range of future, devastating mudslides. || ",
            "hits": 22
        },
        {
            "id": 11304,
            "url": "http://svs.gsfc.nasa.gov/11304/",
            "result_type": "Produced Video",
            "release_date": "2013-07-08T07:00:00-04:00",
            "title": "Planetary Scientist Profile: Brent Garry",
            "description": "NASA Geologist Brent Garry discusses his work studying volcanoes and lava flows on the Earth, the Moon, and Mars. || ",
            "hits": 49
        },
        {
            "id": 11249,
            "url": "http://svs.gsfc.nasa.gov/11249/",
            "result_type": "Produced Video",
            "release_date": "2013-05-15T11:00:00-04:00",
            "title": "Landsat 8 Long Swath",
            "description": "After two months of on-orbit testing and calibration, Landsat 8 (previously called LDCM) fired its propulsion system on April 12, 2013, and ascended to its final orbit 438 miles (705 km) above Earth. The animation, made from scenes taken a week later on April 19, allows viewers to fly with the satellite from its final operating orbit. 56 continuous Landsat scenes from that orbit have been stitched together into a seamless view from Russia to South Africa. Orbiting at 16,800 mph (27,000 kph), Landsat 8 made this flight in just more than 20 minutes. The animation moves faster, covering 5,665 miles (9,117 kilometers) in nearly 16 minutes. You would have to be moving about 21,930 mph (35,290 kph) to get a similar view — only slightly slower than the Apollo astronauts who entered Earth's orbit from the moon at 25,000 mph (40,200 kph). We pan down the long swath of data from Landsat 8, starting in northern Russia, passing over the Caucasus Mountains, the Republic of Georgia, Armenia, Turkey (passing Lake Van), Iraq, and Saudi Arabia (the cities of Medina and Jeddah), crossing the Red Sea into Eritrea, Ethiopia, the Kenya-Uganda border and catching the eastern edge of Lake Victoria, Tanzania, Zimbabwe, a little bit of Mozambique, and ending in northern South Africa. || ",
            "hits": 66
        },
        {
            "id": 30017,
            "url": "http://svs.gsfc.nasa.gov/30017/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-03-07T00:00:00-05:00",
            "title": "GEOS-5 Nature Run Collection",
            "description": "Through numerical experiments that simulate the dynamical and physical processes governing weather and climate variability of Earth's atmosphere, models create a dynamic portrait of our planet. This 10-kilometer global mesoscale simulation (Nature Run) using the NASA Goddard Earth Observing System Model (GEOS-5) explores the evolution of surface temperatures as the sun heats the Earth and fuels cloud formation in the tropics and along baroclinic zones; the presence of water vapor and precipitation within these global weather patterns; the dispersion of global aerosols from dust, biomass burning, fossil fuel emissions, and volcanoes; and the winds that transport these aerosols from the surface to upper-levels.The full GEOS-5 simulation covered 2 years—from May 2005 to May 2007. It ran on 3,750 processors of the Discover supercomputer at the NASA Center for Climate Simulation, consuming 3 million processor hours and producing over 400 terabytes of data. GEOS-5 development is funded by NASA's Modeling, Analysis, and Prediction Program. || ",
            "hits": 159
        },
        {
            "id": 11171,
            "url": "http://svs.gsfc.nasa.gov/11171/",
            "result_type": "Produced Video",
            "release_date": "2013-01-15T00:00:00-05:00",
            "title": "Nature's Night Lights",
            "description": "\"The night is nowhere near as dark as most of us think. In fact, the Earth is never really dark,\" says scientist Steven Miller of Colorado State University. Auroras dance across the skies. Wildfires and volcanoes rage. Moonlight and starlight reflect off water, snow, clouds and deserts. The night-imaging capability of the NASA-NOAA Suomi National Polar-orbiting Partnership satellite is capturing all of this, giving scientists like Miller a new way to see storms and weather patterns, atmospheric waves and other dynamic events that don't stop at sundown. \"For all the reasons that we need to see the Earth during the day, we also need to see the Earth at night,\" says Miller. \"The Earth never sleeps; it's constantly moving, evolving, building up here and tearing down there.\" Watch the video to see different views of the Persian Gulf region in the changing light of the moon. || ",
            "hits": 22
        },
        {
            "id": 11113,
            "url": "http://svs.gsfc.nasa.gov/11113/",
            "result_type": "Produced Video",
            "release_date": "2012-10-17T09:00:00-04:00",
            "title": "Planetary Scientist Profile: Lynn Carter",
            "description": "NASA scientist Lynn Carter talks about her work in the Planetary Geodynamics Laboratory. || ",
            "hits": 39
        },
        {
            "id": 10977,
            "url": "http://svs.gsfc.nasa.gov/10977/",
            "result_type": "Produced Video",
            "release_date": "2012-05-24T00:00:00-04:00",
            "title": "Paint By Particle",
            "description": "Satellites, balloon-borne instruments and ground-based devices make 30 million observations of the atmosphere each day. Yet these measurements still give an incomplete picture of the complex interactions within the membrane surrounding Earth. Enter climate models. Through mathematical experiments, modelers can move Earth forward or backward in time to create a dynamic portrait of the planet. Researchers from NASA Goddard's Global Modeling and Assimilation Office recently ran a simulation of the atmosphere that captured how winds whip aerosols around the world. Such simulations allow scientists to better understand how these tiny particulates travel in the atmosphere and influence weather and climate. In the visualization below, covering August 2006 to April 2007, watch as dust and sea salt swirl inside cyclones, carbon bursts from fires, sulfate streams from volcanoes—and see how these aerosols paint the modeled world. || ",
            "hits": 54
        },
        {
            "id": 10904,
            "url": "http://svs.gsfc.nasa.gov/10904/",
            "result_type": "Produced Video",
            "release_date": "2012-02-14T00:00:00-05:00",
            "title": "Love's Terrain",
            "description": "Over centuries, the planet second closest to the sun was known by many names: Ishtar, Ouaiti, Hesperus, Aphrodite. But just as with the heart's memory one name prevails. In honor of Valentine's Day, homage is paid to the celestial sphere that personifies the mythological goddess of love and beauty—Venus. Of all the planets in our solar system Venus is nearest in size to Earth, though its dry rocky landscape is much hotter. Processed images of the surface using data collected by instruments onboard NASA's Magellan spacecraft reveal vast plains intermixed with sloping highlands and ancient volcanoes. These features are highlighted on a rotating globe of Venus in the color-coded visualization below, where high elevation terrain is shaded yellow and red with low elevation regions tinted blue and green. Black gaps represent areas of the planet uncharted during the first mapping cycle made by Magellan, which surveyed Venus over a period of four years beginning in 1990. || ",
            "hits": 107
        },
        {
            "id": 30187,
            "url": "http://svs.gsfc.nasa.gov/30187/",
            "result_type": "Hyperwall Visual",
            "release_date": "2012-02-06T12:00:00-05:00",
            "title": "Kilauea Volcanic Flow",
            "description": "This animation, which depicts the growth of the Kamoamoa Flow Field, Kilauea Volcano, Hawaii, was generated from a sequence of ten multispectral images acquired between September 3 and 17, 1995. During this time period lava flows breaking out above the Paluma Pali (or cliff), at an elevation of 480 meters, completed the 5 kilometer journey to the Pacific Ocean.To visualize the progress of the lava flows, infrared images of the flows were superimposed over a common true-color background image. The colors of the lava flows are a function of temperature: the hottest temperatures are displayed in bright yellow, intermediate temperatures grade from bright red to orange, and the coolest temperatures are displayed in dark orange and brown. Image-morphing techniques were used to approximate the shape and position of the flows at 30-min intervals over the 14-day period. Finally, the morphed images were superimposed over a digital elevation model (DEM) and rendered as 3-D perspective views of the flow field. || ",
            "hits": 39
        },
        {
            "id": 3896,
            "url": "http://svs.gsfc.nasa.gov/3896/",
            "result_type": "Visualization",
            "release_date": "2011-12-28T00:00:00-05:00",
            "title": "Mars Roll",
            "description": "A redux of entry #2455 using MGS/MOLA data for the Martian topography and MGS/MOC for the Martian surface color. The animation rolls Mars to show major features of the Martian topography. Major features depicted include: Olympus Mons, Valles Marineris, Hellas Basin, and the Martian North and South Poles. || ",
            "hits": 82
        },
        {
            "id": 10741,
            "url": "http://svs.gsfc.nasa.gov/10741/",
            "result_type": "Produced Video",
            "release_date": "2011-03-30T00:00:00-04:00",
            "title": "Planetary Science: Astrogeology Profiles",
            "description": "Meet some of the people in NASA Goddard's Planetary Science division. || ",
            "hits": 50
        },
        {
            "id": 10621,
            "url": "http://svs.gsfc.nasa.gov/10621/",
            "result_type": "Produced Video",
            "release_date": "2010-09-17T18:00:00-04:00",
            "title": "Robots on the Roof",
            "description": "The Aerosol Robotic Network (AERONET) is one of the first places that scientists turn when volcanoes, wildfires, pollution plumes, dust storms and many other phenomena-both natural and manmade-make an appearance. The network of ground-based instruments, called sun photometers, measures the many tiny particles blowing about in the atmosphere called aerosols. The particles are often impossible to see with human eyes, but AERONET's sensors can detect their presence by measuring subtle fluctuations in sunlight as the particles reflect and scatter the sun's rays. || ",
            "hits": 30
        },
        {
            "id": 10550,
            "url": "http://svs.gsfc.nasa.gov/10550/",
            "result_type": "Produced Video",
            "release_date": "2010-05-18T00:00:00-04:00",
            "title": "Forest Recovering From Mount St. Helens Eruption",
            "description": "The 1980 Mount Saint Helens eruption was one of the most significant natural disasters in the US in the past half-century. The eruption laid waste to 230 square miles. Landsat captured the extent of the destruction, with grey tones revealing widespread lava flows and ash deposits. Subsequent Landsat images over the years show the spread of vegetation recovery across the site. || ",
            "hits": 76
        },
        {
            "id": 10398,
            "url": "http://svs.gsfc.nasa.gov/10398/",
            "result_type": "Produced Video",
            "release_date": "2009-02-20T00:00:00-05:00",
            "title": "USGS Video of a Hawaiian Volcano",
            "description": "Aerosols smaller than 1 micrometer are mostly formed by condensation processes such as conversion of sulfur dioxide (SO2) gas (released from volcanic eruptions) to sulfate particles and by formation of soot and smoke during burning processes. After formation, the aerosols are mixed and transported by atmospheric motions and are primarily removed by cloud and precipitation processes. Video courtesy of United States Geological Survey. || ",
            "hits": 53
        },
        {
            "id": 10392,
            "url": "http://svs.gsfc.nasa.gov/10392/",
            "result_type": "Produced Video",
            "release_date": "2009-02-19T00:00:00-05:00",
            "title": "Volcanic Ash Still Image",
            "description": "Aerosols are complex particles; they can occur in nature but can also be generated by humans. One source of naturally-occurring aerosols is volcanoes. Large-scale volcanic activity may last only a few days, but the massive outpouring of gases and ash can influence climate patterns for years. Sulfuric gases convert to sulfate aerosols, sub-micron droplets containing about 75 percent sulfuric acid. Following eruptions, these aerosol particles can linger as long as three to four years in the stratosphere. Still image courtesy of United States Geological Survey. || ",
            "hits": 46
        },
        {
            "id": 10364,
            "url": "http://svs.gsfc.nasa.gov/10364/",
            "result_type": "Produced Video",
            "release_date": "2009-02-01T00:00:00-05:00",
            "title": "NOAA-N Prime Mission Overview",
            "description": "The NOAA-N Prime satellite is slated for launch by NASA on February 4th, 2009. Operated by NOAA, N Prime will be the last in the Television Infrared Observation Satellite Series (TIROS) that have been observing Earth's weather and environment for nearly 50 years. N Prime's main role will be to provide continuity of service until the launch of the next generation, highly advanced National Polar-orbiting Operational Environmental Satellite System (NPOESS). || ",
            "hits": 54
        },
        {
            "id": 20178,
            "url": "http://svs.gsfc.nasa.gov/20178/",
            "result_type": "Animation",
            "release_date": "2009-01-21T12:00:00-05:00",
            "title": "NOAA-N Prime Beauty Shot Animation",
            "description": "An artist concept of the spacecraft. The microwave instruments on board NOAA-N Prime are so sensitive that they can see Earth's surface through clouds. NOAA-N Prime will deliver essential atmospheric and surface parameters to use in scientific forecast models. N Prime provides essential critical information for creating accurate weather forecasts 2-3 days in advance. || ",
            "hits": 36
        },
        {
            "id": 10372,
            "url": "http://svs.gsfc.nasa.gov/10372/",
            "result_type": "Produced Video",
            "release_date": "2009-01-21T00:00:00-05:00",
            "title": "NOAA-N Prime and GOES-O in Orbit Animation",
            "description": "Since 1960, NOAA has operated a fleet of Polar-orbiting Environmental Satellites called POES, complimented by the higher altitude (36,000km) Geostationary Operational Environmental Satellites (GOES). The stationary GOES satellites give a constant view from two points in space, while the polar-orbiting NOAA-N Prime circles the Earth at a lower altitude (860km) once every 102 minutes. These two systems provide continuous data about the global atmosphere. || ",
            "hits": 44
        },
        {
            "id": 3169,
            "url": "http://svs.gsfc.nasa.gov/3169/",
            "result_type": "Visualization",
            "release_date": "2005-06-01T12:00:00-04:00",
            "title": "Sulfur Dioxide from the Mount Pinatubo Volcanic Eruption, 1991 (WMS)",
            "description": "This animation shows levels of sulfur dioxide in the atmosphere after the volcanic eruption of Mt. Pinatubo in the Philippines.This product is available through our Web Map Service. || background-bluemarble-equatorial.png (1024x256) [226.3 KB] || pinatubo_so2-thm.png (80x40) [3.9 KB] || pinatubo_so2-pre.png (320x160) [39.3 KB] || pinatubo_so2-pre_searchweb.png (320x180) [39.6 KB] || pinatubo_so2.webmhd.webm (960x540) [173.9 KB] || 1024x256 (1024x256) [4.0 KB] || pinatubo_so2.m2v (1024x256) [4.8 MB] || a003169_pinatubo_so2.mp4 (640x160) [987.3 KB] || ",
            "hits": 67
        },
        {
            "id": 3116,
            "url": "http://svs.gsfc.nasa.gov/3116/",
            "result_type": "Visualization",
            "release_date": "2005-03-02T12:00:00-05:00",
            "title": "Mount St. Helens Before, During, and After (WMS)",
            "description": "Mount St. Helens erupted on May 18, 1980, devastating more than 150 square miles of forest in southwestern Washington state. This animation shows Landsat images of the Mount St. Helens area in 1973, 1983, and 2000, illustrating the destruction and regrowth of the forest. The 1983 image clearly shows the new crater on the northern slope where the eruption occurred, the rivers and lakes covered with ash, and the regions of deforestation. The 2000 image, taken twenty years after the eruption, still shows the changed crater, but much of the devastated area is covered by new vegetation growth. || ",
            "hits": 99
        },
        {
            "id": 2908,
            "url": "http://svs.gsfc.nasa.gov/2908/",
            "result_type": "Visualization",
            "release_date": "2004-06-23T18:00:00-04:00",
            "title": "Volcano Activity from 1960 through 1995 (WMS)",
            "description": "This animation represents cumulative global volcanic activity over a 36-year span, from 1960 through 1995. Volcanoes occur near but not on tectonic plate boundaries. If a plate boundary is a convergent boundary, where one plate is subducting under another, then volcanoes occur on the top plate, over the area where rock from the subducting plate has melted, is rising, and has broken through to the surface. The Mt. St. Helens eruption is visible in this animation starting in March, 1980. || ",
            "hits": 56
        },
        {
            "id": 2864,
            "url": "http://svs.gsfc.nasa.gov/2864/",
            "result_type": "Visualization",
            "release_date": "2004-04-22T12:00:00-04:00",
            "title": "Earth-Mars Volcano Comparisons: Final Composite",
            "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, still dwarfs Earth's Mauna Loa, Hawaii volcano. When measured from the ocean floor, Mauna Loa is 10km. high compared to Olympus Mons at 23km. This post-produced animation composite was created using various elements from animations #2865 through #2872. || ",
            "hits": 63
        },
        {
            "id": 2865,
            "url": "http://svs.gsfc.nasa.gov/2865/",
            "result_type": "Visualization",
            "release_date": "2004-04-22T12:00:00-04:00",
            "title": "Earth-Mars Volcano Comparisons: True Color Earth",
            "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, still dwarfs Earth's Mauna Loa, Hawaii volcano. When measured from the ocean floor, Mauna Loa is 10km. high compared to Olympus Mons at 23km. This animation is one element of the Earth-Mars comparison, showing Earth in its true color beauty. This animation is match-framed to animations #2864 through #2872. || ",
            "hits": 50
        },
        {
            "id": 2866,
            "url": "http://svs.gsfc.nasa.gov/2866/",
            "result_type": "Visualization",
            "release_date": "2004-04-22T12:00:00-04:00",
            "title": "Earth-Mars Volcano Comparisons: Earth with Elevation Color Map",
            "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, dwarfs Earth's Mauna Loa, Hawaii volcano. When measured from the ocean floor, Mauna Loa is approximately 10km. high compared to Olympus Mons at 23km. This animation is one element of the Earth-Mars comparison, showing a bare Earth (no oceans) via an elevation color map. This color map is the same one used to map Mars in Animation #2868. Instead of using sea level as zero (i.e., yellow) we use Earth's mean elevation which is approximately 1 km. below sea level. We then map the higher elevations in greens, reds, and white at the highest peaks, and blue and purple are used for the low lying areas. This animation is match-framed to animations #2864 through #2872. || ",
            "hits": 61
        },
        {
            "id": 2867,
            "url": "http://svs.gsfc.nasa.gov/2867/",
            "result_type": "Visualization",
            "release_date": "2004-04-22T12:00:00-04:00",
            "title": "Earth-Mars Volcano Comparisons: Elevation color-mapped Earth with True Color Land",
            "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, dwarfs Earth's Mauna Loa, Hawaii volcano. When measured from the ocean floor, Mauna Loa is approximately 10km. high compared to Olympus Mons at 23km. This animation is one element of the Earth-Mars comparison. It shows ocean bathymetry via an elevation color map (greens, blues, and purples indicate deeper ocean depths respectively) along with true color land (everything above sea level). This animation is match-framed to animations #2864 through #2872. || ",
            "hits": 56
        },
        {
            "id": 2868,
            "url": "http://svs.gsfc.nasa.gov/2868/",
            "result_type": "Visualization",
            "release_date": "2004-04-22T12:00:00-04:00",
            "title": "Earth-Mars Volcano Comparisons: True Color Mars",
            "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, dwarfs Earth's Mauna Loa, Hawaii volcano. When measured from the ocean floor, Mauna Loa is approximately 10km. high compared to Olympus Mons at 23km. This animation is one element of the Earth-Mars comparison, showing Mars in it's true color beauty. The beginning of this animation is match-framed to animations #2864 through #2872. || ",
            "hits": 70
        },
        {
            "id": 2869,
            "url": "http://svs.gsfc.nasa.gov/2869/",
            "result_type": "Visualization",
            "release_date": "2004-04-22T12:00:00-04:00",
            "title": "Earth-Mars Volcano Comparisons: Elevation Color-Mapped Mars",
            "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, dwarfs Earth's Mauna Loa, Hawaii volcano.  When measured from the ocean floor, Mauna Loa is approximately 10km. high compared to Olympus Mons at 23km.  This animation is one element of the Earth-Mars comparison.  It shows Mars' differing terrain via an elevation color map.  Yellow indicates the mean elevation.  Green, blue, and purple are low lying areas.  Red, brown, and white are the highest elevations.  This animation is match-framed to animations #2864 through #2872 and uses the same color map as animation #2866. || ",
            "hits": 94
        },
        {
            "id": 2870,
            "url": "http://svs.gsfc.nasa.gov/2870/",
            "result_type": "Visualization",
            "release_date": "2004-04-22T12:00:00-04:00",
            "title": "Earth-Mars Volcano Comparisons: True Color Olympus Mons over Elevation Color-Mapped Earth Bathymetry with True Color Land Features",
            "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, dwarfs Earth's Mauna Loa, Hawaii volcano. When measured from the ocean floor, Mauna Loa is approximately 10km. high compared to Olympus Mons at 23km. In this animation, Olympus Mons obstructs the view of Mauna Loa, but gives the viewer a good perspective of the overall size of this giant volcano. This animation is match-framed to animations #2864 through #2872. || ",
            "hits": 75
        },
        {
            "id": 2871,
            "url": "http://svs.gsfc.nasa.gov/2871/",
            "result_type": "Visualization",
            "release_date": "2004-04-22T12:00:00-04:00",
            "title": "Earth-Mars Volcano Comparisons: Transparent Olympus Mons over Elevation Color-Mapped Earth with True Color Land",
            "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, dwarfs Earth's Mauna Loa, Hawaii volcano. When measured from the ocean floor, Mauna Loa is approximately 10km. high compared to Olympus Mons at 23km. In this animation, a transparent Olympus Mons is juxtaposed over Mauna Loa, allowing the viewer to better see the size differences between these land masses. This animation is match-framed to animations #2864 through #2872. || ",
            "hits": 71
        },
        {
            "id": 2872,
            "url": "http://svs.gsfc.nasa.gov/2872/",
            "result_type": "Visualization",
            "release_date": "2004-04-22T12:00:00-04:00",
            "title": "Earth-Mars Volcano Comparisons: Mars Inside a Transparent Earth",
            "description": "Despite the 2:1 relative size difference between Earth and Mars, the Martian volcano, Olympus Mons, dwarfs Earth's Mauna Loa, Hawaii volcano. When measured from the ocean floor, Mauna Loa is approximately 10km. high compared to Olympus Mons at 23km. This animation not only shows the relative size differences between Mauna Loa and Olympus Mons, but also shows the size difference between these 2 planets. The equatorial radius of Mars is approximately 3397 km. compared to Earth's equatorial radius of 6378.1 km. This animation is match-framed to animations #2864 through #2872. || ",
            "hits": 62
        },
        {
            "id": 2877,
            "url": "http://svs.gsfc.nasa.gov/2877/",
            "result_type": "Visualization",
            "release_date": "2004-04-22T12:00:00-04:00",
            "title": "Earth-Mars Planet Comparisons (False Color with Axes and Orbit Plane)",
            "description": "This is a visualization showing the relative size of Mars compared to that of Earth. This version uses false color textures (there are corresponding true color versions as well). The colors correspond to the heights above/below 'sea level.' This version also includes pole axes and an orbit plane. || ",
            "hits": 64
        },
        {
            "id": 2878,
            "url": "http://svs.gsfc.nasa.gov/2878/",
            "result_type": "Visualization",
            "release_date": "2004-04-22T12:00:00-04:00",
            "title": "Earth-Mars Planet Comparisons (True Color)",
            "description": "This is a visualization showing the relative size of Mars compared to that of Earth. This version uses true color textures (there are corresponding false color versions as well). || ",
            "hits": 121
        },
        {
            "id": 2879,
            "url": "http://svs.gsfc.nasa.gov/2879/",
            "result_type": "Visualization",
            "release_date": "2004-04-22T12:00:00-04:00",
            "title": "Earth-Mars Planet Comparisons (True Color with Axes and Orbit Plane)",
            "description": "This is a visualization showing the relative size of Mars compared to that of Earth. This version uses true color textures (there are corresponding false color versions as well) and includes pole axes and and orbit plane. || ",
            "hits": 96
        },
        {
            "id": 2883,
            "url": "http://svs.gsfc.nasa.gov/2883/",
            "result_type": "Visualization",
            "release_date": "2004-01-16T12:00:00-05:00",
            "title": "Mars: Olympus Mons",
            "description": "MOLA-based still image showing Martian topography of Olympus Mons as both color and elevation. || Olympus Mons on Mars, in false color || olympus_mons_false.jpg (1280x1024) [260.9 KB] || olympus_mons_false_web.jpg (320x256) [13.9 KB] || olympus_mons_false_thm.png (80x40) [4.8 KB] || olympus_mons_false_web_searchweb.jpg (320x180) [84.0 KB] || olympus_mons_false.tif (1280x1024) [1.9 MB] || ",
            "hits": 109
        },
        {
            "id": 2428,
            "url": "http://svs.gsfc.nasa.gov/2428/",
            "result_type": "Visualization",
            "release_date": "2002-04-16T12:00:00-04:00",
            "title": "MOLA-based Flyover of Tharsis Volcanos",
            "description": "MOLA-based animations showing Martian topography as both color and elevation.  The exaggeration is 3x.  This was created for a talk James Garvin will give on The Hill in late April 2002. || ",
            "hits": 22
        },
        {
            "id": 2410,
            "url": "http://svs.gsfc.nasa.gov/2410/",
            "result_type": "Visualization",
            "release_date": "2002-03-14T12:00:00-05:00",
            "title": "Farallon Plate Remnants",
            "description": "The Rockies are fifteen hundred kilometers, or one thousand miles, to the east. The cause must be the tectonic plate that built these mountains. Its name is Farallon. Farallon started off normally enough. It plunged beneath the North American Plate at a forty-five degree angle. This process sprouted volcanoes to form the Sierra Nevada in what is now California.  Next, mantle motions pulled North America westward over Farallon, and the plate scraped along the bottom of the continent - for fifteen hundred kilometers.  As North America continued its westward trek, Farallon settled to the bottom of the mantle.The image is output from a model run using the TERRA mantle software. To learn more about Bunge's work, visit his web site at: http://www.geophysik.uni-muenchen.de/Members/bunge. || ",
            "hits": 45
        },
        {
            "id": 2089,
            "url": "http://svs.gsfc.nasa.gov/2089/",
            "result_type": "Visualization",
            "release_date": "2001-03-27T12:00:00-05:00",
            "title": "Views of Mars with MOLA and Viking data",
            "description": "These views of Mars were generated for the National Geographic Society as reference materials for their February 2001 'Mars Revealed' poster. || View looking into Chryse Plantia from the west || chryseA0010.jpg (640x480) [47.5 KB] || chryseA0010_web.jpg (320x240) [8.2 KB] || chryseA0010.tif (640x480) [301.0 KB] || View looking into Chryse Plantia from the west || chryseA0011.jpg (640x480) [55.1 KB] || chryseA0011_web.jpg (320x240) [9.1 KB] || chryseA0011.tif (640x480) [382.3 KB] || ",
            "hits": 11
        }
    ]
}