{
    "count": 3,
    "next": null,
    "previous": null,
    "results": [
        {
            "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": 55
        },
        {
            "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": 46
        },
        {
            "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": 64
        }
    ]
}