{
    "count": 10,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 3535,
            "url": "https://svs.gsfc.nasa.gov/3535/",
            "result_type": "Visualization",
            "release_date": "2008-08-15T00:00:00-04:00",
            "title": "Halloween Storms 2003: SOHO/EIT and TRACE at 195 Angstroms",
            "description": "This visualization compares the full-disk solar view of SOHO/EIT (green, on the left) with the small field of view of the TRACE ultraviolet telescope (gold, on the right). The yellow border of the TRACE imagery is projected on the appropriate location on the green EIT imagery.  Notice that TRACE can track features as they move across the solar disk. The instrument pointing is adjusted on a regular basis, which can produce a considerable amount of jittering in the image. This is a variation on the treatment of the same data as Solar Dynamics Observatory (SDO): Data Collection Comparison.Note that this movie does not play synchronous with the other animations that are part of the SDO Prelaunch package. || ",
            "hits": 21
        },
        {
            "id": 3435,
            "url": "https://svs.gsfc.nasa.gov/3435/",
            "result_type": "Visualization",
            "release_date": "2007-08-14T00:00:00-04:00",
            "title": "Solar Dynamics Observatory (SDO): Data Collection Comparison",
            "description": "Solar Dynamics Observatory (SDO) will dramatically increase our ability to collect data about the Sun. This visualization compares the temporal and spatial resolution of SOHO/EIT with TRACE. SDO will enable TRACE-like image and temporal resolution over the entire solar disk. This movie opens with a full-disk view of the Sun in ultraviolet light (195 angstroms) from SOHO/EIT using the traditional TRACE 'gold' color table. We zoom in on the active region on the western limb where the TRACE instrument is pointing and fade-in an inset of the higher-resolution TRACE data. To emphasize the comparison, the TRACE inset is moved aside (with a solid white border) revealing the matching EIT data view (enclosed in the faint white border). At this point, we step through the time series of data frames. In this movie, much of the TRACE imagery is collected at time intervals between 3 and 40 seconds. On the other hand, a new SOHO/EIT image is taken about every 12 minutes (720 seconds). The SDO Atmospheric Imaging Assembly (AIA) will take full-disk solar images at four times the SOHO/EIT spatial resolution, a whopping 4096x4096, and at least 70 times the temporal resolution, 10 seconds or better per image. This creates a data rate over 1000x higher than SOHO/EIT. It is roughly equivalent to TRACE spatial and temporal resolution, but over the entire solar disk. || ",
            "hits": 43
        },
        {
            "id": 3212,
            "url": "https://svs.gsfc.nasa.gov/3212/",
            "result_type": "Visualization",
            "release_date": "2005-08-16T12:00:00-04:00",
            "title": "Space Weather Forecasting: Active 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 bad match (as in this case) indicates that the region will generate flare events over the next few days. || ",
            "hits": 8
        },
        {
            "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": 33
        },
        {
            "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": 30
        },
        {
            "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": 14
        },
        {
            "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": 11
        },
        {
            "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": 14
        },
        {
            "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": 13
        },
        {
            "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": 15
        }
    ]
}