{
    "count": 13,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 2717,
            "url": "https://svs.gsfc.nasa.gov/2717/",
            "result_type": "Visualization",
            "release_date": "2003-04-11T12:00:00-04:00",
            "title": "Closeup of Solar 'Tadpoles' with time tags",
            "description": "Here is a close-up view of dark 'tentacles' or 'tadpoles' moving towards the solar surface in this solar flare of April 21, 2002 seen by TRACE.  One theory proposed in this press release is that they are due to voids created by magnetic reconnection in the flare.  This version of the visualization displays the instrument clock time tags. || ",
            "hits": 9
        },
        {
            "id": 2718,
            "url": "https://svs.gsfc.nasa.gov/2718/",
            "result_type": "Visualization",
            "release_date": "2003-04-11T12:00:00-04:00",
            "title": "Closeup of Solar 'Tadpoles' without time tags",
            "description": "Here is a close-up view of dark 'tentacles' or 'tadpoles' moving towards the solar surface in this solar flare of April 21, 2002 seen by TRACE.  One theory proposed in this press release is that they are due to voids created by magnetic reconnection in the flare.  This version of the visualization does not display the instrument clock time tags. || ",
            "hits": 26
        },
        {
            "id": 2509,
            "url": "https://svs.gsfc.nasa.gov/2509/",
            "result_type": "Visualization",
            "release_date": "2003-01-31T12:00:00-05:00",
            "title": "A Multi-Mission View of the AR9906 Solar Flare with Instrument Labels",
            "description": "Here's a view of the Sun, from the point of view of a fleet of Sun-observing spacecraft - SOHO, TRACE, and RHESSI. The time scales of the data samples in this visualization range from six hours to as short as 12 seconds and the display rate varies throughout the movie. The region and event of interest is the solar flare over solar active region AR9906 on April 21, 2002. In this visualization, the instrument names appear in a color roughly matching the color used for the data, and black corresponds to no (current) instrument coverage. || ",
            "hits": 13
        },
        {
            "id": 2511,
            "url": "https://svs.gsfc.nasa.gov/2511/",
            "result_type": "Visualization",
            "release_date": "2003-01-31T12:00:00-05:00",
            "title": "A Multi-Mission View of the AR9906 Solar Flare without Instrument Labels",
            "description": "Here's a view of the Sun, from the point of view of a fleet of Sun-observing spacecraft - SOHO, TRACE, and RHESSI. The time scales of the data samples in this visualization range from 6 hours to as short as 12 seconds and the display rate varies throughout the movie. The region and event of interest is the solar flare over solar active region AR9906 on April 21, 2002. In this visualization, black corresponds to no (current) instrument coverage (there used to be a LASCO C1 camera inside the ring of LASCO C2, but that instrument didn't recover after SOHO was temporarily 'lost' in 1998). || ",
            "hits": 16
        },
        {
            "id": 2553,
            "url": "https://svs.gsfc.nasa.gov/2553/",
            "result_type": "Visualization",
            "release_date": "2003-01-31T12:00:00-05:00",
            "title": "A Multi-Mission View of the AR9906 Solar Flare with Alternate Instrument Labels",
            "description": "Here's a view of the Sun, from the point of view of a fleet of Sun-observing spacecraft - SOHO, TRACE, and RHESSI. The time scales of the data samples in this visualization range from 6 hours to as short as 12 seconds and the display rate varies throughout the movie. The region and event of interest is the solar flare over solar active region AR9906 on April 21, 2002. In this visualization, black corresponds to no (current) instrument coverage (there used to be a LASCO C1 camera inside the ring of LASCO C2, but that instrument didn't recover after SOHO was temporarily 'lost' in 1998). || ",
            "hits": 25
        },
        {
            "id": 2464,
            "url": "https://svs.gsfc.nasa.gov/2464/",
            "result_type": "Visualization",
            "release_date": "2002-06-10T12:00:00-04:00",
            "title": "Another View of AR9906 from TRACE",
            "description": "Another view of the flare over AR9906 on April 21, 2002.  This version represents the full resolution of the TRACE data.  This visualization represents eight hours of observing time. || ",
            "hits": 11
        },
        {
            "id": 2458,
            "url": "https://svs.gsfc.nasa.gov/2458/",
            "result_type": "Visualization",
            "release_date": "2002-06-05T12:00:00-04:00",
            "title": "RHESSI Observes the Flare over AR9906 - Time Tagged",
            "description": "Close-up view of the solar active region AR9906 on April 21, 2002 with TRACE and RHESSI data. RHESSI observes x-rays from this flare. The red contours represent the 12-25 keV photon energy range and the blue contours represent 50-100 keV. || ",
            "hits": 14
        },
        {
            "id": 2459,
            "url": "https://svs.gsfc.nasa.gov/2459/",
            "result_type": "Visualization",
            "release_date": "2002-06-05T12:00:00-04:00",
            "title": "RHESSI Observes the Flare over AR9906 - No time tags",
            "description": "Close-up view of the solar active region AR9906 on April 21, 2002 with TRACE data and RHESSI. RHESSI observes x-rays from this flare. The red contours represent the 12-25 keV photon energy range and the blue contours represent 50-100 keV. || ",
            "hits": 7
        },
        {
            "id": 2460,
            "url": "https://svs.gsfc.nasa.gov/2460/",
            "result_type": "Visualization",
            "release_date": "2002-06-05T12:00:00-04:00",
            "title": "RHESSI Observes the Flare over AR9906 - zoom with times",
            "description": "Zoom in to solar active region AR9906 on April 21, 2002 with SOHO/EIT, TRACE and RHESSI data. RHESSI observes x-rays from this flare. The red contours represent the 12-25 keV photon energy range and the blue contours represent 50-100 keV. || Movie of RHESSI and TRACE data. || a002460.00100_print.png (720x480) [447.6 KB] || ar9906-zoom-dates_pre.jpg (320x240) [6.9 KB] || a002460.webmhd.webm (960x540) [6.9 MB] || ar9906-zoom-dates.mpg (640x480) [15.0 MB] || a002460.dv (720x480) [118.8 MB] || ",
            "hits": 14
        },
        {
            "id": 2461,
            "url": "https://svs.gsfc.nasa.gov/2461/",
            "result_type": "Visualization",
            "release_date": "2002-06-05T12:00:00-04:00",
            "title": "RHESSI Observes the Flare over AR9906 - zoom without times",
            "description": "Zoom in to solar active region AR9906 on April 21, 2002 with SOHO/EIT, TRACE and RHESSI data. RHESSI observes x-rays from this flare. The red contours represent the 12-25 keV photon energy range and the blue contours represent 50-100 keV. || ",
            "hits": 9
        },
        {
            "id": 2462,
            "url": "https://svs.gsfc.nasa.gov/2462/",
            "result_type": "Visualization",
            "release_date": "2002-06-05T12:00:00-04:00",
            "title": "RHESSI Observes the Flare over AR9906 - rotate view with times",
            "description": "Zoom in (with rotation) to solar active region AR9906 on April 21, 2002 with SOHO/EIT,TRACE and RHESSI data. RHESSI observes x-rays from this flare. The red contours represent the 12-25 keV photon energy range and the blue contours represent 50-100 keV. || ",
            "hits": 12
        },
        {
            "id": 2463,
            "url": "https://svs.gsfc.nasa.gov/2463/",
            "result_type": "Visualization",
            "release_date": "2002-06-05T12:00:00-04:00",
            "title": "RHESSI Observes the Flare over AR9906 - Rotate View Without Times",
            "description": "Zoom in (with rotation) to solar active region AR9906 on April 21, 2002 with SOHO/EIT, TRACE and RHESSI data. RHESSI observes x-rays from this flare. The red contours represent the 12-25 keV photon energy range and the blue contours represent 50-100 keV. || ",
            "hits": 7
        },
        {
            "id": 2446,
            "url": "https://svs.gsfc.nasa.gov/2446/",
            "result_type": "Visualization",
            "release_date": "2002-05-29T12:00:00-04:00",
            "title": "TRACE Observes the X-ray Flare Over AR9906",
            "description": "The TRACE spacecraft observes an X-ray flare over solar active region AR9906, April 21, 2002. || Movie of the flaring of active region AR9906 || a002446.00070_print.png (720x480) [447.5 KB] || xflare-ar9906_pre.jpg (320x240) [5.3 KB] || a002446.webmhd.webm (960x540) [2.1 MB] || a002446.dv (720x480) [44.6 MB] || xflare-ar9906.mpg (320x240) [1.7 MB] || ",
            "hits": 28
        }
    ]
}