{
    "count": 4,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 20132,
            "url": "https://svs.gsfc.nasa.gov/20132/",
            "result_type": "Animation",
            "release_date": "2008-01-23T00:00:00-05:00",
            "title": "Voyager 2 Proves Solar System is Squashed",
            "description": "As of August 30, 2007, NASA's Voyager 2 spacecraft has followed its twin Voyager 1 into the solar system's final frontier, a vast region at the edge of our solar system where the solar wind runs up against the thin gas between the stars. || ",
            "hits": 117
        },
        {
            "id": 2959,
            "url": "https://svs.gsfc.nasa.gov/2959/",
            "result_type": "Visualization",
            "release_date": "2004-07-08T12:00:00-04:00",
            "title": "Halloween Solar Storms from SOHO/EIT, 195 Angstroms",
            "description": "This view from SOHO/EIT in the 195 angstrom band, shows the multitude of solar flares released in the Fall of 2003 as a group of active regions rotated back into view. This movie is synchronized to play with animation IDs 2960 and 2961. For more information on how X-ray solar flares are classified (B, C, M, X), visit SpaceWeather.com. || ",
            "hits": 29
        },
        {
            "id": 2960,
            "url": "https://svs.gsfc.nasa.gov/2960/",
            "result_type": "Visualization",
            "release_date": "2004-07-08T12:00:00-04:00",
            "title": "Halloween Solar Storms from SOHO/EIT, 304 Angstroms",
            "description": "This view from SOHO/EIT in the 304 angstrom band, shows a group of active regions rotating back into view. This movie is synchronized to play with animation IDs 2959 and 2961. One obvious difference is that solar flares are not as visible at this wavelength than at the 195 angstrom band. The 304 angstrom filter was not used as frequently as the 195 angstrom filter, so this movie has more jumps in its time coverage. For more information on how X-ray solar flares are classified (B, C, M, X), visit SpaceWeather.com. || ",
            "hits": 11
        },
        {
            "id": 2961,
            "url": "https://svs.gsfc.nasa.gov/2961/",
            "result_type": "Visualization",
            "release_date": "2004-07-08T12:00:00-04:00",
            "title": "Halloween Solar Storms from SOHO/EIT and SOHO/LASCO",
            "description": "This movie is a combination of SOHO/EIT at 195 angstroms as well as the LASCO/C2 and C3 cameras. At this scale we can see the flashes from solar flares in SOHO/EIT (green) and the subsequent coronal mass ejections in SOHO/LASCO/C2 (red) and SOHO/LASCO/C3 (blue). This movie is synchronized to play with animation IDs 2960 and 2959. For more information on how X-ray solar flares are classified (B, C, M, X), visit SpaceWeather.com. || ",
            "hits": 24
        }
    ]
}