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    "results": [
        {
            "id": 20036,
            "url": "https://svs.gsfc.nasa.gov/20036/",
            "result_type": "Animation",
            "release_date": "2004-12-03T12:00:00-05:00",
            "title": "IMAGE and Cluster View Magnetic Reconnection",
            "description": "The IMAGE and Cluster spacecraft were ideally positioned in their orbits to view the reconnection event which led to the proton aurora formation. || ",
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            "id": 20037,
            "url": "https://svs.gsfc.nasa.gov/20037/",
            "result_type": "Animation",
            "release_date": "2004-12-03T12:00:00-05:00",
            "title": "Proton Aurora Forms from Reconnection Event",
            "description": "Solar wind protons can breach the Earth's magnetic field through a magnetic reconnection event.  Sometimes when this happens we see a (proton) aurora when the solar protons make it to the Earth's atmosphere. || ",
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