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    "results": [
        {
            "id": 5200,
            "url": "https://svs.gsfc.nasa.gov/5200/",
            "result_type": "Visualization",
            "release_date": "2023-12-11T12:00:00-05:00",
            "title": "Mars Disappearing Solar Wind: MAVEN Visualizations",
            "description": "This data visualization depicts a period of decreased solar wind at Mars that occurred on December 25, 2022, causing the planet’s magnetosphere to expand outward.   Ion velocity and density data collected by the MAVEN spacecraft is presented using a color-mapped satellite orbit tail and vectors along MAVEN’s orbit. || maven_solar_wind_comp.02715_print.jpg (1024x576) [84.4 KB] || maven_solar_wind_comp.02715_searchweb.png (320x180) [47.3 KB] || maven_solar_wind_comp.02715_thm.png (80x40) [4.3 KB] || maven_solar_wind_comp (3840x2160) [0 Item(s)] || maven_solar_wind_comp_2160p60.mp4 (3840x2160) [187.6 MB] || maven_solar_wind_comp_prores.mov (3840x2160) [10.1 GB] || ",
            "hits": 215
        },
        {
            "id": 14477,
            "url": "https://svs.gsfc.nasa.gov/14477/",
            "result_type": "Produced Video",
            "release_date": "2023-12-11T12:00:00-05:00",
            "title": "The Day the Solar Wind Disappeared from Mars",
            "description": "Learn about the “disappearance” of the solar wind at Mars that was witnessed by MAVEN – an event last seen nearly a quarter-century ago at Earth.Complete transcript available.Universal Production Music: “Space Museum” by Harry Gregson Williams [BMI], Atmosphere Music Ltd. [PRS]; “Currents and Crime Scenes” by Dylan Matthew Love and Harry Gregson Williams [BMI], Atmosphere Music Ltd. [PRS]Watch this video on the NASA Goddard YouTube channel. || MAVEN_Solar_Wind_Disappear_V4_print.jpg (1024x576) [142.7 KB] || MAVEN_Solar_Wind_Disappear_V4.jpg (1280x720) [459.3 KB] || MAVEN_Solar_Wind_Disappear_V4.png (1280x720) [800.2 KB] || MAVEN_Solar_Wind_Disappear_V4_searchweb.png (320x180) [69.9 KB] || MAVEN_Solar_Wind_Disappear_V4_thm.png (80x40) [6.5 KB] || 14477_MAVEN_Solar_Wind_Disappear_720.mp4 (1280x720) [43.4 MB] || 14477_MAVEN_Solar_Wind_Disappear_1080.mp4 (1920x1080) [243.1 MB] || MavenSolarWindCaptionsV2.en_US.srt [3.8 KB] || MavenSolarWindCaptionsV2.en_US.vtt [3.6 KB] || 14477_MAVEN_Solar_Wind_Disappear_4K.mp4 (3840x2160) [3.0 GB] || 14477_MAVEN_Solar_Wind_Disappear_ProRes.mov (3840x2160) [20.7 GB] || ",
            "hits": 117
        },
        {
            "id": 14204,
            "url": "https://svs.gsfc.nasa.gov/14204/",
            "result_type": "Produced Video",
            "release_date": "2022-08-31T09:00:00-04:00",
            "title": "Mars Patchy Proton Aurora",
            "description": "NASA’s MAVEN (Mars Atmosphere and Volatile Evolution) mission and the United Arab Emirates’ Emirates Mars Mission (EMM) have released joint observations of dynamic proton aurora events at Mars. Remote auroral observations by EMM paired with in-situ plasma observations made by MAVEN open new avenues for understanding the Martian atmosphere. This collaboration was made possible by recent data-sharing between the two missions and highlights the value of multi-point observations in space.Learn more about this discovery by MAVEN and EMM. || ",
            "hits": 87
        },
        {
            "id": 4954,
            "url": "https://svs.gsfc.nasa.gov/4954/",
            "result_type": "Visualization",
            "release_date": "2021-11-11T00:00:00-05:00",
            "title": "Mercury Makes Waves Cruising through the Solar Wind",
            "description": "Mercury orbits the Sun in a unique regime. The solar wind is still fresh from the Sun, and the Sun’s magnetic field strength (which drops with the square of distance) is rapidly waning. Furthermore, Mercury’s highly elliptical orbit means the planet passes through a wider range of distances from the Sun than any other planet. As a result, Mercury provides a unique opportunity to study how the Sun’s influence on a planet varies with distance.These animations provide a conceptual schematic of the results of one such investigation as described in “Occurrence rate of ultra-low frequency waves in the foreshock of Mercury increases with heliocentric distance.” Using data from NASA’s MESSENGER spacecraft, the authors has detected Ultra Low Frequency (ULF) waves rebounding from Mercury’s foreshock, the turbulent area where solar wind particles collide with Mercury’s magnetosphere. These waves are caused by solar wind protons – the steady stream of particles escaping the Sun –collide with and reflect off of this foreshock against the stream of the solar wind. The authors discovered that the ULF wave production rate varied throughout Mercury’s orbit. MESSENGER detected more ULF waves as Mercury moved farther from the Sun in its orbit, and fewer as it approached the Sun. The results support an existing theory that claimed that ULF waves are affected in part by the strength of the solar magnetic field, which is at its weakest when Mercury is farthest from the Sun. || ",
            "hits": 157
        },
        {
            "id": 13625,
            "url": "https://svs.gsfc.nasa.gov/13625/",
            "result_type": "Produced Video",
            "release_date": "2020-05-25T11:00:00-04:00",
            "title": "First Map of Mars Electric Currents",
            "description": "MAVEN data have enabled the first map of the electric current systems (blue and red arrows) that shape the induced magnetic field surrounding Mars.Credit: NASA/Goddard/MAVEN/CU Boulder/SVSUniversal Production Music: “A Lucid Dream” and “Shimmer Oscillations” by James Joshua OttoWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || MarsElectricCurrentsPreview6_print.jpg (1024x576) [305.8 KB] || MarsElectricCurrentsPreview6.jpg (1920x1080) [853.6 KB] || MarsElectricCurrentsPreview6_searchweb.png (320x180) [50.6 KB] || MarsElectricCurrentsPreview6_thm.png (80x40) [5.3 KB] || 13625_Mars_Electric_Currents_Twitter.mp4 (1280x720) [63.8 MB] || 13625_Mars_Electric_Currents_Facebook.mp4 (1920x1080) [359.1 MB] || 13625_Mars_Electric_Currents_YouTube.webm (3840x2160) [91.7 MB] || 13625_Mars_Electric_Currents_Captions.en_US.srt [7.2 KB] || 13625_Mars_Electric_Currents_Captions.en_US.vtt [6.8 KB] || 13625_Mars_Electric_Currents_YouTube.mp4 (3840x2160) [2.8 GB] || 13625_Mars_Electric_Currents_MASTER.mov (3840x2160) [14.2 GB] || 13625_Mars_Electric_Currents_Facebook.mp4.hwshow [134 bytes] || ",
            "hits": 119
        },
        {
            "id": 4825,
            "url": "https://svs.gsfc.nasa.gov/4825/",
            "result_type": "Visualization",
            "release_date": "2020-05-25T00:00:00-04:00",
            "title": "MAVEN – Mars and Solar Wind Simulation",
            "description": "This simulation depicts the solar wind interacting with the Mars upper atmosphere, with MAVEN's orbit embedded. || maven_cme44.03600_print.jpg (1024x512) [253.9 KB] || maven_cme44.03600_searchweb.png (320x180) [92.7 KB] || maven_cme44.03600_thm.png (80x40) [5.2 KB] || 1920x1080_16x9_30p (2048x1024) [0 Item(s)] || maven_cme44_1024p30.webm (2048x1024) [5.9 MB] || maven_cme44_1024p30.mp4 (2048x1024) [195.1 MB] || maven_cme44_1024p30.mp4.hwshow [58 bytes] || ",
            "hits": 46
        },
        {
            "id": 4639,
            "url": "https://svs.gsfc.nasa.gov/4639/",
            "result_type": "Visualization",
            "release_date": "2018-05-09T13:00:00-04:00",
            "title": "MMS Sees a New Type of Reconnection",
            "description": "The Magnetospheric Multiscale (MMS) mission consists of four identical satellites that traverse various regions of Earth's magnetosphere measuring the particles and electric and magnetic field which influence them.In the turbulent plasma between Earth's magnetopause and bow shock, a region called the magnetosheath, the MMS satellite constellation has measured multiple jets of energetic electrons between magnetic bubbles.  This appears to be a new 'flavor' of magnetic reconnection based on electrons and occuring on smaller time and spatial scales than the standard model of magnetic reconnection with ions.In these data visualizations, the arrows represent the data collected by the spacecraft.  To better comprehend changes as the spacecraft moves along, the data are allowed to 'echo' along the spacecraft trail.  The length of the vectors represent the relative magnitude of the vector.  However, the electron and proton vectors are scaled so equal velocities correspond to vectors of equal magnitude.Magenta represents the direction and magnitude of the magnetic field at the spacecraft position.Green represents the direction and magnitude of the net electric current created by the motion of the electrons and ions measured at the spacecraft position.The four MMS spacecraft are represented by colored spheres, corresponding to the plotted data lines in the lower graphicMMS1MMS2MMS3MMS4The clocks on MMS are synchronized for the TAI (International Atomic Time) system provided through the Global Positioning System (GPS) satellites.  It provides a high-precision time reference for comparing MMS measurements to other datasets. || ",
            "hits": 609
        },
        {
            "id": 4393,
            "url": "https://svs.gsfc.nasa.gov/4393/",
            "result_type": "Visualization",
            "release_date": "2015-11-05T14:00:00-05:00",
            "title": "Solar Wind and Mars Bow Shock",
            "description": "Simulation of the solar wind at Mars compared with MAVEN observations, showing the predicted bow shock. Available for download in up to 4k resolution. || final_shock01.2500_print.jpg (1024x576) [205.3 KB] || final_shock01.2500_searchweb.png (320x180) [100.4 KB] || final_shock01.2500_thm.png (80x40) [6.6 KB] || final_shock01_1920x1080_60fps.mp4 (1920x1080) [66.6 MB] || APPLE_TV_4393_Mars_Solar_Wind_Bow_Shock_1920x1080_appletv.m4v (1280x720) [19.0 MB] || WEBM_4393_Mars_Solar_Wind_Bow_Shock_1920x1080.webm (960x540) [15.1 MB] || 1920x1080_16x9_60p (1920x1080) [0 Item(s)] || NASA_TV_4393_Mars_Solar_Wind_Bow_Shock_1920x1080.mpeg (1280x720) [128.4 MB] || PRORES_B-ROLL_4393_Mars_Solar_Wind_Bow_Shock_1920x1080_prores.mov (1280x720) [537.1 MB] || 3840x2160_16x9_60p (3840x2160) [0 Item(s)] || 4393_Mars_Solar_Wind_Bow_Shock_1920x1080.mov (1920x1080) [1.0 GB] || final_shock01_4k_60fps.mp4 (3840x2160) [214.3 MB] || ",
            "hits": 75
        },
        {
            "id": 10722,
            "url": "https://svs.gsfc.nasa.gov/10722/",
            "result_type": "Produced Video",
            "release_date": "2011-02-07T12:00:00-05:00",
            "title": "IBEX Spacecraft Finds Discoveries Close to Home",
            "description": "IBEX found that Energetic Neutral Atoms, or ENAs, are coming from a region just outside Earth's magnetopause where nearly stationary protons from the solar wind interact with the tenuous cloud of hydrogen atoms in Earth's exosphere. || ",
            "hits": 50
        },
        {
            "id": 3478,
            "url": "https://svs.gsfc.nasa.gov/3478/",
            "result_type": "Visualization",
            "release_date": "2007-12-11T00:00:00-05:00",
            "title": "THEMIS Explores the Earth's Bow Shock",
            "description": "The solar wind's first contact with the Earth's magnetic field creates a region known as the bow shock, much like the bow wave of a boat moving through the water. This region can also create additional turbulence which generates bursts of explosion-like currents. In this visualization, the orbits of the THEMIS fleet are combined with a 2-D slice from a hybrid magnetosphere simulation which illustrates these turbulent regions in the bow shock. This hybrid magnetosphere simulation treats the slow-moving ions by particle-in-cell computational methods and the faster electrons as a massless fluid. These simulations more accurately represent the magnetospheric physics, enabling a view of turbulent non-linear processes not visible in the simpler magnetohydrodynamic models. In this simulation, the color table is somewhat unusual. In order of increasing density, the colors run from white through violet, blue, green to black. || ",
            "hits": 85
        },
        {
            "id": 3391,
            "url": "https://svs.gsfc.nasa.gov/3391/",
            "result_type": "Visualization",
            "release_date": "2006-12-14T00:00:00-05:00",
            "title": "THEMIS Orbits: Dayside Science Configuration",
            "description": "In the early part of the mission, the five THEMIS satellites will follow the same orbit single-file. The apogee of the orbit will take the spacecraft just beyond the bow shock of the Earth's magnetosphere. This will enable the satellites to collect data in this region over a short range of time so that the time history can be studied. The dates in this visualization are based on an ephemeris assuming a launch on January 20, 2007. The satellite colors are: red=P1, green=P2, cyan=P3, blue=P4, magenta=P5. || ",
            "hits": 34
        }
    ]
}