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    "results": [
        {
            "id": 5093,
            "url": "https://svs.gsfc.nasa.gov/5093/",
            "result_type": "Visualization",
            "release_date": "2023-04-14T09:00:00-04:00",
            "title": "Solar Eclipse Animation Elements",
            "description": "Due to their relative scale and distances, the disks of the Sun and the Moon appear to be almost the same size in the sky when standing on Earth. This means that even though the Moon is much smaller than the Sun, it can block most or all of the Sun's light, resulting in a dark shadow over Earth called a solar eclipse.These videos are designed to help describe some of the dynamics that determine how solar eclipses work and why they are important for those of us living on Earth. || ",
            "hits": 426
        },
        {
            "id": 13859,
            "url": "https://svs.gsfc.nasa.gov/13859/",
            "result_type": "Produced Video",
            "release_date": "2021-06-18T12:00:00-04:00",
            "title": "Why Does NASA Observe The Sun in Different Colors?",
            "description": "The Solar Dynamics Observatory, or SDO, was launched on Feb. 11, 2010, and began collecting science data a few months later. With two imaging instruments – the Atmospheric Imaging Assembly and the Helioseismic and Magnetic Imager, which were designed in concert to provide complementary views of the Sun – SDO sees the Sun in more than 10 distinct wavelengths of light, showing solar material at different temperatures. SDO also measures the Sun’s magnetic field and the motion of solar material at its surface, and, using a technique called helioseismology, allows scientists to probe deep into the Sun's interior, where the Sun’s complex magnetic fields sprout from. And with more than a decade of observation under its belt, SDO has provided scientists with hundreds of millions of images of our star. || ",
            "hits": 239
        },
        {
            "id": 13184,
            "url": "https://svs.gsfc.nasa.gov/13184/",
            "result_type": "Produced Video",
            "release_date": "2019-04-29T00:00:00-04:00",
            "title": "Goddard at 60",
            "description": "On July 29, 1958, President Eisenhower signed the National Aeronautics and Space Act, establishing the National Aeronautics and Space Administration. When it began operations on October 1, 1958, NASA consisted mainly of the four laboratories and some 80 employees of the government's 46-year-old research agency, the National Advisory Committee for Aeronautics (NACA). Goddard Space Flight Center was established on May 1, 1959 as NASA's first space flight center.In celebration of its 60th year, we look back at the innovations and scientific impacts the women and men of Goddard have made throughout its history. || ",
            "hits": 38
        },
        {
            "id": 13166,
            "url": "https://svs.gsfc.nasa.gov/13166/",
            "result_type": "Produced Video",
            "release_date": "2019-04-09T17:00:00-04:00",
            "title": "Heliophysics Overview",
            "description": "Heliophysics is the study of the Sun, and how it influences the very nature of space — and, in turn, the atmospheres of planets and the technology that exists there. Space is not, as is often believed, completely empty; instead, we live in the extended atmosphere of an active star. Our Sun sends out a steady outpouring of particles and energy -- the solar wind – as well as a constantly writhing magnetic system. This extensive, dynamic solar atmosphere surrounds the Sun, Earth, the planets, and extends far out into the solar system.Studying this system not only helps us understand fundamental information about how the universe works, but also helps protect our technology and astronauts in space. NASA seeks knowledge of near-Earth space, because -- when extreme -- space weather can interfere with our communications, satellites and power grids. The study of the Sun and space can also teach us more about how stars contribute to the habitability of planets throughout the universe.Mapping out this interconnected system requires a holistic study of the Sun’s influence on space, Earth and other planets.  NASA has a fleet of spacecraft strategically placed throughout our heliosphere -- from Parker Solar Probe at the Sun observing the very start of the solar wind, to satellites around Earth, to the farthest human-made object, Voyager, which is sending back observations on interstellar space. Each mission is positioned at a critical, well-thought out vantage point to observe and understand the flow of energy and particles throughout the solar system -- all helping us untangle the effects of the star we live with. || ",
            "hits": 52
        },
        {
            "id": 13159,
            "url": "https://svs.gsfc.nasa.gov/13159/",
            "result_type": "Produced Video",
            "release_date": "2019-03-27T10:00:00-04:00",
            "title": "5 Things About Interstellar Space",
            "description": "5 Things About Interstellar Space || Interstellar_space_thumbnail.jpg (1398x809) [92.2 KB] || Interstellar_space_thumbnail_print.jpg (1024x592) [56.8 KB] || Interstellar_space_thumbnail_searchweb.png (320x180) [52.4 KB] || Interstellar_space_thumbnail_thm.png (80x40) [6.8 KB] || 5ThingsInterstellarFINAL.mp4 (1280x720) [583.2 MB] || 5ThingsInterstellarFINAL.webm (1280x720) [20.0 MB] || 5THINGSABOUTINTERSTELLARSPACE.scc.en_US.srt [3.5 KB] || 5THINGSABOUTINTERSTELLARSPACE.scc.en_US.vtt [3.3 KB] || ",
            "hits": 64
        },
        {
            "id": 13148,
            "url": "https://svs.gsfc.nasa.gov/13148/",
            "result_type": "Produced Video",
            "release_date": "2019-02-12T08:00:00-05:00",
            "title": "5 Things About Earth’s Radiation Donuts",
            "description": "5 Things About Earth’s Radiation Donuts || HalloweenBeltProfile.slate_GSE.HRstills.0000_print.jpg (1024x576) [124.2 KB] || HalloweenBeltProfile.slate_GSE.HRstills.0000.jpg (2560x1440) [721.8 KB] || HalloweenBeltProfile.slate_GSE.HRstills.0000_searchweb.png (320x180) [88.2 KB] || HalloweenBeltProfile.slate_GSE.HRstills.0000_thm.png (80x40) [6.1 KB] || RADIATIONDONUTSSVSV2.mp4 (1280x720) [114.9 MB] || RADIATIONDONUTSSVSV2.webm (1280x720) [12.2 MB] || VanAllenShowCaptions.en_US.srt [2.2 KB] || VanAllenShowCaptions.en_US.vtt [2.2 KB] || ",
            "hits": 74
        },
        {
            "id": 13011,
            "url": "https://svs.gsfc.nasa.gov/13011/",
            "result_type": "Produced Video",
            "release_date": "2018-07-25T00:00:00-04:00",
            "title": "Sounds of the Sun",
            "description": "An illustration of a sunspot inspired by imagery from NASA's Solar Dynamics Observatory (SDO). || sunspot.gif (1280x720) [1.5 MB] || sunspot_searchweb.png (320x180) [95.7 KB] || ",
            "hits": 240
        },
        {
            "id": 13003,
            "url": "https://svs.gsfc.nasa.gov/13003/",
            "result_type": "Produced Video",
            "release_date": "2018-07-20T12:30:00-04:00",
            "title": "Parker Solar Probe Science Briefing - Visual Resources",
            "description": "July 20, 2018 - Live from NASA Kennedy - 1:00 p.m. ESTHosted by Karen Fox - Heliophysics Communications Lead, NASA Goddard/NASA HQSpeakers:Nicola Fox - Parker Solar Probe Project Scientist, The Johns Hopkins University Applied Physics LabAlex Young - Solar Scientist from NASA GoddardThomas Zurbuchen - Associate Administrator for the Science Mission Directorate at NASABetsy Congdon - Thermal Protection System Engineer at The Johns Hopkins University Applied Physics Lab || ",
            "hits": 51
        },
        {
            "id": 12820,
            "url": "https://svs.gsfc.nasa.gov/12820/",
            "result_type": "Produced Video",
            "release_date": "2018-01-04T00:00:00-05:00",
            "title": "Going for GOLD: Exploring the Interface to Space",
            "description": "Going for GOLD: Exploring the Interface to Space || 12820_GOLD_FB_Live.00001_print.jpg (1024x576) [125.3 KB] || 12820_GOLD_FB_Live.00001_searchweb.png (320x180) [84.7 KB] || 12820_GOLD_FB_Live.00001_thm.png (80x40) [6.6 KB] || 12820_GOLD_FB_Live.mp4 (1280x720) [5.1 GB] || 12820_GOLD_FB_Live.mov (1280x720) [41.9 GB] || 12820_GOLD_FB_Live.webm (960x540) [1.7 GB] || 12820_GOLD_FB_Live.en_US.srt [119.6 KB] || 12820_GOLD_FB_Live.en_US.vtt [112.9 KB] || ",
            "hits": 37
        },
        {
            "id": 12061,
            "url": "https://svs.gsfc.nasa.gov/12061/",
            "result_type": "Produced Video",
            "release_date": "2017-08-07T12:00:00-04:00",
            "title": "Eclipse Safety",
            "description": "Learn how to watch the 2017 American Eclipse safely. || BillIngalls_16x9.jpg (1153x649) [267.3 KB] || BillIngalls_1024x576.jpg (1024x576) [227.9 KB] || BillIngalls_1024x576_thm.png (80x40) [7.7 KB] || BillIngalls_1024x576_searchweb.png (320x180) [106.1 KB] || ",
            "hits": 194
        },
        {
            "id": 4579,
            "url": "https://svs.gsfc.nasa.gov/4579/",
            "result_type": "Visualization",
            "release_date": "2017-06-21T05:00:00-04:00",
            "title": "Flying Around The Eclipse Shadow",
            "description": "A view of the Moon's shadow during the August 21, 2017 eclipse from both the night and day sides of the Earth. || night_to_day.0300_print.jpg (1024x576) [47.6 KB] || night_to_day.0300_searchweb.png (320x180) [28.2 KB] || night_to_day.0300_thm.png (80x40) [3.2 KB] || eclipse_flyaround_1080p30.mp4 (1920x1080) [36.2 MB] || eclipse_flyaround_720p30.mp4 (1280x720) [12.7 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || eclipse_flyaround_720p30.webm (1280x720) [5.4 MB] || eclipse_flyaround_720p30.wmv (1280x720) [42.8 MB] || FlyingAroundTheEclipseShadow.mov (1280x720) [682.8 MB] || eclipse_flyaround_360p30.mp4 (640x360) [4.3 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || eclipse_flyaround_2160p30.mp4 (3840x2160) [122.4 MB] || FlyingAroundTheEclipseShadow4k.mov (3840x2160) [2.4 GB] || eclipse_flyaround_1080p30.mp4.hwshow [222 bytes] || ",
            "hits": 74
        },
        {
            "id": 12458,
            "url": "https://svs.gsfc.nasa.gov/12458/",
            "result_type": "Produced Video",
            "release_date": "2017-06-12T12:00:00-04:00",
            "title": "Shadow of the Eclipse",
            "description": "See the most accurate map for Aug 21, 2017's total solar eclipse. || usa_eclipse_map_16x9_1920x1080_1024x576.jpg (1024x576) [212.7 KB] || usa_eclipse_map_16x9_1920x1080_1920x1080.jpg (1920x1080) [700.1 KB] || usa_eclipse_map_16x9_1920x1080_1920x1080_thm.png (80x40) [8.0 KB] || usa_eclipse_map_16x9_1920x1080_1024x576_searchweb.png (320x180) [110.9 KB] || usa_eclipse_map_16x9_1920x1080.tif (1920x1080) [3.9 MB] || usa_eclipse_map_16x9.tif (4800x2700) [21.5 MB] || ",
            "hits": 86
        },
        {
            "id": 12533,
            "url": "https://svs.gsfc.nasa.gov/12533/",
            "result_type": "Produced Video",
            "release_date": "2017-05-18T11:00:00-04:00",
            "title": "Science Comes Alive at NASA Goddard",
            "description": "Science Comes Alive at NASA Goddard   TRT: 3:35Music Credit: Killer TracksOld River [CM099]Mainframe Disturbance [ICON007]Never Lost Combat [KOK2425]Simple Logic [CM099]Shout [CM116]Hope for Change [NYB120]Illuminating [KT332]Breaking the Atmosphere [ICON013]Chop It Up [KT332] || 12533_At_NASA_Goddard_Promo_w_Title_youtube_hq.00001_print.jpg (1024x576) [25.3 KB] || 12533_At_NASA_Goddard_Promo_w_Title_appletv.m4v (1280x720) [139.9 MB] || 12533_At_NASA_Goddard_Promo_w_Title.webm (960x540) [106.0 MB] || 12533_At_NASA_Goddard_Promo_w_Title_appletv_subtitles.m4v (1280x720) [140.0 MB] || 12533_At_NASA_Goddard_Promo_LONG_w_Title.en_US.srt [5.1 KB] || 12533_At_NASA_Goddard_Promo_LONG_w_Title.en_US.vtt [4.9 KB] || 12533_At_NASA_Goddard_Promo_w_Title_youtube_hq.mov (1920x1080) [1.5 GB] || 12533_At_NASA_Goddard_Promo_w_Title_prores.mov (1280x720) [3.6 GB] || 12533_At_NASA_Goddard_Promo_w_Title.mov (1920x1080) [6.8 GB] || ",
            "hits": 56
        },
        {
            "id": 12481,
            "url": "https://svs.gsfc.nasa.gov/12481/",
            "result_type": "Produced Video",
            "release_date": "2017-03-27T12:00:00-04:00",
            "title": "2017's All American Solar Eclipse",
            "description": "On August 21, 2017, a solar eclipse will be visible across North America. || usa_suns.0750_print.jpg (1024x576) [140.4 KB] || usa_suns.0750_1024x576.jpg (1024x576) [129.2 KB] || usa_suns.0750_searchweb.png (320x180) [88.7 KB] || usa_suns.0750_thm.png (80x40) [6.9 KB] || usa_suns.0750.tif (1920x1080) [5.0 MB] || ",
            "hits": 201
        },
        {
            "id": 4552,
            "url": "https://svs.gsfc.nasa.gov/4552/",
            "result_type": "Visualization",
            "release_date": "2017-02-06T00:00:00-05:00",
            "title": "2017 Eclipse State Maps",
            "description": "The path of totality passes through 14 states during the total solar eclipse on August 21, 2017. A map of each of these states, created for NASA's official eclipse 2017 website, is presented here. Except for Montana, each map is 8 inches wide (or high) at 300 DPI. The umbra is shown at 3-minute intervals, with times in the local time zone at the umbra center. The duration of totality is outlined in 30-second increments. Interstate highways are blue, other major roads are red, and secondary roads are gray.Some sources list only 12 states for this eclipse, but in fact the path of totality also grazes the southwestern borders of both Montana and Iowa. The Montana part of the path is in a roadless area at the southern end of the Beaverhead Mountains, a range that defines sections of both the Montana-Idaho border and the Continental Divide. The Iowa part of the path is west of Interstate 29 near Hamburg, south of 310 Street, and bounded on the west by the Missouri River. It includes the Lower Hamburg Bend Wildlife Management Area. || ",
            "hits": 100
        },
        {
            "id": 11905,
            "url": "https://svs.gsfc.nasa.gov/11905/",
            "result_type": "Produced Video",
            "release_date": "2015-06-23T12:00:00-04:00",
            "title": "Space Weather Imagery of June 22 - 23, 2015 Events",
            "description": "The sun emitted a CME and mid-level solar flare, peaking at 2:23 p.m. EDT, on June 22, 2015. Again on June 25, 2015, a mid-level solar flare peaked at 4:16 a.m. EDT.NASA’s Solar Dynamics Observatory, which watches the sun constantly, captured an image of the event. Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth's atmosphere to physically affect humans on the ground, however -- when intense enough -- they can disturb the atmosphere in the layer where GPS and communications signals travel.  To see how this event may affect Earth, please visit NOAA's Space Weather Prediction Center at http://spaceweather.gov, the U.S. government's official source for space weather forecasts, alerts, watches and warnings. This first flare is classified as an M6.6 flare and the second was M7.9. M-class flares are a tenth the size of the most intense flares, the X-class flares. The number provides more information about its strength. An M2 is twice as intense as an M1, an M3 is three times as intense, etc. || ",
            "hits": 65
        },
        {
            "id": 11696,
            "url": "https://svs.gsfc.nasa.gov/11696/",
            "result_type": "Produced Video",
            "release_date": "2014-12-25T11:00:00-05:00",
            "title": "Twisted Solar Blob",
            "description": "NASA’s Solar Dynamics Observatory (SDO) monitors the sun 24/7, recording its outbursts in high-definition. On September 26, 2014, the spacecraft captured a twisted blob of plasma erupting in a dramatic liftoff. The plasma, which is ionized helium cooked to over 100,000 degrees Fahrenheit, corkscrewed outward along the path of the sun's complex magnetic field. Like densely looped carpeting, magnetic field lines crisscross through the sun's surface and outer layers. This weave usually prevents plasma from escaping. But if the magnetic field lines become unsteady or suddenly align into new patterns, a filament can whip into space. Watch the video to see the event unfold. || ",
            "hits": 72
        },
        {
            "id": 11720,
            "url": "https://svs.gsfc.nasa.gov/11720/",
            "result_type": "Produced Video",
            "release_date": "2014-11-20T00:00:00-05:00",
            "title": "Sunspot Live Shots 2014",
            "description": "Canned interviews for Sunspot live shot 11/20/2014 || Alex_Young_Canned_interview_youtube_hq_print.jpg (1024x576) [102.0 KB] || Alex_Young_Canned_interview_youtube_hq_web.png (320x180) [86.5 KB] || Alex_Young_Canned_interview_youtube_hq_thm.png (80x40) [6.8 KB] || Alex_Young_Canned_interview_appletv.m4v (960x540) [86.6 MB] || Alex_Young_Canned_interview_appletv.webmhd.webm (960x540) [40.6 MB] || Alex_Young_Canned_interview_appletv_subtitles.m4v (960x540) [86.7 MB] || Alex_Young_Canned_interview_1280x720.wmv (1280x720) [106.0 MB] || Alex_Young_Canned_interview_youtube_hq.mov (1280x720) [289.0 MB] || Alex_Young_Canned_interview_ipod_lg.m4v (640x360) [34.0 MB] || Alex_Young_Canned_Interview.en_US.srt [4.0 KB] || Alex_Young_Canned_Interview.en_US.vtt [4.0 KB] || Alex_Young_Canned_interview_nasaportal.mov (640x360) [86.1 MB] || Alex_Young_Canned_interview_ipod_sm.mp4 (320x240) [18.0 MB] || Alex_Young_Canned_interview_prores.mov (1280x720) [3.1 GB] || ",
            "hits": 34
        },
        {
            "id": 11602,
            "url": "https://svs.gsfc.nasa.gov/11602/",
            "result_type": "Produced Video",
            "release_date": "2014-07-03T11:00:00-04:00",
            "title": "STEREO Solar Conjunction",
            "description": "Since February 2011, the two spacecraft of NASA's STEREO mission have been providing scientists with unprecedented views of the far side of the sun. Placed in an orbit that allows their perspective to changed over the eight years since their launch in 2008 (ck), the satellites are about to enter a new phase of their journey: a time when the bright light and heat of the sun will stand in the way of sending data back to Earth.This phase is a direct result of the orbits for STEREO, which is short for the Solar Terrestrial Relations Observatory. The spacecraft travel at different speeds. This means that over time, the satellites become increasingly out of sync, appearing from Earth's perspective to drift farther apart, able to observe first the sides and eventually the far side of the sun. For the first time ever, thanks to STEREO and near-Earth solar telescopes such as NASA’s Solar Dynamics Observatory the human race has had its first 360-degree view of the sun.The orbits have continued to cause the STEREO spacecraft's position to change, however, and now they are nearing each other once again, this time on the other side of the sun. During this period when the sun blocks Earth's view — a geometrical position known in astronomy as a superior conjunction — radio receivers on Earth will not be able to distinguish STEREO's signal from the sun's radiation. Communication with the spacecraft will cease and the satellites will both go into safe mode without collecting data for a time. This will happen for STEREO-Ahead from March 24 to July 7, 2015. STEREO-Behind will be in superior conjunction from Jan. 22 to March 23, 2015. At least one spacecraft, therefore, will always be collecting data. Before this occurs, the heating from the sun will also begin to affect – though not shut down — data collection. From wherever they are in space, the STEREO spacecraft aim their antenna toward Earth to send down data. This position puts the antenna fairly close to pointing at the sun, exposing the instruments to more heat than it can safely bear. The antenna can be adjusted to point in different directions, but the signal coming to Earth will be much fainter and won't allow for as much data to be downloaded.  This antenna adjustment will begin on Aug. 20, 2014, for the STEREO-Ahead spacecraft and on Dec. 1, 2014, for STEREO-Behind. During this phase, STEREO instruments will continue to run 24 hours a day, but they will gather lower-resolution data than usual. Some of this data will be downloaded whenever STEREO can link up with an Earth receiver. The rest of the data will be stored on board to be downloaded when the spacecraft reach a more auspicious geometrical position in early 2016. To test for this off-pointing from the sun, STEREO-Ahead will undergo tests and not be collecting data from July 6-12, 2014.  The same tests will be performed on STEREO-Behind from Sept. 29 – Oct. 6, 2014. Throughout this entire phase until 2016, at least one STEREO spacecraft will be capturing data at any one time, so scientists will have an uninterrupted record of events on the sun to coordinate with the observations of solar telescopes on the Earth side. Real time monitoring of the sun, its flares and coronal mass ejections – information used by the US National Oceanic and Atmospheric Administration to help forecast space weather — will also continue via a fleet of NASA spacecraft closer to Earth. || ",
            "hits": 68
        },
        {
            "id": 11419,
            "url": "https://svs.gsfc.nasa.gov/11419/",
            "result_type": "Produced Video",
            "release_date": "2014-01-07T00:00:00-05:00",
            "title": "Pole Reversal",
            "description": "Like a bar magnet, the sun has a magnetic north and south pole. The comparison to a simple bar magnet ends there, however, as the sun's magnetic fields are on the move. In fact, approximately every 11 years the polarity of the sun’s northern and southern hemisphere flips. This change is part of a regular cycle called the solar cycle. Each cycle is defined by periods of high and low solar activity caused by the movement of magnetic field lines that extend out from the sun. Now, a new animation created from data collected by the ESA/NASA SOHO spacecraft shows how migrating magnetic field lines result in a reversal of the sun’s polarity. Watch the video to see the evolution of the sun’s magnetic field from January 1997 to December 2013. || ",
            "hits": 306
        },
        {
            "id": 11418,
            "url": "https://svs.gsfc.nasa.gov/11418/",
            "result_type": "Produced Video",
            "release_date": "2014-01-02T00:00:00-05:00",
            "title": "Solar Continuum",
            "description": "Many of the sun's features are invisible to the naked eye. To paint a full picture of our constantly changing star, scientists use telescopes launched into space. Each telescope is outfitted with special filters that can see the sun in different wavelengths of light. To track how material and heat of different temperature moves through the sun's atmosphere, scientists only need to select the specific wavelength with which a feature can best be seen. Watch the video for a tour of the wide range of wavelengths that NASA's Solar Dynamics Observatory spacecraft uses to observe the sun. || ",
            "hits": 74
        },
        {
            "id": 11416,
            "url": "https://svs.gsfc.nasa.gov/11416/",
            "result_type": "Produced Video",
            "release_date": "2013-12-26T00:00:00-05:00",
            "title": "Death Of A Comet",
            "description": "Comet ISON was born along with the solar system some 4.5 billion years ago. But after a close encounter with the sun, its time has finally come to an end. On November 28, 2013, the comet shot around the sun on a dangerous trajectory that brought it within 700,000 miles of the surface. As it disappeared from view of sun-observing spacecraft, scientists waited with bated breath to learn of its fate. Would the comet disintegrate in the fierce heat and gravity of the sun or remain intact? Some remnant of the comet did indeed survive the trip around the sun, but it quickly dimmed and fizzled, signaling a close to ISON's magnificent journey through space. Watch the video for a look at Comet ISON’s final moments. || ",
            "hits": 98
        },
        {
            "id": 4128,
            "url": "https://svs.gsfc.nasa.gov/4128/",
            "result_type": "Visualization",
            "release_date": "2013-12-24T00:00:00-05:00",
            "title": "Solar Dynamics Observatory - Argo view - Slices of SDO",
            "description": "Argos (or Argus Panoptes) was the 100-eyed giant in Greek mythology (wikipedia).While the Solar Dynamics Observatory (SDO) has significantly less than 100 eyes, (see \"SDO Jewelbox: The Many Eyes of SDO\"), seeing connections in the solar atmosphere through the many filters of SDO presents a number of interesting challenges. This visualization experiment illustrates a mechanism for highlighting these connections. This visualization is a variation of the original Solar Dynamics Observatory - Argo view. In this case, the different wavelength filters are presented in three sets around the Sun at full 4Kx4K resolution. This enables monitoring of changes in time over all wavelengths at any location around the limb of the Sun. The wavelengths presented are: 617.3nm optical light from SDO/HMI. From SDO/AIA we have 170nm (pink), then 160nm (green), 33.5nm (blue), 30.4nm (orange), 21.1nm (violet), 19.3nm (bronze), 17.1nm (gold), 13.1nm (aqua) and 9.4nm (green).We've locked the camera to rotate the view of the Sun so each wedge-shaped wavelength filter passes over a region of the Sun. As the features pass from one wavelength to the next, we can see dramatic differences in solar structures that appear in different wavelengths.Filaments extending off the limb of the Sun which are bright in 30.4 nanometers, appear dark in many other wavelengths.Sunspots which appear dark in optical wavelengths, are festooned with glowing ribbons in ultraviolet wavelengths.small flares, invisible in optical wavelengths, are bright ribbons in ultraviolet wavelengths.if we compare the visible light limb of the Sun with the 170 nanometer filter on the left, with the visible light limb and the 9.4 nanometer filter on the right, we see that the 'edge' is at different heights. This effect is due to the different amounts of absorption, and emission, of the solar atmosphere in ultraviolet light.in far ultraviolet light, the photosphere is dark since the black-body spectrum at a temperature of 5700 Kelvin emits very little light in this wavelength. || ",
            "hits": 65
        },
        {
            "id": 4117,
            "url": "https://svs.gsfc.nasa.gov/4117/",
            "result_type": "Visualization",
            "release_date": "2013-12-17T10:00:00-05:00",
            "title": "Solar Dynamics Observatory - Argo view",
            "description": "Argos (or Argus Panoptes) was the 100-eyed giant in Greek mythology (wikipedia).While the Solar Dynamics Observatory (SDO) has significantly less than 100 eyes, (see \"SDO Jewelbox: The Many Eyes of SDO\"), seeing connections in the solar atmosphere through the many filters of SDO presents a number of interesting challenges. This visualization experiment illustrates a mechanism for highlighting these connections.The wavelengths presented are: 617.3nm optical light from SDO/HMI. From SDO/AIA we have 170nm (pink), then 160nm (green), 33.5nm (blue), 30.4nm (orange), 21.1nm (violet), 19.3nm (bronze), 17.1nm (gold), 13.1nm (aqua) and 9.4nm (green).We've locked the camera to rotate the view of the Sun so each wedge-shaped wavelength filter passes over a region of the Sun. As the features pass from one wavelength to the next, we can see dramatic differences in solar structures that appear in different wavelengths.Filaments extending off the limb of the Sun which are bright in 30.4 nanometers, appear dark in many other wavelengths.Sunspots which appear dark in optical wavelengths, are festooned with glowing ribbons in ultraviolet wavelengths.Small flares, invisible in optical wavelengths, are bright ribbons in ultraviolet wavelengths.If we compare the visible light limb of the Sun with the 170 nanometer filter on the left, with the visible light limb and the 9.4 nanometer filter on the right, we see that the 'edge' is at different heights. This effect is due to the different amounts of absorption, and emission, of the solar atmosphere in ultraviolet light.In far ultraviolet light, the photosphere is dark since the black-body spectrum at a temperature of 5700 Kelvin emits very little light in this wavelength. || ",
            "hits": 95
        },
        {
            "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": 104
        },
        {
            "id": 11373,
            "url": "https://svs.gsfc.nasa.gov/11373/",
            "result_type": "Produced Video",
            "release_date": "2013-12-12T00:00:00-05:00",
            "title": "Canyon Of Fire",
            "description": "In September 2013, a 200,000-mile-long loop of solar material erupted in the sun's atmosphere leaving behind what looks like a canyon of fire. These giant loops, called filaments, consist of charged particles held in place by magnetic fields that extend out from the sun’s surface. On September 29-30, NASA’s Solar Dynamics Observatory spacecraft watched as a filament about 25 times the Earth’s width expanded and then collapsed just north of the sun’s equator. Moments later, it saw a glowing canyon trace the channel where magnetic fields held the structure aloft. Watch the video to see the event unfold. || ",
            "hits": 23
        },
        {
            "id": 11429,
            "url": "https://svs.gsfc.nasa.gov/11429/",
            "result_type": "Produced Video",
            "release_date": "2013-12-05T17:00:00-05:00",
            "title": "Sun Magnetic Field Flip Live Shots and Media Resources",
            "description": "On Dec. 6, 2013, NASA scientists Alex Young and Holly Gilbert discussed how the sun's magnetic field is in the process of flipping. || ",
            "hits": 117
        },
        {
            "id": 11270,
            "url": "https://svs.gsfc.nasa.gov/11270/",
            "result_type": "Produced Video",
            "release_date": "2013-06-11T00:00:00-04:00",
            "title": "1,000 Days Of The Sun",
            "description": "In the spring of 2010, NASA’s Solar Dynamics Observatory, or SDO, provided its first views of the sun. Since then the spacecraft has had virtually unbroken coverage of our star, capturing one image every 12 seconds in 10 different wavelengths. The collection of images chronicles the sun’s rise toward solar maximum, the peak of solar activity in its regular 11-year cycle. Repeatedly caught in the act were solar flares and coronal mass ejections, powerful eruptions that can send radiation and solar material toward Earth and interfere with satellite operations in space. SDO’s constant monitoring of the sun help scientists understand what causes these giant explosions—with the goal of someday improving our ability to predict this space weather. Watch the video to see a time-lapse sequence of SDO observations that spans three years in the life of the sun. || ",
            "hits": 60
        },
        {
            "id": 11198,
            "url": "https://svs.gsfc.nasa.gov/11198/",
            "result_type": "Produced Video",
            "release_date": "2013-03-28T00:00:00-04:00",
            "title": "Raindrops Falling On The Sun",
            "description": "On July 19, 2012, million-degree plasma in the sun's atmosphere began to cool and fall to the surface, resulting in a dazzling magnetic display known as coronal rain. Because the plasma is charged, it's strongly influenced by the sun's magnetic field. As it rained down, it condensed along twisted magnetic field lines close to the surface and formed giant streaming arcs, some as tall as five Earths stacked high. An ultra high-definition telescope aboard NASA's Solar Dynamics Observatory (SDO) captured images of the display, which lasted hours and was initiated by two eruptive events on the sun: a solar flare and coronal mass ejection. Scientists used a 304-angstrom-wavelength filter to see the plasma downpour. Watch the video to see it for yourself. || ",
            "hits": 218
        },
        {
            "id": 11105,
            "url": "https://svs.gsfc.nasa.gov/11105/",
            "result_type": "Produced Video",
            "release_date": "2012-10-23T00:00:00-04:00",
            "title": "Gradient Sun",
            "description": "Scientific imagery can be stunning. There's a simple reason why: the same tools to create art are often used in the pursuit of science. One such tool, recognizable to many people as an image effect available on digital photo editing programs, is the gradient filter. When applied to images, the filter sharpens detail by boosting contrast. Scientists use it to accentuate fine structures that might otherwise be lost in the background noise of some scenes. Applying the filter to satellite views of the sun, for example, enhances the giant arcs of solar material in the sun's atmosphere called coronal loops. By studying these loops, scientists can track the structure and movement of magnetic fields that drive the creation of sunspots and giant radiation bursts known as solar flares. Watch the video to see the eye-catching effect this filter has on images of the sun captured by NASA's Solar Dynamics Observatory satellite. || ",
            "hits": 17
        },
        {
            "id": 10941,
            "url": "https://svs.gsfc.nasa.gov/10941/",
            "result_type": "Produced Video",
            "release_date": "2012-04-24T10:00:00-04:00",
            "title": "Space Weather FAQ Interviews",
            "description": "NASA scientists answer some frequently asked questions about the sun, space weather, and the effects on Earth. Each video is one or more scientists responding to the question above it. The videos are available as ProRes files for broadcast use and have had minor audio equalizing and color correction applied.The scientists interviewed are:Dr. Holly Gilbert, NASA HeliophysicistDr. Alex Young, NASA HeliophysicistDr. Phil Chamberlin, NASA Research Heliophysicist and SDO Deputy Project ScientistThere are also two short videos created with this interview content. They are available here.Additional responses to these questions are available upon specific request.For space weather-related footage, animations, and features, visit the Space Weather gallery. || ",
            "hits": 32
        },
        {
            "id": 10959,
            "url": "https://svs.gsfc.nasa.gov/10959/",
            "result_type": "Produced Video",
            "release_date": "2012-04-24T10:00:00-04:00",
            "title": "NASA Scientists Answer Top Space Weather Questions",
            "description": "NASA scientists answer some common questions about the sun, space weather, and how they affect the Earth. This is a two-part series.Part One addresses:1. What is space weather?2. What are coronal mass ejections?3. What are solar flares?4. What are solar energetic particles?5. What causes flares and CMEs?Part Two addresses:1. Do all flares and CMEs affect the Earth?2. What happens when a flare or CME hits the Earth?3. How quickly can we feel the effects of space weather?4. Why are there more flares and CMEs happening now?For more information about all these questions and more, visit NASA's Space Weather FAQ.For individual interview responses to frequently asked space weather questions, go here. || ",
            "hits": 35
        },
        {
            "id": 10754,
            "url": "https://svs.gsfc.nasa.gov/10754/",
            "result_type": "Produced Video",
            "release_date": "2011-11-10T00:00:00-05:00",
            "title": "The Truth About 2012: Solar Storms",
            "description": "Should we be concerned about solar storms in 2012? Heliophysicist Alex Young from NASA Goddard Space Flight Center sorts out truth from fiction. || ",
            "hits": 38
        },
        {
            "id": 10421,
            "url": "https://svs.gsfc.nasa.gov/10421/",
            "result_type": "Produced Video",
            "release_date": "2009-04-07T00:00:00-04:00",
            "title": "SOHO/TRACE Intro",
            "description": "On April 3, 2009, countries from around the world participated in the '100 Hours of Astronomy' webcast to celebrate the International Year of Astronomy. This movie was used to introduce the SOHO/TRACE segment. Alex Young and Dawn Meyers, NASA scientists, describe how both SOHO and TRACE view the sun in their own unique way. || ",
            "hits": 47
        },
        {
            "id": 10287,
            "url": "https://svs.gsfc.nasa.gov/10287/",
            "result_type": "Produced Video",
            "release_date": "2008-07-15T12:00:00-04:00",
            "title": "Get Ready for the August 1, 2008 Total Solar Eclipse",
            "description": "On August 1, 2008 a rare total solar eclipse will appear in the skies over parts of Canada, Greenland, Russia, Mongolia, and China. During this spectacular event, the moon will cross in front of the sun, completely blocking out the sun's disk, and casting a shadow over part of the Earth. While only people in a small area of the world will be able to see the eclipse in person, viewers all accross the globe can view the eclipse as it happens on NASA TV and www.nasa.gov. || ",
            "hits": 111
        }
    ]
}