{
    "count": 2,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 3211,
            "url": "https://svs.gsfc.nasa.gov/3211/",
            "result_type": "Visualization",
            "release_date": "2005-08-16T12:00:00-04:00",
            "title": "Space Weather Forecasting: Quiet Times Ahead",
            "description": "SOHO/MDI magnetograms combined with the Potential-Field Source-Surface (PFSS) model can be used to generate a model of magnetic field lines in the lower part of the solar corona. When these models are compared to the loops visible in TRACE imagery, a good match (as in this case) indicates that the region will not generate flare events over the next few days. || ",
            "hits": 13
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            "id": 3212,
            "url": "https://svs.gsfc.nasa.gov/3212/",
            "result_type": "Visualization",
            "release_date": "2005-08-16T12:00:00-04:00",
            "title": "Space Weather Forecasting: Active Times Ahead",
            "description": "SOHO/MDI magnetograms combined with the Potential-Field Source-Surface (PFSS) model can be used to generate a model of magnetic field lines in the lower part of the solar corona. When these models are compared to the loops visible in TRACE imagery, a bad match (as in this case) indicates that the region will generate flare events over the next few days. || ",
            "hits": 18
        }
    ]
}