{ "count": 25, "next": null, "previous": null, "results": [ { "id": 5373, "url": "https://svs.gsfc.nasa.gov/5373/", "result_type": "Visualization", "release_date": "2024-09-03T13:00:00-04:00", "title": "PREFIRE First Light", "description": "Visualization emphasizing two passes of PREFIRE over Greenland. Information about the rates of atmospheric emission can be derived from the change in emission at the intersection of the passes. || prefire_first_light_FINAL_2160p30.00450_print.jpg (1024x576) [224.8 KB] || prefire_first_light_FINAL_2160p30.00450_thm.png (80x40) [6.3 KB] || prefire_first_light_FINAL_2160p30.00450_searchweb.png (320x180) [78.7 KB] || prefire_first_light_FINAL [0 Item(s)] || prefire_first_light_FINAL_1080p30.mp4 (1920x1080) [47.2 MB] || prefire_first_light_FINAL_4K [0 Item(s)] || prefire_first_light_FINAL_2160p30.mp4 (3840x2160) [133.7 MB] || prefire_first_light_FINAL_2160p30.mp4.hwshow [199 bytes] || ", "hits": 136 }, { "id": 14086, "url": "https://svs.gsfc.nasa.gov/14086/", "result_type": "Produced Video", "release_date": "2022-02-10T13:00:00-05:00", "title": "Landsat 9 Data Release", "description": "The data from Landsat 9 is available for anyone to download from the USGS data archive. Launched on Sept. 27, 2021, the new satellite and its instruments went through testing and calibration by the mission team. Now, with both Landsat 9 and Landsat 8 in orbit, there will be high-quality, medium-resolution images of Earth’s landscapes and coastal regions every eight days.Music: Amazing Discoveries by Damien Deshayes [SACEM], published by KTSA Publishing [SACEM] available from Universal Production Music; The Troubleshooter by Anders Johan Greger Lewen [STIM], published by Primetime Productions, Ltd [PRS]; Bright Patterns by Gregg Lehrman [ASCAP] and John Christopher Nye [ASCAP], published by Soundcast Music [SESAC]Complete transcript available.Watch this video on the NASA Goddard YouTube channel. || 14086_Landsat9_data-print.jpg (1920x1080) [626.5 KB] || 14086_Landsat9_data-print_searchweb.png (320x180) [53.8 KB] || 14086_Landsat9_data-print_thm.png (80x40) [4.7 KB] || 14086_Landsat9_data_MASTER-pr.mov (1920x1080) [3.1 GB] || 14086_Landsat9_data-yt.mp4 (1920x1080) [369.6 MB] || 14086_Landsat9_data-tw.mp4 (1920x1080) [50.5 MB] || 14086_Landsat9_data-yt.webm (1920x1080) [25.2 MB] || 14086_Landsat9_data.en_US.srt [4.9 KB] || 14086_Landsat9_data.en_US.vtt [4.7 KB] || ", "hits": 154 }, { "id": 13292, "url": "https://svs.gsfc.nasa.gov/13292/", "result_type": "Produced Video", "release_date": "2019-08-23T15:00:00-04:00", "title": "TIRS-2 Ready For Integration", "description": "The Thermal Infrared Sensor 2 (TIRS-2) has passed its tests at NASA's Goddard Space Flight Center and traveled across the country to be integrated onto Landsat 9.Music: Last Outpost by Lennert Busch [PRS], published by Sound Pocket Music [PRS]Complete transcript available.Watch this video on the NASA Goddard YouTube channel. || TIRS-2_shipping_20190813-28_print.jpg (1024x576) [83.4 KB] || TIRS-2_shipping_20190813-28.png (3840x2160) [10.7 MB] || TIRS-2_shipping_20190813-28_searchweb.png (320x180) [82.4 KB] || TIRS-2_shipping_20190813-28_thm.png (80x40) [5.8 KB] || 13292_TIRS-2_Ships_MASTER_V3.mov (1920x1080) [2.6 GB] || 13292_TIRS-2_Ships.mp4 (1920x1080) [160.5 MB] || 13292_TIRS-2_Ships_MASTER_V3_facebook_720.mp4 (1280x720) [91.2 MB] || 13292_TIRS-2_Ships_MASTER_V3.webm (960x540) [33.0 MB] || 13292_TIRS-2_Ships-captions.en_US.srt [1.2 KB] || 13292_TIRS-2_Ships-captions.en_US.vtt [1.2 KB] || ", "hits": 49 }, { "id": 30979, "url": "https://svs.gsfc.nasa.gov/30979/", "result_type": "Hyperwall Visual", "release_date": "2018-07-31T00:00:00-04:00", "title": "ECOSTRESS Installation and First Data", "description": "The first light image from ECOSTRESS, showing the Nile river valley. || ecostress_first_light_PIA22590.png (1920x1080) [1.3 MB] || ecostress_first_light_PIA22590_print.jpg (1024x576) [99.0 KB] || ecostress_first_light_PIA22590_searchweb.png (320x180) [55.4 KB] || ecostress_first_light_PIA22590_thm.png (80x40) [4.5 KB] || ecostress_first_light_PIA22590.hwshow [228 bytes] || ", "hits": 165 }, { "id": 30911, "url": "https://svs.gsfc.nasa.gov/30911/", "result_type": "Hyperwall Visual", "release_date": "2017-11-13T00:00:00-05:00", "title": "2017 North Atlantic Hurricane Season Simulation", "description": "GEOs model run showing 2017 Atlantic hurricane season || plot_ir4-goeseast_proj_F517R06K-GEOS_06KM-REPLAY-20170905_1745_print.jpg (1024x576) [98.0 KB] || plot_ir4-goeseast_proj_F517R06K-GEOS_06KM-REPLAY-20170905_1745.png (5760x3240) [5.5 MB] || plot_ir4-goeseast_proj_F517R06K-GEOS_06KM-REPLAY-20170905_1745_searchweb.png (320x180) [44.2 KB] || plot_ir4-goeseast_proj_F517R06K-GEOS_06KM-REPLAY-20170905_1745_thm.png (80x40) [3.8 KB] || plot_ir4-goeseast_proj_720p.webm (1280x720) [49.6 MB] || plot_ir4-goeseast_proj_720p.mp4 (1280x720) [156.3 MB] || ", "hits": 45 }, { "id": 30912, "url": "https://svs.gsfc.nasa.gov/30912/", "result_type": "Hyperwall Visual", "release_date": "2017-11-13T00:00:00-05:00", "title": "2017 North Atlantic Hurricane Season Simulation Compared With Observations", "description": "A video comparing model output and satellite imagery. || ir_compare2m-globe_F517R06K-F517R06K_20170801_0000_print.jpg (1024x547) [132.7 KB] || ir_compare2m-globe_F517R06K-F517R06K_20170801_0000.png (5760x3081) [5.8 MB] || ir_compare2m-globe_F517R06K-F517R06K_20170801_0000_searchweb.png (320x180) [60.4 KB] || ir_compare2m-globe_F517R06K-F517R06K_20170801_0000_thm.png (80x40) [5.7 KB] || ir_compare2m-globe_720p.webm (1280x720) [16.1 MB] || ir_compare2m-globe_720p.mp4 (1280x720) [198.3 MB] || ", "hits": 15 }, { "id": 30913, "url": "https://svs.gsfc.nasa.gov/30913/", "result_type": "Hyperwall Visual", "release_date": "2017-11-13T00:00:00-05:00", "title": "SC17 North Atlantic Icelandic Low 1.5-km - Simulation", "description": "A video of a low pressure weather system shows which types of clouds the GEOS model can reproduce. || plot_ir4-northatlantic_map_G5ECMWF-GEOS_01KM-GEOS-20170427_1200_print.jpg (1024x576) [183.4 KB] || plot_ir4-northatlantic_map_G5ECMWF-GEOS_01KM-GEOS-20170427_1200.png (5760x3240) [12.6 MB] || plot_ir4-northatlantic_map_G5ECMWF-GEOS_01KM-GEOS-20170427_1200_searchweb.png (320x180) [81.4 KB] || plot_ir4-northatlantic_map_G5ECMWF-GEOS_01KM-GEOS-20170427_1200_thm.png (80x40) [7.0 KB] || plot_ir4-northatlantic_map_720p.mp4 (1280x720) [44.5 MB] || plot_ir4-northatlantic_map_720p.webm (1280x720) [1.8 MB] || ", "hits": 33 }, { "id": 4163, "url": "https://svs.gsfc.nasa.gov/4163/", "result_type": "Visualization", "release_date": "2014-05-29T00:00:00-04:00", "title": "GPM Senses East Coast Snow Storm on March 17th, 2014", "description": "The Global Precipitation Measurement (GPM) Mission is a joint satellite mission between NASA and JAXA. GPM has the capability of differentiating between liquid and frozen precipitation. In this visualization we see a large east coast snow storm through the eyes of GPM. || ", "hits": 20 }, { "id": 4153, "url": "https://svs.gsfc.nasa.gov/4153/", "result_type": "Visualization", "release_date": "2014-03-25T01:00:00-04:00", "title": "GPM/GMI First Light", "description": "Eleven days after the Feb. 27 launch of the Global Precipitation Measurement (GPM) Core Observatory, the two instruments aboard took their first joint images of an interesting precipitation event. On March 10, the Core Observatory passed over an extra-tropical cyclone about 1055 miles (1700 kilometers) due east of Japan's Honshu Island. The storm formed from the collision of a cold front wrapping around a warm front, emerging over the ocean near Okinawa on March 8. It moved northeast over the ocean south of Japan, drawing cold air west-to-east over the land, a typical winter weather pattern that also brought heavy snow over Hokkaido, the northernmost of the four main islands. After the GPM images were taken, the storm continued to move eastward, slowly intensifying before weakening in the central North Pacific.This visualization shows data from the GPM Microwave Imager, which observes different types of precipitation with 13 channels. Scientists analyze that data and then use it to calculate the light to heavy rain rates and falling snow within the storm.For more information on this topic: GPM web siteOther multimedia items related to this story: GPM GMI First Light (#11508) GPM DPR First Light (#11509) || ", "hits": 34 }, { "id": 11432, "url": "https://svs.gsfc.nasa.gov/11432/", "result_type": "Produced Video", "release_date": "2013-12-09T17:28:00-05:00", "title": "Briefing Materials: Taking Landsat to the Extreme", "description": "At 2:30pm (PST) on Monday, Dec. 9, 2013, there was be a press conference as part of the American Geophysical Union Fall Meeting.What is the coldest place in the world? It is a high ridge in Antarctica on the East Antarctic Plateau where temperatures in several hollows can dip below minus 133.6° Fahrenheit (minus 92° Celsius) on a clear winter night – colder than the previous recorded low temperature.Scientists at the National Snow and Ice Data Center made the discovery while analyzing the most detailed global surface temperature maps to date, developed with data from remote sensing satellites including the MODIS sensor on NASA's Aqua satellite, and the TIRS sensor on Landsat 8, a joint project of NASA and the U.S. Geological Survey (USGS).The researchers analyzed 32 years of data from several satellite instruments that have mapped Antarctica's surface temperature. Near a high ridge that runs from Dome Arugs to Dome Fuji, the scientists found clusters of pockets that have plummeted to record low temperatures dozens of times. The lowest temperature the satellites detected – minus 136° F (minus 93.2° C), on Aug. 10, 2010.The new record is several degrees colder than the previous low of minus 128.6° F (minus 89.2° C), set in 1983 at the Russian Vostok Research Station in East Antarctica. The coldest permanently inhabited place on Earth is northeastern Siberia, where temperatures dropped to a bone-chilling 90 degrees below zero F (minus 67.8° C) in the towns of Verkhoyansk (in 1892) and Oimekon (in 1933).Related feature story: http://www.nasa.gov/content/goddard/nasa-usgs-landsat-8-satellite-pinpoints-coldest-spots-on-earthBriefing SpeakersTed Scambos, National Snow and Ice Data Center (NSIDC), Cooperative Institute for Research in Environmental Sciences (CIRES), University of Colorado Boulder, Boulder, Colorado, USA;Jim Irons, Landsat 8 Project Scientist, NASA's Goddard Space Flight Center, Greenbelt, Maryland.Presenter 1: Ted Scambos || ", "hits": 155 }, { "id": 30132, "url": "https://svs.gsfc.nasa.gov/30132/", "result_type": "Hyperwall Visual", "release_date": "2013-10-17T12:00:00-04:00", "title": "SOFIA views Orion in Mid-IR", "description": "This three-panel comparison of Orion's Messier 42 (M42) region is composed of a visible light image from the Hubble Space Telescope, a near-infrared image captured by the European Southern Observatory in Chile, and a mid-infrared mosaic image taken by SOFIA's Faint Object InfraRed Camera for the SOFIA Telescope, or FORCAST. The FORCAST image, a two-filter false-color composite (20 microns – green, 37 microns – red), reveals detailed structures in the clouds of star forming material, as well as heat radiating from a cluster of luminous newborn stars seen in the upper right. || ", "hits": 103 }, { "id": 30138, "url": "https://svs.gsfc.nasa.gov/30138/", "result_type": "Hyperwall Visual", "release_date": "2013-10-17T12:00:00-04:00", "title": "SOFIA view Jupiter in Infrared", "description": "Infrared image of Jupiter from SOFIA's First Light flight composed of individual images at wavelengths of 5.4 (blue), 24 (green) and 37 microns (red) made by Cornell University's FORCAST camera. Ground-based infrared observations are impossible at 5.4 and 37 microns and normally very difficult at 24 microns even from high mountaintop observatories such as Mauna Kea due to absorption by water and other molecules in Earth's atmosphere. The white stripe in the infrared image is a region of relatively transparent clouds through which the warm interior of Jupiter can be seen. A recent visual-wavelength picture of approximately the same side of Jupiter is shown for comparison. (Images are oriented with Jupiter's south pole at the top.) || ", "hits": 61 }, { "id": 30142, "url": "https://svs.gsfc.nasa.gov/30142/", "result_type": "Hyperwall Visual", "release_date": "2013-10-17T12:00:00-04:00", "title": "W3 Star-Forming Complex in Perseus by Spitzer and SOFIA", "description": "This mid-infrared image of the W3A star cluster in the inset was captured by the FORCAST camera on the SOFIA flying observatory in 2011. It is overlaid on a near-infrared image of the W3 star-forming region from the Spitzer space telescope. The SOFIA image scale is 150 x 100 arcseconds, and the red, green and blue colors represent 37, 20 and 7 μm. The red, green and blue colors in the background image from Spitzer represent 7.9, 4.5, 3.6 μm. || ", "hits": 40 }, { "id": 11070, "url": "https://svs.gsfc.nasa.gov/11070/", "result_type": "Produced Video", "release_date": "2012-08-15T10:00:00-04:00", "title": "The QWIP Detector; an Infrared Instrument", "description": "All objects emit infrared radiation and the characteristics of the infrared radiation are primarily dependent on the temperature of the object. One of the unique features of the new Quantum Well Infrared Photodetector (QWIP) instrument technology is the ability to, what engineers call \"band gap.\" This means it can spectrally respond to specific wavelengths. This video shows the evolution of taking this instrument from inception, to testing on the ground and from a plane, and ultimately to a NASA science mission. The applications are range from finding caves on Mars to loking for thermal polution in rivers or residual hot spots in forest fires, or monitoring food spoilage. || ", "hits": 109 }, { "id": 30135, "url": "https://svs.gsfc.nasa.gov/30135/", "result_type": "Hyperwall Visual", "release_date": "2011-11-30T12:00:00-05:00", "title": "SOFIA views a star-forming region", "description": "The name W40 designates this object's number in a catalog of HII regions, clouds of ionized hydrogen often associated with star formation and massive stars. W40 is in the constellation Aquila the Eagle, visible in the Northern hemisphere's autumn sky. W40 itself is a difficult target for optical astronomers because it lies less than 3 degrees from the central plane of the Milky Way, at a distance of about 1600 light years behind obscuring clouds of interstellar dust and gas.This three image comparison shows W40 in visible, near-infrared and mid-infrared wavelengths. The visible-light image on the left is from the Digitized Sky Survey. The W40 region is not especially prominent at visual wavelengths due to intervening interstellar dust. The near-infrared image in the middle is a composite produced by SOFIA Basic Science Principal Investigators Shuping and Vacca using archived Spitzer infrared space telescope data. The interstellar dust in the foreground and within the W40 region is mostly transparent at these wavelengths, so W40 stands out prominently and one can view into the interior of the nebula to see embedded protostars. Some of these objects were labeled with IRS (\"InfraRed Source\") numbers by earlier investigators. The mid-infrared image on the right is a composite of 5.4 micron (blue), 24.2 micron (green) and 34.8 micron (red) images taken with SOFIA's FORCAST camera in May 2011.The field of view is approximate 3 arcminutes on a side. The bright sources in this image are protostars and thermal emission from dust and gas. Emission at 24 and 35 microns is primarily from warm dust. Some of the protostars can be seen in the Spitzer near-infrared image, but the SOFIA data allow easier determination of their dust temperatures. The hottest object, appearing blue and located at lower left, has very little dust surrounding it and is likely nearest to completing its evolution into a fully-fledged star. The other protostars represented by white in this color balance are cooler and thus have a large amount of circumstellar dust, some of it probably in a disk surrounding the central star. || ", "hits": 86 }, { "id": 3216, "url": "https://svs.gsfc.nasa.gov/3216/", "result_type": "Visualization", "release_date": "2005-10-05T00:00:00-04:00", "title": "GOES-12 Imagery of Hurricane Katrina: Longwave Infrared Close-up (WMS)", "description": "The GOES-12 satellite sits at 75 degrees west longitude at an altitude of 36,000 kilometers over the equator, in geosynchronous orbit. At this position its Imager instrument takes pictures of cloud patterns in several wavelengths for all of North and South America, a primary measurement used in weather forecasting. The Imager takes a pattern of pictures of parts of the Earth in several wavelengths all day, measurements that are vital in weather forecasting. This animation shows a four-day sequence of GOES-12 images in the longwave infrared wavelengths, from 10.2 to 11.2 microns, during the period that Hurricane Katrina passed through the Gulf of Mexico. This wavelength band is the most common one for observing cloud motions and severe storms throughout the day and night. Since GOES-12 takes images most often over the United States (every 5 to 10 minutes), the motion of the clouds in this close-up of the southeast US is very smooth. || ", "hits": 57 }, { "id": 3231, "url": "https://svs.gsfc.nasa.gov/3231/", "result_type": "Visualization", "release_date": "2005-10-05T00:00:00-04:00", "title": "GOES-12 Imagery of Hurricane Katrina: Full Disk Shortwave Infrared (WMS)", "description": "The GOES-12 satellite sits at 75 degrees west longitude at an altitude of 36,000 kilometers over the equator, in geosynchronous orbit. At this position its Imager instrument takes pictures of cloud patterns in several wavelengths for all of North and South America, a primary measurement used in weather forecasting. Every three hours the Imager takes a picture of the full disk of the Earth. This animation shows a sequence of these full disk images in the shortwave infrared wavelengths, 3.78 to 4.03 microns, during the period that Hurricane Katrina passed through the Gulf of Mexico. This wavelength band shows the day-night cycle, and is useful for identifying fog at night and discriminating between water clouds and snow or ice clouds during the daytime. || ", "hits": 22 }, { "id": 3232, "url": "https://svs.gsfc.nasa.gov/3232/", "result_type": "Visualization", "release_date": "2005-10-05T00:00:00-04:00", "title": "GOES-12 Imagery of Hurricane Katrina: Full Disk Water Vapor (WMS)", "description": "The GOES-12 satellite sits at 75 degrees west longitude at an altitude of 36,000 kilometers over the equator, in geosynchronous orbit. At this position its Imager instrument takes pictures of cloud patterns in several wavelengths for all of North and South America, a primary measurement used in weather forecasting. Every three hours the Imager takes a picture of the full disk of the Earth. This animation shows a sequence of these full disk images in the 6.47 to 7.02 micron wavelength band, during the period that Hurricane Katrina passed through the Gulf of Mexico. This wavelength band is useful for estimating mid-level water vapor content and for observing atmospheric motion in that level. || ", "hits": 31 }, { "id": 3233, "url": "https://svs.gsfc.nasa.gov/3233/", "result_type": "Visualization", "release_date": "2005-10-05T00:00:00-04:00", "title": "GOES-12 Imagery of Hurricane Katrina: Full Disk Longwave Infrared (WMS)", "description": "The GOES-12 satellite sits at 75 degrees west longitude at an altitude of 36,000 kilometers over the equator, in geosynchronous orbit. At this position its Imager instrument takes pictures of cloud patterns in several wavelengths for all of North and South America, a primary measurement used in weather forecasting. Every three hours the Imager takes a picture of the full disk of the Earth. This animation shows a sequence of these full disk images in the longwave infrared wavelengths, from 10.2 to 11.2 microns, during the period that Hurricane Katrina passed through the Gulf of Mexico. This wavelength band is the most common one for observing cloud motions and severe storms throughout the day and night. || ", "hits": 30 }, { "id": 3234, "url": "https://svs.gsfc.nasa.gov/3234/", "result_type": "Visualization", "release_date": "2005-10-05T00:00:00-04:00", "title": "GOES-12 Imagery of Hurricane Katrina: Full Disk Lower Level Temperature (WMS)", "description": "The GOES-12 satellite sits at 75 degrees west longitude at an altitude of 36,000 kilometers over the equator, in geosynchronous orbit. At this position its Imager instrument takes pictures of cloud patterns in several wavelengths for all of North and South America, a primary measurement used in weather forecasting. Every three hours the Imager takes a picture of the full disk of the Earth. This animation shows a sequence of these full disk images in the wavelength band from 12.9 to 13.8 microns, during the period that Hurricane Katrina passed through the Gulf of Mexico. This wavelength band is useful for determining cloud characteristics such as cloud top pressure. || ", "hits": 16 }, { "id": 3235, "url": "https://svs.gsfc.nasa.gov/3235/", "result_type": "Visualization", "release_date": "2005-10-05T00:00:00-04:00", "title": "GOES-10 Imagery of Hurricane Katrina: Full Disk Longwave Infrared (WMS)", "description": "The GOES-10 satellite sits at 135 degrees west longitude at an altitude of 36,000 kilometers over the equator, in geosynchronous orbit. At this position its Imager instrument takes pictures of cloud patterns in several wavelengths for the Pacific Ocean, a primary measurement used in weather forecasting. Every three hours the Imager takes a picture of the full disk of the Earth. This animation shows a sequence of these full disk images in the longwave infrared wavelengths, from 10.2 to 11.2 microns, during the period that Hurricane Katrina passed through the Gulf of Mexico. This wavelength band is the most common one for observing cloud motions and severe storms throughout the day and night. || ", "hits": 24 }, { "id": 3236, "url": "https://svs.gsfc.nasa.gov/3236/", "result_type": "Visualization", "release_date": "2005-10-05T00:00:00-04:00", "title": "GOES-12 Imagery of Hurricane Katrina: Longwave Infrared Overview (WMS)", "description": "The GOES-12 satellite sits at 75 degrees west longitude at an altitude of 36,000 kilometers over the equator, in geosynchronous orbit. At this position its Imager instrument takes pictures of cloud patterns in several wavelengths for all of North and South America, a primary measurement used in weather forecasting. The Imager takes a pattern of pictures of parts of the Earth in several wavelengths all day, measurements that are vital in weather forecasting. This animation shows a four-day sequence of GOES-12 images in the longwave infrared wavelengths, from 10.2 to 11.2 microns, during the period that Hurricane Katrina passed through the Gulf of Mexico. This wavelength band is the most common one for observing cloud motions and severe storms throughout the day and night. Note that most of the images are taken over the United States (about every 5 minutes) with full disk images every 3 hours and several specific images over South America every day. || ", "hits": 20 }, { "id": 3237, "url": "https://svs.gsfc.nasa.gov/3237/", "result_type": "Visualization", "release_date": "2005-10-05T00:00:00-04:00", "title": "GOES-12 Imagery of Hurricane Katrina: Longwave Infrared Progression (WMS)", "description": "The GOES-12 satellite sits at 75 degrees west longitude at an altitude of 36,000 kilometers over the equator, in geosynchronous orbit. At this position its Imager instrument takes pictures of cloud patterns in several wavelengths for all of North and South America, a primary measurement used in weather forecasting. The Imager takes a pattern of pictures of parts of the Earth in several wavelengths all day, measurements that are vital in weather forecasting. This animation shows a four-day sequence of GOES-12 images in the longwave infrared wavelengths, from 10.2 to 11.2 microns, during the period that Hurricane Katrina passed through the Gulf of Mexico. This wavelength band is the most common one for observing cloud motions and severe storms throughout the day and night. Note that most of the images are taken over the United States (about every 5 minutes) with full disk images every 3 hours and several specific images over South America every day. In this animation, new images are placed over old images rather than replacing them, so different parts of the image update at different times as measurements are taken. || ", "hits": 22 }, { "id": 2894, "url": "https://svs.gsfc.nasa.gov/2894/", "result_type": "Visualization", "release_date": "2004-02-11T12:00:00-05:00", "title": "Global Infrared Cloud Cover, September 2001 (WMS)", "description": "This animation is a mosaic of cloud cover data taken by several different satellites in the infrared band. One of the most prominent cloud features during this time was Hurricane Erin near the Atlantic coast of the United States. || ", "hits": 92 }, { "id": 2895, "url": "https://svs.gsfc.nasa.gov/2895/", "result_type": "Visualization", "release_date": "2004-02-11T12:00:00-05:00", "title": "Infrared Cloud Cover over the Atlantic Ocean, September 2001 (WMS)", "description": "This animation is a mosaic of cloud cover data taken by several different satellites in the infrared band. Instead of showing a global composite, it is cropped to highlight the Atlantic Ocean. One of the most prominent cloud features during this time was Hurricane Erin. || ", "hits": 30 } ] }