{
    "count": 7,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 3115,
            "url": "https://svs.gsfc.nasa.gov/3115/",
            "result_type": "Visualization",
            "release_date": "2005-03-08T12:00:00-05:00",
            "title": "Gaps in the Earth's Radiation Belts",
            "description": "The Earth's radiation belts (violet & white) change considerably due to a number of influences, ranging from a changing solar wind to the lightning on the Earth. Here we see a range of variation in the electron flux in early December 2003. White indicates higher electron flux than violet. The gray curves represent the lines of the Earth's magnetic field. These radiation belts are constructed on a per-orbit basis with data from SAMPEX. || ",
            "hits": 91
        },
        {
            "id": 3048,
            "url": "https://svs.gsfc.nasa.gov/3048/",
            "result_type": "Visualization",
            "release_date": "2004-12-15T12:00:00-05:00",
            "title": "Earth's Radiation Belts Tremble Under Impact of Solar Storm",
            "description": "Under the wave of energetic particles from the Halloween 2003 solar storm events, the Earth's radiation belts underwent significant changes in structure.  This visualization is constructed using daily-averaged particle flux data from the SAMPEX satellite installed in a simple dipole model for the Earth's magnetic field.  The toroidal structure of the belts corresponds to regions with electron fluxes in excess of 100 electrons/s/cm^2/steradian with energies of 2-6 MeV.  The color-scale on the cross section is violet for low flux and white for high flux.  The translucent gray arcs represent the fields lines of the Earth's dipole field.  The 3-dimensional structure was built from the SAMPEX measurement by propagating the particle flux values along field lines of a simple magnetic dipole.NOTE:  This visualization shows the Earth's magnetic dipole field lines rotating rigidly with the Earth.  Technically, this is inaccurate.  Ions and electrons in the lower atmosphere can create currents which can make these lines 'drag' with Earth's rotation, but this will occur mostly near the Earth and not higher up.  More details on this process can be found in the FAQ at the The Exploration of the Earth's Magnetosphere web site, Does the Earth's magnetic field rotate?. || ",
            "hits": 42
        },
        {
            "id": 3049,
            "url": "https://svs.gsfc.nasa.gov/3049/",
            "result_type": "Visualization",
            "release_date": "2004-12-15T12:00:00-05:00",
            "title": "Radiation Belts and Plasmapause Fluctuate Under Solar Storm",
            "description": "In this visualization, we see the interaction of the radiation belts (violet/white), the plasmapause (green surface) and magnetopause (gray surface).NOTE: This visualization shows the Earth's magnetic dipole field lines rotating rigidly with the Earth. Technically, this is inaccurate. Ions and electrons in the lower atmosphere can create currents which can make these lines 'drag' with Earth's rotation, but this will occur mostly near the Earth and not higher up. More details on this process can be found in the FAQ at the The Exploration of the Earth's Magnetosphere web site, Does the Earth's magnetic field rotate?. || ",
            "hits": 53
        },
        {
            "id": 3052,
            "url": "https://svs.gsfc.nasa.gov/3052/",
            "result_type": "Visualization",
            "release_date": "2004-12-15T12:00:00-05:00",
            "title": "Earth's Radiation Belts with Safe Zone Orbit",
            "description": "Spacecraft orbiting in the 'Safe Zone', between two and three Earth radii, can be subjected to high levels of harmful radiation as the radiation belts fluctuate in response to space weather events.NOTE:  This visualization shows the Earth's magnetic dipole field lines rotating rigidly with the Earth.  Technically, this is inaccurate.  Ions and electrons in the lower atmosphere can create currents which can make these lines 'drag' with Earth's rotation, but this will occur mostly near the Earth and not higher up.  More details on this process can be found in the FAQ at the The Exploration of the Earth's Magnetosphere web site, Does the Earth's magnetic field rotate?. || ",
            "hits": 79
        },
        {
            "id": 90,
            "url": "https://svs.gsfc.nasa.gov/90/",
            "result_type": "Visualization",
            "release_date": "1995-11-07T12:00:00-05:00",
            "title": "SAMPEX - Yohkoh: Solar Modification of Relativistic Electrons in the Earth's Radiation Belts",
            "description": "The Solar Anomalous and Magnetospheric Particle Explorer, SAMPEX, measures fluxes of energetic particles from the sun, the Earth's magnetosphere, and cosmic ray sources over a broad range of energies. The four instruments aboard SAMPEX are the Low-Energy Ion Analyzer (LEICA), The Heavy Ion Large Telescope (HILT), The Mass Spectrometer Telescope (MAST), and the Proton-Electron Telescope (PET). The Soft X-ray Telescope on the Yohkoh satellite takes daily full-disk soft X-ray images of the Sun. Comparing data sets from the two satellites allows correlation of electron fluxes in the Earth's radiation belts with solar output. || ",
            "hits": 44
        },
        {
            "id": 1386,
            "url": "https://svs.gsfc.nasa.gov/1386/",
            "result_type": "Visualization",
            "release_date": "1995-01-01T12:00:00-05:00",
            "title": "SAMPEX - A Synoptic View of Earth's Electron Radiation Belts: North Pole Energetic Fluxes from PET",
            "description": "The Solar Anomalous and Magnetospheric Particle Explorer, SAMPEX, measures fluxes of energetic particles from the sun, the Earth's magnetosphere, and cosmic ray sources over a broad range of energies.  The four instruments aboard SAMPEX are the Low-Energy Ion Analyzer (LEICA), The Heavy Ion Large Telescope (HILT), The Mass Spectrometer Telescope (MAST), and the Proton-Electron Telescope (PET). || ",
            "hits": 10
        },
        {
            "id": 1387,
            "url": "https://svs.gsfc.nasa.gov/1387/",
            "result_type": "Visualization",
            "release_date": "1995-01-01T12:00:00-05:00",
            "title": "SAMPEX - A Synoptic View of Earth's Electron Radiation Belts: South Pole Energetic Fluxes from PET",
            "description": "The Solar Anomalous and Magnetospheric Particle Explorer, SAMPEX, measures fluxes of energetic particles from the sun, the Earth's magnetosphere, and cosmic ray sources over a broad range of energies.  The four instruments aboard SAMPEX are the Low-Energy Ion Analyzer (LEICA), The Heavy Ion Large Telescope (HILT), The Mass Spectrometer Telescope (MAST), and the Proton-Electron Telescope (PET). || ",
            "hits": 12
        }
    ]
}