{
    "count": 36,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 5609,
            "url": "https://svs.gsfc.nasa.gov/5609/",
            "result_type": "Visualization",
            "release_date": "2026-01-26T05:00:00-05:00",
            "title": "Heliophysics Satellite Fleet - 2026",
            "description": "A tour of the NASA Heliophysics fleet from near-Earth satellites out to the Voyagers beyond the heliopause.",
            "hits": 912
        },
        {
            "id": 5443,
            "url": "https://svs.gsfc.nasa.gov/5443/",
            "result_type": "Visualization",
            "release_date": "2024-12-17T00:00:00-05:00",
            "title": "Heliophysics Sentinels 2024",
            "description": "There have been some changes since the 2022 Heliophysics Fleet.  AIM and ICON have been decommissioned while two other instruments have been added.  AWE is an instrument mounted on the ISS, and RAD is a particle detector on the Curiosity Mars rover.  As of Winter 2024, here's a tour of the NASA Heliophysics fleet from the near-Earth satellites out to the Voyagers beyond the heliopause. || ",
            "hits": 68
        },
        {
            "id": 4898,
            "url": "https://svs.gsfc.nasa.gov/4898/",
            "result_type": "Visualization",
            "release_date": "2022-11-23T00:00:00-05:00",
            "title": "Heliophysics Sentinels 2022",
            "description": "There has been one significant change since the 2020 Heliophysics Fleet.  SET has been decommissioned.  As of Fall 2022, here's a tour of the NASA Heliophysics fleet from the near-Earth satellites out to the Voyagers beyond the heliopause.Excepting the Voyager missions, the satellite orbits are color coded for their observing program:Magenta: TIM (Thermosphere, Ionosphere, Mesosphere) observationsYellow: solar observations and imageryCyan: Geospace and magnetosphereViolet: Heliospheric observations || ",
            "hits": 41
        },
        {
            "id": 4887,
            "url": "https://svs.gsfc.nasa.gov/4887/",
            "result_type": "Visualization",
            "release_date": "2021-03-01T10:00:00-05:00",
            "title": "Heliophysics Sentinels 2020 (Forecast Version)",
            "description": "In addition to the NASA missions used in research for space weather (see 2020 Heliophysics Fleet) there are additional missions operated by NOAA used for space weather forecasting.  As of spring 2020, here's a tour of the NASA and NOAA Heliophysics fleets from the near-Earth satellites out to the inner solar system.The satellite orbits are color coded for their observing program:Magenta: TIM (Thermosphere, Ionosphere, Mesosphere) observationsYellow: solar observations and imageryCyan: Geospace and magnetosphereViolet: Heliospheric observations || ",
            "hits": 29
        },
        {
            "id": 4766,
            "url": "https://svs.gsfc.nasa.gov/4766/",
            "result_type": "Visualization",
            "release_date": "2020-09-21T11:00:00-04:00",
            "title": "IRIS views Nano-Flares on the Sun",
            "description": "Opening full-disk solar view from AIA 304 angstroms, zooming in and fading in IRIS SJI at 1400 angstroms. || SDO304-IRIS1400-nanoflare2014-zoom_stand.HD1080i.00663_print.jpg (1024x576) [139.8 KB] || SDO304-IRIS1400-nanoflare2014-zoom_stand.HD1080i.00663_searchweb.png (320x180) [67.9 KB] || SDO304-IRIS1400-nanoflare2014-zoom_stand.HD1080i.00663_thm.png (80x40) [5.0 KB] || SDO304-IRIS1400-nanoflare2014-zoomHD (1920x1080) [0 Item(s)] || SDO304-IRIS1400-nanoflare2014-zoom_stand.HD1080i_p30.mp4 (1920x1080) [60.5 MB] || SDO304-IRIS1400-nanoflare2014-zoom_stand.HD1080i_p30.webm (1920x1080) [3.0 MB] || SDO304-IRIS1400-nanoflare2014-zoomHD (3840x2160) [0 Item(s)] || SDO304-IRIS1400-nanoflare2014-zoom_stand.UHD2160_p30.mp4 (3840x2160) [203.9 MB] || SDO304-IRIS1400-nanoflare2014-zoom_stand.HD1080i_p30.mp4.hwshow [218 bytes] || ",
            "hits": 34
        },
        {
            "id": 13691,
            "url": "https://svs.gsfc.nasa.gov/13691/",
            "result_type": "Produced Video",
            "release_date": "2020-09-21T11:00:00-04:00",
            "title": "NASA’s IRIS spots Nanojets: Shining light on heating the solar corona",
            "description": "In pursuit of understanding why the Sun's atmosphere is so much hotter than the surface, and to help differentiate between a host of theories about what causes this heating, researchers turn to NASA's Interface Region Imaging Spectrograph (IRIS) mission. IRIS was finely tuned with a high-resolution imager to zoom in on specific hard-to-see events on the Sun.A paper published in Nature on Sept. 21, 2020, reports on the first ever clear images of nanojets — bright, thin lights that travel perpendicular to magnetic structures in the solar atmosphere called the corona — in a process that reveals the existence of one of the potential coronal heating candidates: nanoflares. || ",
            "hits": 38
        },
        {
            "id": 4822,
            "url": "https://svs.gsfc.nasa.gov/4822/",
            "result_type": "Visualization",
            "release_date": "2020-09-15T10:00:00-04:00",
            "title": "Heliophysics Sentinels 2020",
            "description": "There have been few changes since the 2018 Heliophysics Fleet.  Van Allen Probes and SORCE have been decommissioned, while Solar Orbiter, ICON and SET have been added.  As of spring 2020, here's a tour of the NASA Heliophysics fleet from the near-Earth satellites out to the Voyagers beyond the heliopause.Excepting the Voyager missions, the satellite orbits are color coded for their observing program:Magenta: TIM (Thermosphere, Ionosphere, Mesosphere) observationsYellow: solar observations and imageryCyan: Geospace and magnetosphereViolet: Heliospheric observations || ",
            "hits": 36
        },
        {
            "id": 4360,
            "url": "https://svs.gsfc.nasa.gov/4360/",
            "result_type": "Visualization",
            "release_date": "2018-12-10T11:00:00-05:00",
            "title": "Heliophysics Sentinels 2018",
            "description": "This movie presents the trajectories of the heliophysics fleet from close to Earth to out beyond the heliopause. || Sentinels2018.Sentinels2Voyager.GSE.AU.clockSlate_EarthTarget.UHD3840.00000_print.jpg (1024x576) [74.5 KB] || Sentinels2018.Sentinels2Voyager.GSE.AU.clockSlate_EarthTarget.UHD3840.00000_searchweb.png (180x320) [65.6 KB] || Sentinels2018.Sentinels2Voyager.GSE.AU.clockSlate_EarthTarget.UHD3840.00000_thm.png (80x40) [5.1 KB] || Sentinels2018.Sentinels2Voyager_1080p30.mp4 (1920x1080) [40.3 MB] || Sentinels2018.Sentinels2Voyager_1080p30.webm (1920x1080) [6.3 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || Sentinels2018.Sentinels2Voyager_2160p30.mp4 (3840x2160) [125.7 MB] || Sentinels2018.Sentinels2Voyager_1080p30.mp4.hwshow || ",
            "hits": 50
        },
        {
            "id": 4589,
            "url": "https://svs.gsfc.nasa.gov/4589/",
            "result_type": "Visualization",
            "release_date": "2017-10-25T10:00:00-04:00",
            "title": "Heliophysics Sentinels 2017",
            "description": "This visualization starts from near Earth and the Earth orbiting satellite fleet out to the Moon, then past the Sun-Earth Lagrange point 1 to out beyond the heliopause.  This is the long-play version. || Sentinels2017.Sentinels2Voyager.GSE.AU.clockSlate_EarthTarget.UHD3840.00000_print.jpg (1024x576) [136.1 KB] || Sentinels2017.Sentinels2Voyager.GSE.AU.clockSlate_EarthTarget.UHD3840.00000_searchweb.png (180x320) [84.6 KB] || Sentinels2017.Sentinels2Voyager.GSE.AU.clockSlate_EarthTarget.UHD3840.00000_thm.png (80x40) [6.0 KB] || Sentinels2017.Sentinels2Voyager.HD1080i_p30.webm (1920x1080) [12.4 MB] || SlowPlay (1920x1080) [0 Item(s)] || Sentinels2017.Sentinels2Voyager.HD1080i_p30.mp4 (1920x1080) [111.6 MB] || SlowPlay (3840x2160) [0 Item(s)] || Sentinels2017.Sentinels2Voyager_2160p30.mp4 (3840x2160) [336.2 MB] || Sentinels2017.Sentinels2Voyager.HD1080i_p30.mp4.hwshow [209 bytes] || ",
            "hits": 24
        },
        {
            "id": 12604,
            "url": "https://svs.gsfc.nasa.gov/12604/",
            "result_type": "Produced Video",
            "release_date": "2017-06-22T14:00:00-04:00",
            "title": "Scientists Uncover Origins of Dynamic Jets on Sun's Surface",
            "description": "At any given moment, as many as 10 million wild jets of solar material burst from the sun’s surface. They erupt as fast as 60 miles per second, and can reach lengths of 6,000 miles before collapsing. These are spicules, and despite their grass-like abundance, scientists didn’t understand how they form. Now, for the first time, a computer simulation — so detailed it took a full year to run — shows how spicules form, helping scientists understand how spicules can break free of the sun’s surface and surge upward so quickly. This work relied upon high-cadence observations from NASA’s Interface Region Imaging Spectrograph, or IRIS, and the Swedish 1-meter Solar Telescope in La Palma. Together, the spacecraft and telescope peer into the lower layers of the sun’s atmosphere, known as the interface region, where spicules form. The results of this NASA-funded study were published in Science on June 22, 2017 — a special time of the year for the IRIS mission, which celebrates its fourth anniversary in space on June 26.Research: On the generation of solar spicules and Alfvénic waves.Journal: Science, June 22, 2017.Link to paper: http://science.sciencemag.org/content/356/6344/1269.full || ",
            "hits": 48
        },
        {
            "id": 20265,
            "url": "https://svs.gsfc.nasa.gov/20265/",
            "result_type": "Animation",
            "release_date": "2017-04-03T13:00:00-04:00",
            "title": "ICON Beauty Pass",
            "description": "Beauty pass showing ICON observing the ionosphere. Credit: NASA/GSFC/CIL || AirGlow_final_ProRes.00001_print.jpg (1024x576) [87.7 KB] || AirGlow_final_ProRes.00001_web.png (320x180) [74.1 KB] || AirGlow_final_ProRes.00001_searchweb.png (180x320) [74.1 KB] || AirGlow_final_ProRes.00001_thm.png (80x40) [6.0 KB] || AirGlow_final_H264.mov (1920x1080) [19.5 MB] || 1920x1080_16x9_60p (1920x1080) [0 Item(s)] || AirGlow_final_ProRes.webm (1920x1080) [1.0 MB] || AirGlow_final_ProRes.mov (1920x1080) [304.3 MB] || ",
            "hits": 27
        },
        {
            "id": 30822,
            "url": "https://svs.gsfc.nasa.gov/30822/",
            "result_type": "Infographic",
            "release_date": "2016-12-06T00:00:00-05:00",
            "title": "NASA's Heliophysics Fleet",
            "description": "The current Heliophysics fleet || hpd-fleet-chart-jan-2024_print.jpg (1024x576) [180.0 KB] || hpd-fleet-chart-jan-2024.png (3840x2160) [7.3 MB] || hpd-fleet-chart-jan-2024_searchweb.png (320x180) [91.3 KB] || hpd-fleet-chart-jan-2024_thm.png (80x40) [7.2 KB] || nasas-fleets-by-division-helio-jewel.hwshow [228 bytes] ||",
            "hits": 69
        },
        {
            "id": 12292,
            "url": "https://svs.gsfc.nasa.gov/12292/",
            "result_type": "Produced Video",
            "release_date": "2016-06-24T15:00:00-04:00",
            "title": "Solar Highlights of 2016/2017",
            "description": "A collection of solar highlights featuring:- NASA's Solar Dynamics Observatory (SDO)- NASA's Interface Region Imaging Spectrograph (IRIS) mission- ESA/NASA's Solar and Heliospheric Observatory (SOHO)- NASA's Solar TErrestrial RElations Observatory (STEREO) mission || ",
            "hits": 170
        },
        {
            "id": 11916,
            "url": "https://svs.gsfc.nasa.gov/11916/",
            "result_type": "Produced Video",
            "release_date": "2015-07-23T11:45:00-04:00",
            "title": "Taking A Slice Of Light",
            "description": "Sometimes studying the sun requires looking at it one strip at a time. || c-1920.jpg (1920x1080) [542.3 KB] || c-1280.jpg (1280x720) [361.9 KB] || c-1024.jpg (1024x576) [269.6 KB] || c-1024_print.jpg (1024x576) [257.0 KB] || c-1024_searchweb.png (320x180) [121.9 KB] || c-1024_thm.png (80x40) [26.6 KB] || ",
            "hits": 40
        },
        {
            "id": 4318,
            "url": "https://svs.gsfc.nasa.gov/4318/",
            "result_type": "Visualization",
            "release_date": "2015-06-26T14:00:00-04:00",
            "title": "A Slice of Light: How IRIS Observes the Sun",
            "description": "Short version of the IRIS visualization with windowed SJI imagery. || SDO304IRISspectraWin4.2015MarA_stand.HD1080i.00400_print.jpg (1024x576) [122.9 KB] || SDO304IRISspectraWin4.2015MarA_stand.HD1080i.00400_searchweb.png (320x180) [95.6 KB] || SDO304IRISspectraWin4.2015MarA_stand.HD1080i.00400_thm.png (80x40) [7.6 KB] || SDO304IRISspectraWin4_1080p.mp4 (1920x1080) [22.3 MB] || Windowed.short (1920x1080) [128.0 KB] || SDO304IRISspectraWin4_1080p.webm (1920x1080) [4.3 MB] || ",
            "hits": 69
        },
        {
            "id": 11897,
            "url": "https://svs.gsfc.nasa.gov/11897/",
            "result_type": "Produced Video",
            "release_date": "2015-06-26T14:00:00-04:00",
            "title": "A Slice of Light: How IRIS Observes the Sun",
            "description": "Watch this video on the NASAexplorer YouTube channel.0 || IRISthumb.jpg (720x480) [26.9 KB] || IRISthumb_searchweb.png (320x180) [44.2 KB] || IRISthumb_thm.png (80x40) [15.0 KB] || G2015-050_How_IRIS_Sees_Sun_appletv.m4v (960x540) [32.0 MB] || G2015-050_How_IRIS_Sees_Sun_youtube_hq.mov (1920x1080) [100.4 MB] || G2015-050_How_IRIS_Sees_Sun.mov (1920x1080) [2.0 GB] || G2015-050_How_IRIS_Sees_Sun_1280x720.wmv (1280x720) [32.4 MB] || G2015-050_How_IRIS_Sees_Sun_prores.mov (1280x720) [1.0 GB] || G2015-050_How_IRIS_Sees_Sun.webm (1920x1080) [8.5 MB] || G2015-050_How_IRIS_Sees_Sun_appletv_subtitles.m4v (960x540) [31.9 MB] || G2015-050_How_IRIS_Sees_Sun_ipod_lg.m4v (640x360) [12.8 MB] || G2015-050_How_IRIS_Sees_Sun.en_US.vtt [1.3 KB] || G2015-050_How_IRIS_Sees_Sun.en_US.srt [1.3 KB] || G2015-050_How_IRIS_Sees_Sun_ipod_sm.mp4 (320x240) [6.8 MB] || ",
            "hits": 62
        },
        {
            "id": 4288,
            "url": "https://svs.gsfc.nasa.gov/4288/",
            "result_type": "Visualization",
            "release_date": "2015-06-10T00:00:00-04:00",
            "title": "The 2015 Earth-Orbiting Heliophysics Fleet",
            "description": "Movie showing the heliosphysics missions from near Earth orbit out to the orbit of the Moon.This video is also available on our YouTube channel. || Helio2015A.MMStour.slate_RigRHS.HD1080i.0500_print.jpg (1024x576) [112.6 KB] || Helio2015A.MMStour.HD1080.webm (1920x1080) [6.7 MB] || WithoutTimeStamp (1920x1080) [128.0 KB] || Helio2015A.MMStour.HD1080.mov (1920x1080) [196.3 MB] || Helio2015_4288.pptx [198.6 MB] || Helio2015_4288.key [201.3 MB] || ",
            "hits": 76
        },
        {
            "id": 4282,
            "url": "https://svs.gsfc.nasa.gov/4282/",
            "result_type": "Visualization",
            "release_date": "2015-03-25T00:00:00-04:00",
            "title": "March Solar X-flare from IRIS and SDO",
            "description": "Zoom in on the view of the flare, using SDO and IRIS. || SDO304_IRIS1330_March2015A_stand.HD1080i.00500_print.jpg (1024x576) [151.2 KB] || SDO304_IRIS1330_March2015A_stand.HD1080i.00500_searchweb.png (320x180) [88.9 KB] || SDO304_IRIS1330_March2015A_stand.HD1080i.00500_web.png (320x180) [88.9 KB] || SDO304_IRIS1330_March2015A_stand.HD1080i.00500_thm.png (80x40) [6.9 KB] || SDO304_IRIS1330_March2015A_HD1080.webm (1920x1080) [4.0 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || SDO304_IRIS1330_March2015A_stand_HD1080.mp4 (1920x1080) [121.2 MB] || SDO304_IRIS1330_March2015A_HD1080.mov (1920x1080) [353.5 MB] || SDO304_IRIS1330_March2015A_stand_HD1080.mp4.hwshow [205 bytes] || ",
            "hits": 37
        },
        {
            "id": 11708,
            "url": "https://svs.gsfc.nasa.gov/11708/",
            "result_type": "Produced Video",
            "release_date": "2014-10-16T14:00:00-04:00",
            "title": "NASA's IRIS Helps Explain Mysterious Heat of the Solar Atmosphere",
            "description": "This movie shows succeeding images from NASA’s IRIS of the same area of the sun in different wavelengths.  Each image carries information about how fast the solar material is moving, which has shown scientists that a series of loops are twisting in the sun’s lower atmosphere.Credit: NASA/IRIS/Pereira || S3_still.png (1534x1154) [1.1 MB] || S3_still_web.jpg (319x240) [22.4 KB] || S3_still_searchweb.png (320x180) [67.4 KB] || S3_still_thm.png (80x40) [8.5 KB] || S3.mov (768x576) [2.8 MB] || S3.webmhd.webm (960x540) [1.8 MB] || ",
            "hits": 98
        },
        {
            "id": 11599,
            "url": "https://svs.gsfc.nasa.gov/11599/",
            "result_type": "Produced Video",
            "release_date": "2014-08-28T11:30:00-04:00",
            "title": "Beautiful Explosion",
            "description": "A giant burst of solar material surged off the side of the sun on May 9, 2014—and NASA's newest sun-watching mission caught the event in extraordinary detail. This was the first explosion known as a coronal mass ejection (CME) that the Interface Region Imaging Spectrograph, or IRIS, spacecraft was able to observe. The spacecraft must commit to pointing at certain areas of the sun at least a day in advance, so catching a CME in the act involves some educated guesses and a little bit of luck. On this day it focused in on the left side of the sun and happened to see the base of the CME.  It recorded super-hot material erupting from the sun at speeds of 1.5 million mph. Watch the video to see it for yourself. || ",
            "hits": 106
        },
        {
            "id": 11556,
            "url": "https://svs.gsfc.nasa.gov/11556/",
            "result_type": "Produced Video",
            "release_date": "2014-05-30T09:30:00-04:00",
            "title": "A First for NASA's IRIS: Observing a Gigantic Eruption of Solar Material",
            "description": "A coronal mass ejection, or CME, surged off the side of the sun on May 9, 2014, and NASA's newest solar observatory caught it in extraordinary detail. This was the first CME observed by the Interface Region Imaging Spectrograph, or IRIS, which launched in June 2013 to peer into the lowest levels of the sun's atmosphere with better resolution than ever before. Watch the movie to see how a curtain of solar material erupts outward at speeds of 1.5 million miles per hour.IRIS must commit to pointing at certain areas of the sun at least a day in advance, so catching a CME in the act involves some educated guesses and a little bit of luck. \"We focus in on active regions to try to see a flare or a CME,\" said Bart De Pontieu, the IRIS science lead at Lockheed Martin Solar & Astrophysics Laboratory in Palo Alto, California. \"And then we wait and hope that we'll catch something. This is the first clear CME for IRIS so the team is very excited.\" The IRIS imagery focuses in on material of 30,000 Kelvin at the base, or foot points, of the CME. The line moving across the middle of the movie is the entrance slit for IRIS's spectrograph, an instrument that can split light into its many wavelengths – a technique that ultimately allows scientists to measure temperature, velocity and density of the solar material behind the slit. The field of view for this imagery is about five Earth's wide and about seven and a half Earth's tall. The IRIS Observatory was designed by and the mission is managed by Lockheed Martin Solar & Astrophysics Laboratory. NASA's Ames Research Center in Mountain View, California, provides mission operations and ground data systems. NASA's Goddard Space Flight Center in Greenbelt, Maryland, manages the Explorers Program for NASA's Science Mission Directorate in Washington, D.C. || ",
            "hits": 63
        },
        {
            "id": 11522,
            "url": "https://svs.gsfc.nasa.gov/11522/",
            "result_type": "Produced Video",
            "release_date": "2014-05-07T12:00:00-04:00",
            "title": "The Best Observed X-class Flare",
            "description": "On March 29, 2014 the sun released an X-class flare. It was observed by NASA's Interface Region Imaging Spectrograph, or IRIS; NASA's Solar Dynamics Observatory, or SDO; NASA's Reuven Ramaty High Energy Solar Spectroscopic Imager, or RHESSI; the Japanese Aerospace Exploration Agency's Hinode; and the National Solar Observatory's Dunn Solar Telescope located at Sacramento Peak in New Mexico. To have a record of such an intense flare from so many observatories is unprecedented.  Such research can help scientists better understand what catalyst sets off these large explosions on the sun. Perhaps we may even some day be able to predict their onset and forewarn of the radio blackouts solar flares can cause near Earth – blackouts that can interfere with airplane, ship and military communications. || ",
            "hits": 88
        },
        {
            "id": 4164,
            "url": "https://svs.gsfc.nasa.gov/4164/",
            "result_type": "Visualization",
            "release_date": "2014-05-07T10:00:00-04:00",
            "title": "A Multi-Mission View of a Solar Flare: Optical to Gamma-rays",
            "description": "To improve our understanding of complex phenomena such as solar flares, a wide variety of tools are needed.  In the case of astronomy, those tools enable us to analyze the light in many different wavelengths and many different ways.Many different instruments are observing the Sun almost continuously, both from space and on the surface of the Earth.  On March 29, 2014, the Dunn Solar Telescope at Sacramento Peak, New Mexico was observing a solar active region and requested other observatories to watch as well.  As a result of this coordination, the region was being observed by a large number of different instruments, ground and space-based, when it subsequently erupted with an X-class flare.  This visualization presents various combinations of the datasets collected during this effort.  The color text represents the dominant color of the dataset in the imagery.Solar Dynamics Observatory (SDO): HMI (617.1nm).  This data represents the Sun is visible light similar to how we see it from the ground.Solar Dynamics Observatory (SDO): AIA (17.1nm).  Solar ultraviolet emission, which can only be seen from space, reveals plasma flowing, and escaping, along magnetic fields.IRIS Slit-Jaw Imager: 140.0nm.  This high-resolution imager also contains a slit (the dark vertical line in the center of the field) which directs the light to an ultraviolet spectrometer which is used to extract even more information about the light.  The imager slews back-and-forth across the region, providing spectra over a larger area of the Sun.Hinode/X-ray Telescope: x-ray band. Indicates very hot plasma.RHESSI: 50-100 keV.  High-energy gamma-ray emission.  Emission from these locations represent the very highest energy photons from the flare event.Dunn Solar Telescope: G-band filter.  This filter, showing much of the solar surface (photosphere) in visible light, provides a detailed view of the sunspots and convection cells.  The view moves because the instrument was repointed several times during the observation.Dunn Solar Telescope: IBIS ( Hydrogen alpha, 656.3nm;  Calcium 854.2 nm;  Iron 630.15nm).  This is the small rectangular view within the Dunn Solar Telescope G-band view.  This instrument can tune the wavelength during the observation, which provides views of the solar atmosphere at different depths. || ",
            "hits": 39
        },
        {
            "id": 11467,
            "url": "https://svs.gsfc.nasa.gov/11467/",
            "result_type": "Produced Video",
            "release_date": "2014-03-20T00:00:00-04:00",
            "title": "Deconstructing The Sun",
            "description": "On January 28, 2014, NASA's Interface Region Imaging Spectrograph, or IRIS, spacecraft saw its strongest solar flare since it launched in 2013. Solar flares are bursts of X-rays and light that stream out into space, but no one yet knows the fine details of what sets them off. By observing a layer of the sun’s lower atmosphere called the chromosphere, which helps regulate how energy and material flows up from the sun's surface, IRIS can see part of the process that powers these events. However, there's a bit of luck involved in making such observations. IRIS’s instruments can’t look at the entire sun at once, so scientists must decide what areas might be the most interesting to watch. On January 28, scientists focused IRIS’s telescope and imaging spectrograph on a magnetically active region on the sun. Perfect timing: They witnessed a medium-sized solar flare in the act of erupting. Watch the video to see the flare through IRIS's eyes. || ",
            "hits": 27
        },
        {
            "id": 4146,
            "url": "https://svs.gsfc.nasa.gov/4146/",
            "result_type": "Visualization",
            "release_date": "2014-02-21T10:00:00-05:00",
            "title": "IRIS close-up of a solar flare",
            "description": "The Slit-Jaw Imager (SJI) aboard IRIS (Interface Region Imaging Spectrograph) observes a tiny region of the Sun at an image resolution (0.166 arc-seconds per pixel) almost four times higher than the Solar Dynamics Observatory (SDO) (0.6 arc-seconds per pixel). In addition, IRIS has a narrow slit in the imaging plane (the thin, dark vertical line in the center of the inset) which directs some of the light to a spectrograph which allows solar physicists to determine velocity and temperature of the solar plasma.In this zoom-in from a full-disk view of the Sun from SDO, the imager is observering the Sun at a wavelength of 133nm (1330 angstroms). The imager field-of-view is moved across the solar disk in four steps, allowing the slit to pass over different regions of the Sun to determine the properties of the plasma.Note: IRIS and SDO are in very different orbits. You can see samples of the orbits at The 2013 Earth-Orbiting Heliophysics Fleet. IRIS is in a near-Earth orbit, while SDO is much higher at geosynchronous orbit. This difference in camera location creates a small parallax between the images composited from these two cameras. || ",
            "hits": 33
        },
        {
            "id": 11483,
            "url": "https://svs.gsfc.nasa.gov/11483/",
            "result_type": "Produced Video",
            "release_date": "2014-02-21T09:45:00-05:00",
            "title": "NASA's IRIS Spots Its Largest Solar Flare",
            "description": "On Jan. 28, 2014, NASA's Interface Region Imaging Spectrograph, or IRIS, witnessed its strongest solar flare since it launched in the summer of 2013. Solar flares are bursts of x-rays and light that stream out into space, but scientists don't yet know the fine details of what sets them off. IRIS peers into a layer of the sun's lower atmosphere just above the surface, called the chromosphere, with unprecedented resolution. However, IRIS can't look at the entire sun at the same time, so the team must always make decisions about what region might provide useful observations. On Jan. 28, scientists spotted a magnetically active region on the sun and focused IRIS on it to see how the solar material behaved under intense magnetic forces. At 2:40 p.m. EST, a moderate flare, labeled an M-class flare — which is the second strongest class flare after X-class – erupted from the area, sending light and x-rays into space. IRIS studies the layer of the sun’s atmosphere called the chromosphere that is key to regulating the flow of energy and material as they travel from the sun's surface out into space. Along the way, the energy heats up the upper atmosphere, the corona, and sometimes powers solar events such as this flare. IRIS is equipped with an instrument called a spectrograph that can separate out the light it sees into its individual wavelengths, which in turn correlates to material at different temperatures, velocities and densities. The spectrograph on IRIS was pointed right into the heart of this flare when it reached its peak, and so the data obtained can help determine how different temperatures of plasma flow where, giving scientists more insight into how flares work. || ",
            "hits": 29
        },
        {
            "id": 11448,
            "url": "https://svs.gsfc.nasa.gov/11448/",
            "result_type": "Produced Video",
            "release_date": "2014-02-06T00:00:00-05:00",
            "title": "Into The Fire",
            "description": "On June 27, 2013, NASA's Interface Region Imaging Spectrograph, or IRIS, launched into space to study the mysterious lowest layers of the sun’s atmosphere. These layers make up what's called the interface region, an area where solar material is constantly writhing and exploding. The spacecraft is designed to take high-resolution images of the interface region in unprecedented detail. Such images will help scientists see how energy traveling through the region heats the sun's upper atmosphere to temperatures a thousand times hotter than the surface. Initial observations show the region is much more violent than previously understood, and contains a multitude of thin, fibril-like structures that have never before been seen. Watch the video for close-up views of the sun captured by IRIS. || ",
            "hits": 17
        },
        {
            "id": 11385,
            "url": "https://svs.gsfc.nasa.gov/11385/",
            "result_type": "Produced Video",
            "release_date": "2013-12-17T10:00:00-05:00",
            "title": "Jewel Box Sun",
            "description": "Telescopes help distant objects appear bigger, but this is only one of their advantages. Telescopes can also collect light in ranges that our eyes alone cannot see, providing scientists ways of observing a whole host of material and processes that would otherwise be inaccessible. A new NASA movie of the sun based on data from NASA's Solar Dynamics Observatory, or SDO, shows the wide range of wavelengths – invisible to the naked eye – that the telescope can view. SDO converts the wavelengths into an image humans can see, and the light is colorized into a rainbow of colors. As the colors sweep around the sun in the movie, viewers should note how different the same area of the sun appears. This happens because each wavelength of light represents solar material at specific temperatures. Different wavelengths convey information about different components of the sun's surface and atmosphere, so scientists use them to paint a full picture of our constantly changing and varying star.Yellow light of 5800 angstroms, for example, generally emanates from material of about 10,000 degrees F (5700 degrees C), which represents the surface of the sun. Extreme ultraviolet light of 94 angstroms, which is typically colorized in green in SDO images, comes from atoms that are about 11 million degrees F (6,300,000 degrees C) and is a good wavelength for looking at solar flares, which can reach such high temperatures. By examining pictures of the sun in a variety of wavelengths – as is done not only by SDO, but also by NASA's Interface Region Imaging Spectrograph, NASA's Solar Terrestrial Relations Observatory and the European Space Agency/NASA Solar and Heliospheric Observatory — scientists can track how particles and heat move through the sun's atmosphere. || ",
            "hits": 116
        },
        {
            "id": 4127,
            "url": "https://svs.gsfc.nasa.gov/4127/",
            "result_type": "Visualization",
            "release_date": "2013-12-16T12:00:00-05:00",
            "title": "The 2013 Earth-Orbiting Heliophysics Fleet",
            "description": "There've been a few changes since the 2012 Earth-Orbiting Heliophysics Fleet. As of Fall of 2013, here's a tour of the NASA Near-Earth Heliophysics fleet, covering the space from near-Earth orbit out to the orbit of the Moon.The satellite orbits are color coded for their observing program:Magenta: TIM (Thermosphere, Ionosphere, Mesosphere) observationsYellow: solar observations and imageryCyan: Geospace and magnetosphereViolet: Heliospheric observationsNear-Earth Fleet:Hinode: Observes the Sun in multiple wavelengths up to x-rays. SVS pageRHESSI : Observes the Sun in x-rays and gamma-rays. SVS pageTIMED: Studies the upper layers (40-110 miles up) of the Earth's atmosphere.FAST: Measures particles and fields in regions where aurora form.CINDI: Measures interactions of neutral and charged particles in the ionosphere. SORCE: Monitors solar intensity across a broad range of the electromagnetic spectrum.AIM: Images and measures noctilucent clouds. SVS pageVan Allen Probes: Two probes moving along the same orbit esigned to study the impact of space weather on Earth's radiation belts. SVS pageTWINS: Two Wide-Angle Imaging Neutral-Atom Spectrometers (TWINS) are two probes observing the Earth with neutral atom imagers.IRIS: Interface Region Imaging Spectrograph is designed to take high-resolution spectra and images of the region between the solar photosphere and solar atmosphere.Geosynchronous Fleet:SDO: Solar Dynamics Observatory keeps the Sun under continuous observation at 16 megapixel resolution.GOES: The newest GOES satellites include a solar X-ray imager operated by NOAA.Geospace Fleet:Geotail: Conducts measurements of electrons and ions in the Earth's magnetotail. Cluster: This is a group of four satellites which fly in formation to measure how particles and fields in the magnetosphere vary in space and time. SVS pageTHEMIS: This is a fleet of three satellites to study how magnetospheric instabilities produce substorms. Two of the original five satellites were moved into lunar orbit to become ARTEMIS. SVS page IBEX: The Interstellar Boundary Explorer measures the flux of neutral atoms from the heliopause.Lunar Orbiting FleetARTEMIS: Two of the THEMIS satellites were moved into lunar orbit to study the interaction of the Earth's magnetosphere with the Moon. || ",
            "hits": 91
        },
        {
            "id": 40148,
            "url": "https://svs.gsfc.nasa.gov/gallery/irisnasas-new-eyeonthe-sun/",
            "result_type": "Gallery",
            "release_date": "2013-09-25T00:00:00-04:00",
            "title": "IRIS – Interface Region Imaging Spectrograph",
            "description": "The Interface Region Imaging Spectrograph (IRIS) is a NASA Earth-orbiting observatory focused on a poorly understood area of the Sun's lower atmosphere, the chromosphere. Its primary goal is to study how solar material moves, accumulates energy, and heats up as it travels through this region. IRIS gathers unique data, called spectra, of the chromosphere, which is vital for understanding the Sun's heating process and contributes to more accurate solar storm predictions.\n\nIRIS launched on June 28, 2013, from Vandenberg Air Force Base in California.\n\nLearn more: https://science.nasa.gov/mission/iris/",
            "hits": 61
        },
        {
            "id": 11314,
            "url": "https://svs.gsfc.nasa.gov/11314/",
            "result_type": "Produced Video",
            "release_date": "2013-07-25T13:55:00-04:00",
            "title": "IRIS First Light",
            "description": "The images and video on this page are from the IRIS first light media teleconference on July 25, 2013.For supporting media resources, please click here.On July 17, 2013 at 11:14 pm PDT (2:14 pm EDT) the IRIS Lockheed Martin instrument team successfully opened the door on NASA’s Interface Region Imaging Spectrograph, which launched June 27, 2013, aboard a Pegasus XL rocket from Vandenberg Air Force Base, Calif.As the telescope door opened, IRIS’s single instrument began to observe the sun for the first time. Designed to research the interface region in more detail than has ever been done before, IRIS’s instrument is a combination of an ultraviolet telescope and a spectrograph. The telescope provides high-resolution images, capturing data on about 1 percent of the sun at a time. The images can resolve very fine features, as small as 150 miles across. While the telescope can look at only one wavelength of light at a time, the spectrograph collects information about many wavelengths of light at once. The instrument then splits the sun’s light into its various wavelengths and measures how much of any given wavelength is present. Analysis of the spectral lines can also provide velocity, temperature and density information, key information when trying to track how energy and heat moves through the region. || ",
            "hits": 57
        },
        {
            "id": 11313,
            "url": "https://svs.gsfc.nasa.gov/11313/",
            "result_type": "Produced Video",
            "release_date": "2013-07-19T09:00:00-04:00",
            "title": "IRIS Launch",
            "description": "NASA's Interface Region Imaging Spectrograph (IRIS) solar observatory separated from its Pegasus rocket and is in the proper orbit. This followed a successful launch by the Orbital Sciences Pegasus XL rocket from Vandenberg Air Force Base, Calif. It was the final Pegasus launch currently manifested by NASA. NASA's Launch Services Program at the agency's Kennedy Space Center in Florida managed the countdown and launch.IRIS is a NASA Small Explorer Mission to observe how solar material moves, gathers energy and heats up as it travels through a little-understood region in the sun's lower atmosphere. This interface region between the sun's photosphere and corona powers its dynamic million-degree atmosphere and drives the solar wind.NASA's Interface Region Imaging Spectrograph (IRIS) spacecraft launched Wednesday at 7:27 p.m. PDT (10:27 p.m. EDT) from Vandenberg Air Force Base, Calif. The mission to study the solar atmosphere was placed in orbit by an Orbital Sciences Corporation Pegasus XL rocket. || ",
            "hits": 45
        },
        {
            "id": 11256,
            "url": "https://svs.gsfc.nasa.gov/11256/",
            "result_type": "Produced Video",
            "release_date": "2013-06-19T07:00:00-04:00",
            "title": "IRIS: Studying the Energy Flow that Powers the Solar Atmosphere",
            "description": "In late June 2013, the Interface Region Imaging Spectrograph, or IRIS, will launch from Vandenberg Air Force Base, Calif. IRIS will tease out the rules governing the lowest layers of the solar atmosphere — historically some of the hardest to untangle. Known as the solar interface region, this is one of the most complex areas in the sun's atmosphere: all the energy that drives solar activity travels through it. The interface region lies between the sun’s 6,000-degree, white-hot, visible surface, the photosphere, and the much hotter multi-million-degree upper corona. Interactions between the violently moving plasma and the sun’s magnetic field in this area may well be the source of the energy that heats the corona to its million-degree temperatures, some hundreds and occasionally thousands of times hotter than the sun's surface. The chromosphere is also considered a candidate as the origin for giant explosions on the sun such as solar flares and coronal mass ejections. IRIS will use high-resolution images, data and advanced computer models to unravel how solar gases move, gather energy and heat up through the lower solar atmosphere. Outfitted with state-of-the-art tools, IRIS will be able to tease apart what's happening in the solar interface region better than ever before. || ",
            "hits": 46
        },
        {
            "id": 11286,
            "url": "https://svs.gsfc.nasa.gov/11286/",
            "result_type": "Produced Video",
            "release_date": "2013-06-04T12:00:00-04:00",
            "title": "IRIS L-14 Media Briefing",
            "description": "Lying just above the sun's surface is an enigmatic region of the solar atmosphere called the interface region. A relatively thin region, just 3,000 to 6,000 miles thick, it pulses with movement: zones of different temperature and density are scattered throughout, while energy and heat course through the solar material. Understanding how the energy travels through this region – energy that helps heat the upper layer of the atmosphere, the corona, to temperatures of 1,000,000 kelvins, some thousand times hotter than the sun’s surface itself – is the goal of NASA's Interface Region Imaging Spectrograph, or IRIS, scheduled to launch on June 26, 2013 from California's Vandenberg Air Force Base. Scientists wish to understand the interface region in exquisite detail, since energy flowing through this region has an effect on so many aspects of near-Earth space. For one thing, despite the intense amount of energy deposited into the interface region, only a fraction leaksthrough, but this fraction drives the solar wind, the constant stream of particles that flows out to fill the entire solar system. The interface region is also the source of most of the sun's ultraviolet emission, which impacts both the near-Earth space environment and Earth's climate. IRIS's capabilities are uniquely tailored to unravel the interface region by providing both high-resolution images and a kind of data known as spectra, which can see many wavelengths at once. For its high-resolution images, IRIS will capture data on about one percent of the sun at a time. While these are relatively small snapshots, IRIS will be able to see very fine features, as small as 150 miles across. || ",
            "hits": 60
        },
        {
            "id": 11089,
            "url": "https://svs.gsfc.nasa.gov/11089/",
            "result_type": "Produced Video",
            "release_date": "2012-10-18T14:00:00-04:00",
            "title": "IRIS Launch, Deploy and Beauty Passes",
            "description": "Understanding the interface between the photosphere and corona remains a fundamental challenge in solar and heliospheric science. The Interface Region Imaging Spectrograph (IRIS) mission opens a window of discovery into this crucial region by tracing the flow of energy and plasma through the chromosphere and transition region into the corona using spectrometry and imaging. IRIS is designed to provide significant new information to increase our understanding of energy transport into the corona and solar wind and provide an archetype for all stellar atmospheres. The unique instrument capabilities, coupled with state of the art 3-D modeling, will fill a large gap in our knowledge of this dynamic region of the solar atmosphere. The mission will extend the scientific output of existing heliophysics spacecraft that follow the effects of energy release processes from the sun to Earth.IRIS will provide key insights into all these processes, and thereby advance our understanding of the solar drivers of space weather from the corona to the far heliosphere, by combining high-resolution imaging and spectroscopy for the entire chromosphere and adjacent regions. IRIS will resolve in space, time, and wavelength the dynamic geometry from the chromosphere to the low-temperature corona to shed much-needed light on the physics of this magnetic interface region. || ",
            "hits": 27
        },
        {
            "id": 40046,
            "url": "https://svs.gsfc.nasa.gov/gallery/nasas-heliophysics-gallery/",
            "result_type": "Gallery",
            "release_date": "2010-03-04T00:00:00-05:00",
            "title": "NASA's Heliophysics Gallery",
            "description": "Heliophysics studies the nature of the Sun and how it influences the very nature of space and the planets and the technology that exists there. Learn more at nasa.gov/sun.",
            "hits": 292
        }
    ]
}