{
    "count": 11,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 14874,
            "url": "https://svs.gsfc.nasa.gov/14874/",
            "result_type": "Produced Video",
            "release_date": "2025-07-28T10:00:00-04:00",
            "title": "STORIE Thermal Vacuum Test at NASA Goddard Space Flight Center",
            "description": "NASA’s STORIE mission, or Storm Time O+ Ring current Imaging Evolution, has completed its design, build, and testing campaign at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, ahead of its six-month mission onboard the International Space Station (ISS). From its unique vantage point on the ISS, STORIE will use its onboard neutral atom imager to provide an “inside out” view of Earth’s ring current – a region of the magnetosphere where energetic particles are trapped in near-Earth space. In addition to answering fundamental questions about the ring current’s intensity and composition, STORIE will also provide a more detailed understanding of how geomagnetic storms affect Earth.From NASA’s Goddard Space Flight Center, STORIE will be shipped to NASA’s Johnson Space Center in Houston, Texas, where it will be integrated onto a pallet to be installed outside the ISS’s Columbus Module. STORIE will head to the ISS aboard a SpaceX commercial resupply flight no earlier than spring 2026. || ",
            "hits": 162
        },
        {
            "id": 5567,
            "url": "https://svs.gsfc.nasa.gov/5567/",
            "result_type": "Visualization",
            "release_date": "2025-07-21T18:59:59-04:00",
            "title": "New Missions to L1",
            "description": "Three missions, Carruthers, IMAP and SWFO-L1 will be launched to the Sun-Earth Lagrange Point, L1.",
            "hits": 173
        },
        {
            "id": 14869,
            "url": "https://svs.gsfc.nasa.gov/14869/",
            "result_type": "Produced Video",
            "release_date": "2025-07-18T11:00:00-04:00",
            "title": "STORIE Fit Test at NASA Goddard Space Flight Center",
            "description": "NASA’s STORIE mission, or Storm Time O+ Ring current Imaging Evolution, has completed its design, build, and testing campaign at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, ahead of its mission onboard the International Space Station (ISS). From its unique vantage point on the ISS, STORIE will use neutral atom imaging to provide an “inside out” view of Earth’s ring current – a region of the magnetosphere where energetic particles are trapped in near-Earth space. In addition to answering fundamental questions about the ring current’s intensity and composition, STORIE will also provide a more detailed understanding of how geomagnetic storms affect Earth.From NASA’s Goddard Space Flight Center, STORIE will be shipped to NASA’s Johnson Space Center in Houston, Texas, where it will be integrated onto a pallet to be installed outside the ISS’s Columbus Module. STORIE will head to the ISS aboard a SpaceX commercial resupply flight no earlier than spring 2026. || ",
            "hits": 52
        },
        {
            "id": 4087,
            "url": "https://svs.gsfc.nasa.gov/4087/",
            "result_type": "Visualization",
            "release_date": "2013-07-10T13:00:00-04:00",
            "title": "IBEX Heliotail Observations",
            "description": "The IBEX (Interstellar Boundary EXplorer) continues to collect data on the flux of neutral atoms from the boundary of the solar wind with the interstellar medium.Starting with the IBEX satellite in orbit around the Earth, we zoom out to beyond the orbit of Neptune, illustrating the direction of the Sun relative to the local stars (red arrow) and relative to the local interstellar medium (violet arrow). These directions are different because the local interstellar medium (mostly gas and dust) move relative to the local stars.The boundaries of the termination shock (red ellipsoidal surface) and heliopause (green) created by the interaction of the solar wind with the interstellar medium is displayed. The camera rotates to a view 'nose on' with the heliopause, and a sphere is faded in representing the region where the neutral atoms detected by IBEX originate. The sphere around the Sun is 'unwrapped' to reproject the IBEX data into an approximately Aitoff projection. || ",
            "hits": 87
        },
        {
            "id": 3900,
            "url": "https://svs.gsfc.nasa.gov/3900/",
            "result_type": "Visualization",
            "release_date": "2012-01-31T13:00:00-05:00",
            "title": "The Local Interstellar Wind as Seen by IBEX",
            "description": "This visual presents a color-coded full-sky neutral atom map in a Hammer projection. This map is different from earlier IBEX maps in that it shows atoms only at energies where the interstellar wind is the brightest feature in the maps. In Earth's orbit, where IBEX makes its observations, the maximum flow (in red) is seen to arrive from Libra instead of Scorpio because the interstellar wind is forced to curve around the Sun by gravity. || ",
            "hits": 52
        },
        {
            "id": 3769,
            "url": "https://svs.gsfc.nasa.gov/3769/",
            "result_type": "Visualization",
            "release_date": "2010-09-30T12:00:00-04:00",
            "title": "IBEX Skymaps and the Bright Stars",
            "description": "In this image set, the brighter stars from the Tycho skymap have been reprojected into positions corresponding to the coordinate system used by the IBEX mission.The colors represent the number of neutral atoms (in the specified band of energies) detected by IBEX in each block of sky. Each block in the map is roughly a square about 6 degrees by 6 degrees (or the width of 12 full Moons, on a side). For the energy band displayed of 2.73 keV, violet corresponds to undetectable emission, while red corresponds to the detection of about 50 atoms per second per square centimeter in the angular segment of the sky. There is a 'hole' in the data (black) created when the IBEX scan cuts through the Earth's magnetotail.The images in this set have been co-registered for easy compositing. || ",
            "hits": 41
        },
        {
            "id": 3770,
            "url": "https://svs.gsfc.nasa.gov/3770/",
            "result_type": "Visualization",
            "release_date": "2010-09-30T12:00:00-04:00",
            "title": "IBEX Observes Changes in Heliopause Emission",
            "description": "The camera view moves from the heliosphere 'nose', the apparent direction of the heliopause relative to the interstellar wind, towards the 'knot'. The 'knot' represents a direction of high emission of neutral atoms which has changed significantly in the six months since the first IBEX map.We fade-in an artistic conception of the 'knot', which untangles during the six months as we fade to the second IBEX map. || ",
            "hits": 37
        },
        {
            "id": 3635,
            "url": "https://svs.gsfc.nasa.gov/3635/",
            "result_type": "Visualization",
            "release_date": "2009-10-15T12:00:00-04:00",
            "title": "IBEX First Skymap Release",
            "description": "The Interstellar Boundary Explorer (IBEX) mission science team has used data from NASA's IBEX spacecraft to construct the first-ever all-sky map of the interactions occurring at the edge of the solar system, where the sun's influence diminishes and interacts with the interstellar medium. The interstellar boundary region shields our solar system from most of the dangerous galactic cosmic radiation that would otherwise enter from interstellar space.This visualization illustrates the IBEX satellite in Earth orbit (the orbit reaching almost as far as the orbit of the Moon) and pulls out to beyond the heliopause boundary (the true 3-D nature of the boundary is reduced to a 2-D spherical surface). The sphere with the skymap opens to reproject the data into a near-Aitoff type map projection.The skymap shows the measured flux of energetic neutral atoms (ENAs). || ",
            "hits": 53
        },
        {
            "id": 2435,
            "url": "https://svs.gsfc.nasa.gov/2435/",
            "result_type": "Visualization",
            "release_date": "2002-05-09T12:00:00-04:00",
            "title": "IMAGE/LENA Observes Oxygen Atoms in the near-Earth Environment",
            "description": "Electrically charged oxygen atoms (green) are ejected into the magnetosphere due to heating in the ionosphere.  The red 'thermometer' displays the intensity of the solar wind (dynamic pressure) measured by the Geotail spacecraft.  The yellow 'thermometer' represents the source intensity or hydrogen counts as measured by IMAGE/LENA. || ",
            "hits": 14
        },
        {
            "id": 2444,
            "url": "https://svs.gsfc.nasa.gov/2444/",
            "result_type": "Visualization",
            "release_date": "2002-05-09T12:00:00-04:00",
            "title": "IMAGE/HENA Views Oxygen in the Magnetosphere (Rainbow Version)",
            "description": "IMAGE/HENA observes the oxygen ions, expelled from the Earth's atmosphere by the solar wind, return to the polar regions via the magnetic field. || Movie of IMAGE-HENA data using a rainbow color table for oxygen intensity. || a002444.00100_print.png (720x480) [373.3 KB] || HENArainbow_pre.jpg (320x288) [13.5 KB] || a002444.webmhd.webm (960x540) [8.1 MB] || a002444.dv (720x480) [112.3 MB] || HENArainbow.mpg (320x288) [942.9 KB] || ",
            "hits": 33
        },
        {
            "id": 2445,
            "url": "https://svs.gsfc.nasa.gov/2445/",
            "result_type": "Visualization",
            "release_date": "2002-05-09T12:00:00-04:00",
            "title": "IMAGE/HENA Views Oxygen in the Magnetosphere (Blue Version)",
            "description": "IMAGE/HENA observes the oxygen ions, expelled from the Earth's atmosphere by the solar wind, return to the polar regions via the magnetic field. || Movie of IMAGE-HENA data using a blue color table for oxygen intensity. || a002445.00010_print.png (720x480) [371.4 KB] || HENAblue_pre.jpg (320x320) [7.9 KB] || a002445.webmhd.webm (960x540) [8.1 MB] || a002445.dv (720x480) [153.6 MB] || HENAblue.mpg (320x320) [1.3 MB] || ",
            "hits": 23
        }
    ]
}