{
    "count": 3,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 3431,
            "url": "https://svs.gsfc.nasa.gov/3431/",
            "result_type": "Visualization",
            "release_date": "2007-05-29T00:00:00-04:00",
            "title": "Coronal Mass Ejections (CME): Radio Quiet Variety",
            "description": "This is a simple comparison of SOHO/LASCO/C3 difference images (left side) combined with radio data from Wind/WAVES (right side).The LASCO difference images are produced from a time series of images by subtracting the previous image from the current image. Moving material therefore appears white on the leading edge and dark behind it. The WAVES spectrograph shows the variation of radio intensity (black is low, violet is high) in frequency (vertical axis) and time(horizontal axis). A vertical white bar marks the time of the LASCO image.This CME shows no radio-loud emission between 0.2-1.0 MHz. || ",
            "hits": 22
        },
        {
            "id": 3432,
            "url": "https://svs.gsfc.nasa.gov/3432/",
            "result_type": "Visualization",
            "release_date": "2007-05-29T00:00:00-04:00",
            "title": "Coronal Mass Ejections (CME): Radio Loud Variety",
            "description": "This is a simple comparison of SOHO/LASCO/C3 difference images (left side) combined with radio data from Wind/WAVES (right side).The LASCO difference images are produced from a time series of images by subtracting the previous image from the current image.  Moving material therefore appears white on the leading edge and dark behind it.  The WAVES spectrograph shows the variation of radio intensity (black is low, violet is high) in frequency (vertical axis) and time(horizontal axis).  A vertical white bar marks the time of the LASCO image.The radio-loud emission of the CME is the yellow-orange band between 0.2-1.0 MHz. || ",
            "hits": 33
        },
        {
            "id": 2936,
            "url": "https://svs.gsfc.nasa.gov/2936/",
            "result_type": "Visualization",
            "release_date": "2004-05-23T12:00:00-04:00",
            "title": "The fastest CME of Cycle 23 overtakes another fast CME",
            "description": "On November 4, 2003, the Sun produced its fastest coronal mass ejection (CME) for cycle 23 out of the active region 0486 located near the southwest limb of the Sun. The CME was expelled with a speed of approximately 2700 km/s. At the time of the launch of this CME, there was another ejection in progress from the same region. The previous ejection started about 7 hours earlier with a speed of about 1000 km/s. The fastest CME overtook the previous one within 2 hours and produced a spectacular radio radiation detected by the Wind, Ulysses and Cassini spacecraft. The movie shows the radio emission and the two interacting CMEs as observed by the SOHO spacecraft. || ",
            "hits": 55
        }
    ]
}