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    "results": [
        {
            "id": 31380,
            "url": "https://svs.gsfc.nasa.gov/31380/",
            "result_type": "Hyperwall Visual",
            "release_date": "2026-03-30T12:00:00-04:00",
            "title": "APEX-12 (Advanced Plant EXperiment-12) on the ISS",
            "description": "The findings of the APEX series of experiments offer insight into the effects of spaceflight on plant chromosomes, and how these findings could impact human health.",
            "hits": 318
        },
        {
            "id": 14932,
            "url": "https://svs.gsfc.nasa.gov/14932/",
            "result_type": "Produced Video",
            "release_date": "2025-12-02T08:00:00-05:00",
            "title": "Bio-Essential Sugars Discovered in Samples from Asteroid Bennu",
            "description": "OSIRIS-REx Project Scientist Daniel Glavin discusses the discovery of ribose and glucose in samples of asteroid Bennu, and the implications for the formation and evolution of life on Earth.Complete transcript available.Watch this video on the NASA.gov Video YouTube channel. || Bennu-Sugars-Thumbnail_print.jpg (1024x576) [175.2 KB] || Bennu-Sugars-Thumbnail.jpg (1280x720) [534.2 KB] || Bennu-Sugars-Thumbnail.png (1280x720) [892.3 KB] || Bennu-Sugars-Thumbnail_searchweb.png (320x180) [77.4 KB] || Bennu-Sugars-Thumbnail_thm.png (80x40) [6.8 KB] || 14932_Bennu_Sugars_Interview_Glavin_720.mp4 (1280x720) [180.6 MB] || 14932_Bennu_Sugars_Interview_Glavin_1080.mp4 (1920x1080) [1011.6 MB] || BennuSugarsGlavinCaptionsV2.en_US.srt [18.4 KB] || BennuSugarsGlavinCaptionsV2.en_US.vtt [17.5 KB] || 14932_Bennu_Sugars_Interview_Glavin_4K.mp4 (3840x2160) [6.2 GB] || 14932_Bennu_Sugars_Interview_Glavin_ProRes.mov (3840x2160) [47.0 GB] || ",
            "hits": 247
        },
        {
            "id": 14772,
            "url": "https://svs.gsfc.nasa.gov/14772/",
            "result_type": "B-Roll",
            "release_date": "2025-01-29T11:00:00-05:00",
            "title": "Discoveries from Asteroid Bennu: Media Briefing Graphics",
            "description": "OSIRIS-REx MISSION RECAPThis highlight reel recaps the OSIRIS-REx mission, from assembly and launch of the spacecraft in 2016, to arrival at asteroid Bennu in 2018, TAG sample collection in 2020, the delivery of the sample to Earth in 2023, and curation of the Bennu samples in 2024.Credit: NASA || OSIRIS-REx_Collier_Present_2024_Preview_print.jpg (1024x576) [180.7 KB] || OSIRIS-REx_Collier_Present_2024_Preview.png (3840x2160) [8.3 MB] || OSIRIS-REx_Collier_Present_2024_Preview_searchweb.png (320x180) [116.3 KB] || OSIRIS-REx_Collier_Present_2024_Preview_thm.png [9.7 KB] || OSIRIS-REx_Collier_Present_2024_V3_Small.mp4 (1920x1080) [179.0 MB] || OSIRIS-REx_Collier_Present_2024_V3_Medium.mp4 (3840x2160) [500.9 MB] || OSIRIS-REx_Collier_Present_2024_V3_Large.mp4 (3840x2160) [1.6 GB] || ",
            "hits": 499
        },
        {
            "id": 14774,
            "url": "https://svs.gsfc.nasa.gov/14774/",
            "result_type": "Produced Video",
            "release_date": "2025-01-29T11:00:00-05:00",
            "title": "NASA Finds Ingredients of Life in Fragments of Lost World",
            "description": "Scientists studying the Bennu samples have discovered evidence of a wet, salty environment from 4.5 billion years ago that created the molecular building blocks of life.Complete transcript available.Universal Production Music: “Future Tense” by Gresby Race Nash [PRS]; “Take Off” by Nicholas Smith [PRS]; “Big Decision” by Gresby Race Nash [PRS]; “Waiting for the Answer” by Gresby Race Nash [PRS]Watch this video on the NASA Goddard YouTube channel. || 14774-Bennu-Organics-Thumbnail-V4_print.jpg (1024x576) [395.9 KB] || 14774-Bennu-Organics-Thumbnail-V4.jpg (1280x720) [1.2 MB] || 14774-Bennu-Organics-Thumbnail-V4.png (1280x720) [1.8 MB] || 14774-Bennu-Organics-Thumbnail-V4_searchweb.png (320x180) [120.2 KB] || 14774-Bennu-Organics-Thumbnail-V4_thm.png [8.3 KB] || 14774_OSIRIS-REx_Bennu_Organics_720.mp4 (1280x720) [66.1 MB] || 14774_OSIRIS-REx_Bennu_Organics_1080.mp4 (1920x1080) [370.5 MB] || BennuOrganicsCaptions.en_US.srt [6.4 KB] || BennuOrganicsCaptions.en_US.vtt [6.0 KB] || 14774_OSIRIS-REx_Bennu_Organics_4K.mp4 (3840x2160) [2.3 GB] || 14774_OSIRIS-REx_Bennu_Organics_ProRes.mov (3840x2160) [14.5 GB] || ",
            "hits": 382
        },
        {
            "id": 13325,
            "url": "https://svs.gsfc.nasa.gov/13325/",
            "result_type": "Produced Video",
            "release_date": "2019-09-24T13:00:00-04:00",
            "title": "The Nancy Grace Roman Space Telescope's Coronagraph Instrument",
            "description": "Watch this video to learn more about the Roman Space Telescope's coronagraph instrument.Credit: NASA's Goddard Space Flight CenterMusic: \"Concept of Motion\" from Universe Production MusicComplete transcript available. || Roman_CGI_Still.jpg (1920x1080) [396.1 KB] || 13325_Roman_CGI_1080.mp4 (1920x1080) [96.8 MB] || 13325_Roman_CGI_Final_ProRes_1920x1080_2997.mov (1920x1080) [1.3 GB] || 13325_Roman_CGI_1080.webm (1920x1080) [13.9 MB] || Roman_CGI_SRT_Captions.en_US.srt [2.4 KB] || Roman_CGI_SRT_Captions.en_US.vtt [2.4 KB] || ",
            "hits": 130
        },
        {
            "id": 12869,
            "url": "https://svs.gsfc.nasa.gov/12869/",
            "result_type": "Produced Video",
            "release_date": "2018-02-28T00:00:00-05:00",
            "title": "Excellence is in our DNA",
            "description": "Excellence Is In Our DNA (General Purpose Version)Music Credit: Killer Tracks - Track Title:Vibin [KT355] || 12869_Lifeblood_of_Goddard_general_appletv.00955_print.jpg (1024x576) [73.5 KB] || 12869_Lifeblood_of_Goddard_general_appletv.00955_searchweb.png (320x180) [78.9 KB] || 12869_Lifeblood_of_Goddard_general_appletv.00955_thm.png (80x40) [6.9 KB] || 12869_Lifeblood_of_Goddard_general_appletv.m4v (1280x720) [21.3 MB] || 12869_Lifeblood_of_Goddard_general_appletv_subtitles.m4v (1280x720) [21.3 MB] || 12869_Lifeblood_of_Goddard_general.mov (1280x720) [593.4 MB] || 12869_Lifeblood_of_Goddard_general.webm (960x540) [18.5 MB] || 12869_Lifeblood_of_Goddard.en_US.vtt [601 bytes] || 12869_Lifeblood_of_Goddard.en_US.srt [628 bytes] || ",
            "hits": 11
        },
        {
            "id": 12281,
            "url": "https://svs.gsfc.nasa.gov/12281/",
            "result_type": "Produced Video",
            "release_date": "2016-06-10T18:00:00-04:00",
            "title": "Instagram: Solar Storms May Have Been Key to Life on Earth",
            "description": "Our sun's adolescence was stormy—and new evidence shows that these tempests may have been just the key to seeding life as we know it.Some 4 billion years ago, the sun shone with only about three-quarters the brightness we see today, but its surface roiled with giant eruptions spewing enormous amounts of solar material and radiation out into space. These powerful solar explosions may have provided the crucial energy needed to warm Earth, despite the sun's faintness. The eruptions also may have furnished the energy needed to turn simple molecules into the complex molecules such as RNA and DNA that were necessary for life. The research was published in Nature Geoscience on May 23, 2016, by a team of scientists from NASA.Understanding what conditions were necessary for life on our planet helps us both trace the origins of life on Earth and guide the search for life on other planets. Until now, however, fully mapping Earth's evolution has been hindered by the simple fact that the young sun wasn't luminous enough to warm Earth.\"Back then, Earth received only about 70 percent of the energy from the sun than it does today,\" said Vladimir Airapetian, lead author of the paper and a solar scientist at NASA's Goddard Space Flight Center in Greenbelt, Maryland. \"That means Earth should have been an icy ball. Instead, geological evidence says it was a warm globe with liquid water. We call this the Faint Young Sun Paradox. Our new research shows that solar storms could have been central to warming Earth.\" || ",
            "hits": 60
        },
        {
            "id": 12267,
            "url": "https://svs.gsfc.nasa.gov/12267/",
            "result_type": "Produced Video",
            "release_date": "2016-06-09T11:00:00-04:00",
            "title": "How Earth Lost Its Cool",
            "description": "Scientists think solar storms may have been key to warming our planet. || c-1024.jpg (1024x576) [165.2 KB] || c-1280.jpg (1280x720) [234.6 KB] || c-1920.jpg (1920x1080) [360.8 KB] || c-1024_print.jpg (1024x576) [172.3 KB] || c-1024_searchweb.png (320x180) [93.6 KB] || c-1024_web.png (320x180) [93.6 KB] || c-1024_thm.png (80x40) [20.3 KB] || ",
            "hits": 79
        },
        {
            "id": 11853,
            "url": "https://svs.gsfc.nasa.gov/11853/",
            "result_type": "Produced Video",
            "release_date": "2016-05-23T11:00:00-04:00",
            "title": "The Faint Young Star Paradox: Solar Storms May Have Been Key to Life on Earth",
            "description": "Energy from our young sun – 4 billion years ago -- aided in creating molecules in Earth's atmosphere that allowed it to warm up enough to incubate life. Complete transcript available.Watch this video on the NASA Goddard YouTube channel. || faintyoung.jpg (1280x720) [105.6 KB] || faintyoung_searchweb.png (320x180) [81.4 KB] || faintyoung_thm.png (80x40) [15.3 KB] || WEBM_G2015-036_FaintYoungStarParadox_V2.webm (960x540) [39.6 MB] || G2015-036_FaintYoungStarParadox_V2.mov (1920x1080) [1.4 GB] || APPLE_TV_G2015-036_FaintYoungStarParadox_V2_appletv.m4v (1280x720) [54.0 MB] || YOUTUBE_HQ_G2015-036_FaintYoungStarParadox_V2_youtube_hq.mov (1920x1080) [318.5 MB] || NASA_TV_G2015-036_FaintYoungStarParadox_V2.mpeg (1280x720) [346.1 MB] || PRORES_B-ROLL_G2015-036_FaintYoungStarParadox_V2_prores.mov (1280x720) [719.8 MB] || APPLE_TV_G2015-036_FaintYoungStarParadox_V2_appletv_subtitles.m4v (1280x720) [54.0 MB] || G2015-036FaintYoungStarParadox_V2.en_US.srt [1.8 KB] || G2015-036FaintYoungStarParadox_V2.en_US.vtt [1.8 KB] || NASA_PODCAST_G2015-036_FaintYoungStarParadox_V2_ipod_sm.mp4 (320x240) [18.8 MB] || G2015-036_FaintYoungStarParadox_V2_lowres.mp4 (480x272) [14.8 MB] || ",
            "hits": 133
        },
        {
            "id": 10171,
            "url": "https://svs.gsfc.nasa.gov/10171/",
            "result_type": "Produced Video",
            "release_date": "2014-11-20T14:00:00-05:00",
            "title": "Swift: A Decade of Game-Changing Astrophysics",
            "description": "Scientists participating in NASA's Swift mission discuss the spacecraft, the science, and recall their personal experiences as members of the team.Watch this video on the NASA Goddard YouTube channel.For complete transcript, click here. || Swift_Interview_Still_print.jpg (1024x576) [160.8 KB] || Swift_Interview_Still.png (2560x1440) [4.1 MB] || Swift_Interview_Still_web.jpg (180x320) [21.2 KB] || Swift_Interview_Still_thm.png (80x40) [9.1 KB] || Swift_Interview_Still_web.png (320x180) [95.3 KB] || Swift_Interview_Still_searchweb.png (180x320) [95.3 KB] || Swift_10_Interviews_MPEG4_1280X720_2997.mp4 (1280x720) [149.1 MB] || G2014-067_Swift_10_Interviews_FINAL_appletv.webmhd.webm (960x540) [98.0 MB] || G2014-067_Swift_10_Interviews_FINAL_appletv.m4v (960x540) [257.7 MB] || G2014-067_Swift_10_Interviews_FINAL_appletv_subtitles.m4v (960x540) [257.5 MB] || G2014-067_Swift_10_Interviews_FINAL_1280x720.wmv (1280x720) [292.3 MB] || Swift_10_Interviews_H264_Good_1280x720_2997.mov (1280x720) [551.2 MB] || Swift_10_Interviews_H264_640x360_2997_iPhone.m4v (640x360) [94.6 MB] || G2014-067_Swift_10_Interviews.en_US.srt [11.7 KB] || G2014-067_Swift_10_Interviews.en_US.vtt [11.7 KB] || G2014-067_Swift_10_Interviews_FINAL_ipod_lg.m4v (640x360) [102.9 MB] || G2014-067_Swift_10_Interviews_FINAL_ipod_sm.mp4 (320x240) [51.9 MB] || Swift_10_Interviews_H264_Best_1280x720_5994.mov (1280x720) [3.9 GB] || Swift_10_Interviews_ProRes_1280x720_5994.mov (1280x720) [8.7 GB] || ",
            "hits": 55
        },
        {
            "id": 11126,
            "url": "https://svs.gsfc.nasa.gov/11126/",
            "result_type": "Produced Video",
            "release_date": "2012-11-20T00:00:00-05:00",
            "title": "Cosmic Concern",
            "description": "Flying exposes humans to a number of health risks. But perhaps none is more obscure than the hidden threat posed by cosmic radiation. Particles shed from the sun and by exploding stars in distant galaxies constantly bathe our planet in a nuclear soup of hazardous energy. During unpredictable spurts of extreme solar activity, a surge of particles can penetrate Earth's protective magnetic field and enter the atmosphere, causing radiation levels at cruising altitudes near the poles to skyrocket. In humans, large doses of radiation can damage DNA and harm bodily tissue. To help ensure the safety of airline passengers and crew, a NASA-funded project called NAIRAS (Nowcast of Atmospheric Ionizing Radiation System) has modeled the impact of space weather on radiation levels in the atmosphere with up-to-the-hour accuracy. Now, travelers can tally how much cosmic radiation they can expect to receive on a given flight. Watch the animation to see a virtual tour of air traffic around the world. || ",
            "hits": 79
        },
        {
            "id": 10935,
            "url": "https://svs.gsfc.nasa.gov/10935/",
            "result_type": "Produced Video",
            "release_date": "2012-03-21T00:00:00-04:00",
            "title": "Visions of Goddard",
            "description": "Excerpts of 14 short films about the NASA's Goddadrd Space Flight Center. || ",
            "hits": 32
        },
        {
            "id": 10822,
            "url": "https://svs.gsfc.nasa.gov/10822/",
            "result_type": "Produced Video",
            "release_date": "2011-09-15T00:00:00-04:00",
            "title": "Does DNA Have Extraterrestrial Origins?",
            "description": "If terms like adenine and guanine bring back unpleasant memories of Genetics 101 here's one reason to give the words a second thought: A team of scientists has discovered that these and other DNA building blocks can form in outer space and have been deposited on Earth's surface by meteorites. To reach this eye-opening conclusion, researchers ground up and analyzed a set of twelve meteorites collected from Antarctica and Australia. Within them, the scientists found a treasure trove of molecules that may have played a key role in allowing early forms of life to form. Adenine, which helps make up the rungs of DNA's spiraling, ladder-like structure, turned up in eleven of the meteorites. Guanine, another key building block of DNA, was present in eight. Two of the twelve meteorites also contained something extraordinary—exotic molecules that are so rare on Earth that they prove the DNA building blocks must have formed in outer space. The discovery lends support to the theory that a kit of pre-made parts from meteorites or a comet might have kick-started life on Earth. Learn more about the breakthrough in the video below. || ",
            "hits": 997
        },
        {
            "id": 10810,
            "url": "https://svs.gsfc.nasa.gov/10810/",
            "result_type": "Produced Video",
            "release_date": "2011-08-08T14:31:00-04:00",
            "title": "DNA Building Blocks Can Be Made in Space",
            "description": "NASA-funded researchers have evidence that some building blocks of DNA, the molecule that carries the genetic instructions for life, found in meteorites were likely created in space. The research gives support to the theory that a \"kit\" of ready-made parts created in space and delivered to Earth by meteorite and comet impacts assisted the origin of life. || ",
            "hits": 93
        },
        {
            "id": 3149,
            "url": "https://svs.gsfc.nasa.gov/3149/",
            "result_type": "Visualization",
            "release_date": "2005-05-04T12:00:00-04:00",
            "title": "Gamma Ray Bursts May Have Caused Ancient Extinctions",
            "description": "Scientists at NASA the University of Kansas say that a mass extinction on Earth hundreds of millions of years ago could have been triggered by a star explosion called a gamma-ray burst. The scientists do not have direct evidence that such a burst activated the ancient extinction. The strength of their work is their atmospheric modeling — essentially a 'what if' scenario.The scientists calculated that gamma-ray radiation from a relatively nearby star explosion, hitting the Earth for only ten seconds, could deplete up to half of the atmosphere's protective ozone layer. Recovery could take at least five years. With the ozone layer damaged, ultraviolet radiation from the Sun could kill much of the life on land and near the surface of oceans and lakes, and disrupt the food chain.These scientists calculated the potential effect of ultraviolet radiation on life. Deep-sea creatures living several feet below water would be protected. Surface-dwelling plankton and other life near the surface, however, would not survive. Plankton is the foundation of the marine food chain.This visualization shows the regions of the planet most susceptible to DNA damage (shown in red) if a large gamma ray burst were to occur close to Earth.[This text is from the NASA web story on the subject. See the Story URL below.] || ",
            "hits": 391
        },
        {
            "id": 3126,
            "url": "https://svs.gsfc.nasa.gov/3126/",
            "result_type": "Visualization",
            "release_date": "2005-03-08T12:00:00-05:00",
            "title": "Daily Erythemal Index (UV exposure) for 2000-2001 (WMS)",
            "description": "The Erythemal Index is a measure of ultraviolet (UV) radiation at ground level on the Earth. (The word 'erythema' means an abnormal redness of the skin, such as is caused by spending too much time in the sun—a sunburn is damage to your skin cells caused by UV radiation.) Atmospheric ozone shields life at the surface from most of the harmful components of solar radiation. Chemical processes in the atmosphere can affect the level of protection provided by the ozone in the upper atmosphere. This thinning of the atmospheric ozone in the stratosphere leads to elevated levels of UV at ground level and increases the risks of DNA damage in living organisms. || ",
            "hits": 15
        },
        {
            "id": 3114,
            "url": "https://svs.gsfc.nasa.gov/3114/",
            "result_type": "Visualization",
            "release_date": "2005-03-07T12:00:00-05:00",
            "title": "Daily Erythemal Index (UV exposure) Measurements for 2000-2001 (WMS)",
            "description": "The Erythemal Index is a measure of ultraviolet (UV) radiation at ground level on the Earth. (The word 'erythema' means an abnormal redness of the skin, such as is caused by spending too much time in the sun—a sunburn is damage to your skin cells caused by UV radiation.) Atmospheric ozone shields life at the surface from most of the harmful components of solar radiation. Chemical processes in the atmosphere can affect the level of protection provided by the ozone in the upper atmosphere. This thinning of the atmospheric ozone in the stratosphere leads to elevated levels of UV at ground level and increases the risks of DNA damage in living organisms. || ",
            "hits": 45
        },
        {
            "id": 3124,
            "url": "https://svs.gsfc.nasa.gov/3124/",
            "result_type": "Visualization",
            "release_date": "2005-03-07T12:00:00-05:00",
            "title": "Monthly Average Erythemal Index (UV exposure) for 2000-2001 (WMS)",
            "description": "The Erythemal Index is a measure of ultraviolet (UV) radiation at ground level on the Earth. (The word 'erythema' means an abnormal redness of the skin, such as is caused by spending too much time in the sun—a sunburn is damage to your skin cells caused by UV radiation.) Atmospheric ozone shields life at the surface from most of the harmful components of solar radiation. Chemical processes in the atmosphere can affect the level of protection provided by the ozone in the upper atmosphere. This thinning of the atmospheric ozone in the stratosphere leads to elevated levels of UV at ground level and increases the risks of DNA damage in living organisms. || ",
            "hits": 12
        },
        {
            "id": 2216,
            "url": "https://svs.gsfc.nasa.gov/2216/",
            "result_type": "Visualization",
            "release_date": "2001-08-08T12:00:00-04:00",
            "title": "Daily Erythemal Index over the United States for July 2001",
            "description": "The Erythemal Index is a measure of ultraviolet radiation (UV) at ground level on the Earth. UV exists to the left of the visible spectrum and is divided into three components (UV-A, UV-B and UV-C). UV-B (290-320 wavelengths) is the most dangerous form of UV radiation that can reach ground level. Atmospheric ozone shields life at the surface from most of the harmful components of solar radiation. Chemical processes in the atmosphere can effect the level of protection provided by the ozone in the upper atmosphere. This thinning of the atmospheric ozone in the stratosphere leads to elevated levels of UV-B at ground level and increases the risks of DNA damage in living organisms. || ",
            "hits": 13
        },
        {
            "id": 2217,
            "url": "https://svs.gsfc.nasa.gov/2217/",
            "result_type": "Visualization",
            "release_date": "2001-08-08T12:00:00-04:00",
            "title": "Daily Erythemal Index over the United States for July 2001 (With Dates)",
            "description": "The Erythemal Index is a measure of ultraviolet radiation (UV) at ground level on the Earth. UV exists to the left of the visible spectrum and is divided into three components (UV-A, UV-B and UV-C). UV-B (290-320 wavelengths) is the most dangerous form of UV radiation that can reach ground level. Atmospheric ozone shields life at the surface from most of the harmful components of solar radiation. Chemical processes in the atmosphere can effect the level of protection provided by the ozone in the upper atmosphere. This thinning of the atmospheric ozone in the stratosphere leads to elevated levels of UV-B at ground level and increases the risks of DNA damage in living organisms. || ",
            "hits": 16
        },
        {
            "id": 2218,
            "url": "https://svs.gsfc.nasa.gov/2218/",
            "result_type": "Visualization",
            "release_date": "2001-08-08T12:00:00-04:00",
            "title": "Erythemal Index for August 2000 through July 2001: Zoom to North America (With Dates)",
            "description": "The Erythemal Index is a measure of ultraviolet radiation (UV) at ground level on the Earth. UV exists to the left of the visible spectrum and is divided into three components (UV-A, UV-B and UV-C). UV-B (290-320 wavelengths) is the most dangerous form of UV radiation that can reach ground level. Atmospheric ozone shields life at the surface from most of the harmful components of solar radiation. Chemical processes in the atmosphere can effect the level of protection provided by the ozone in the upper atmosphere. This thinning of the atmospheric ozone in the stratosphere leads to elevated levels of UV-B at ground level and increases the risks of DNA damage in living organisms. || ",
            "hits": 3
        },
        {
            "id": 2219,
            "url": "https://svs.gsfc.nasa.gov/2219/",
            "result_type": "Visualization",
            "release_date": "2001-08-08T12:00:00-04:00",
            "title": "Erythemal Index for August 2000 through July 2001: Slow Zoom to North America (With Dates)",
            "description": "The Erythemal Index is a measure of ultraviolet radiation (UV) at ground level on the Earth. UV exists to the left of the visible spectrum and is divided into three components (UV-A, UV-B and UV-C). UV-B (290-320 wavelengths) is the most dangerous form of UV radiation that can reach ground level. Atmospheric ozone shields life at the surface from most of the harmful components of solar radiation. Chemical processes in the atmosphere can effect the level of protection provided by the ozone in the upper atmosphere. This thinning of the atmospheric ozone in the stratosphere leads to elevated levels of UV-B at ground level and increases the risks of DNA damage in living organisms. || ",
            "hits": 10
        },
        {
            "id": 2220,
            "url": "https://svs.gsfc.nasa.gov/2220/",
            "result_type": "Visualization",
            "release_date": "2001-08-08T12:00:00-04:00",
            "title": "Erythemal Index for August 2000 through July 2001: Rotating Globe (With Dates)",
            "description": "The Erythemal Index is a measure of ultraviolet radiation (UV) at ground level on the Earth. UV exists to the left of the visible spectrum and is divided into three components (UV-A, UV-B and UV-C). UV-B (290-320 wavelengths) is the most dangerous form of UV radiation that can reach ground level. Atmospheric ozone shields life at the surface from most of the harmful components of solar radiation. Chemical processes in the atmosphere can effect the level of protection provided by the ozone in the upper atmosphere. This thinning of the atmospheric ozone in the stratosphere leads to elevated levels of UV-B at ground level and increases the risks of DNA damage in living organisms. || ",
            "hits": 4
        },
        {
            "id": 2221,
            "url": "https://svs.gsfc.nasa.gov/2221/",
            "result_type": "Visualization",
            "release_date": "2001-08-08T12:00:00-04:00",
            "title": "Erythemal Index for August 2000 through July 2001: Slow Rotating Globe (With Dates)",
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}