{
    "count": 1,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 4987,
            "url": "https://svs.gsfc.nasa.gov/4987/",
            "result_type": "Visualization",
            "release_date": "2022-04-28T11:00:00-04:00",
            "title": "Fast Magnetic Reconnection and the Hall Effect",
            "description": "Magnetic reconnection is one of the most complex processes known for converting energy from magnetic fields to particle motion.  It takes place in solar flares and regions of planetary (and stellar) magnetospheres.  Having been studied since the 1950s, many details of the process are still undergoing study.One of the key components in magnetic reconnection is the collision of two magnetic field regions with opposite-directed field lines, imbedded in a plasma.  The field and plasma combination forms an X-shaped configuration at their closest, and most intense point.These visualizations are plotted from a reconnection model generated by VPIC (Vector Particle-In-Cell) code.  Quantities are plotted in 'dimensionless' coordinates, that are normalized to the ion inertial length (di). || ",
            "hits": 259
        }
    ]
}