{
    "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": 10
        },
        {
            "id": 2766,
            "url": "https://svs.gsfc.nasa.gov/2766/",
            "result_type": "Visualization",
            "release_date": "2003-07-09T12:00:00-04:00",
            "title": "Hi-resolution Solar Views from VAULT: Quiet Region",
            "description": "This movie presents the VAULT imagery in the context of simultaneous multi-mission observations. We zoom-in to a subset of the image which focuses on a relatively calm solar region which still reveals a great deal of activity. || ",
            "hits": 15
        }
    ]
}