{
    "count": 11,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 12179,
            "url": "https://svs.gsfc.nasa.gov/12179/",
            "result_type": "Produced Video",
            "release_date": "2017-07-25T09:30:00-04:00",
            "title": "NASA Jets Chase The Total Solar Eclipse",
            "description": "For most viewers, the Aug. 21, 2017, total solar eclipse will last less than two and half minutes. But for one team of NASA-funded scientists, the eclipse will last over seven minutes. Their secret? Following the shadow of the Moon in two retrofitted WB-57F jet planes. Amir Caspi of the Southwest Research Institute in Boulder, Colorado, and his team will use two of NASA’s WB-57F research jets to chase the darkness across America on Aug. 21. Taking observations from twin telescopes mounted on the noses of the planes, Caspi will capture the clearest images of the Sun’s outer atmosphere — the corona — to date and the first-ever thermal images of Mercury, revealing how temperature varies across the planet’s surface. || ",
            "hits": 72
        },
        {
            "id": 12329,
            "url": "https://svs.gsfc.nasa.gov/12329/",
            "result_type": "Produced Video",
            "release_date": "2016-09-01T12:00:00-04:00",
            "title": "Snapshots from the Edge of the Sun",
            "description": "GIF of animated sun with corona and solar wind labels. || coronasolarwind.gif (1041x586) [2.2 MB] || ",
            "hits": 46
        },
        {
            "id": 3846,
            "url": "https://svs.gsfc.nasa.gov/3846/",
            "result_type": "Visualization",
            "release_date": "2011-12-16T00:00:00-05:00",
            "title": "From the Sun to the Earth: The View from STEREO-A with no CME Enhancement",
            "description": "This visualization shows the original dataset from STEREO-A used to extract the motion of the coronal mass ejection (CME) in ID 3890. The data are combined from the SECCHI instrument, which includes an ultraviolet image of the Sun (EUVI), two coronographs (COR-1 & COR-2), and the wide-angle Heliospheric Imagers (HI-1 & HI-2).On this scale, the CME is so faint as to be invisible. However, the Heliospheric Imagers support such a broad range of image intensity that it is possible to observe the CME propagating through the field of view by computing differences of images with the preceeding image. This process is shown in animation #3890.The Earth (left side) and Venus (middle) are so bright as to 'bloom' along the readout line of the CCD (Charge-coupled device) pixels, which creates the bright vertical lines that move slightly with time. The dark shape on the left of the field of view is created by an occulting tab that was installed to (occasionally) hide the bright Earth in the view.The little cross markers label three other planets in the view of STEREO. Uranus is almost invisible in the scale of this imagery, but is visible in full-resolution datasets. || ",
            "hits": 68
        },
        {
            "id": 3890,
            "url": "https://svs.gsfc.nasa.gov/3890/",
            "result_type": "Visualization",
            "release_date": "2011-12-06T00:00:00-05:00",
            "title": "From the Sun to the Earth: CME Enhancement",
            "description": "This visualization shows the dataset from STEREO-A processed to enhance the visibility of the coronal mass ejection (CME) in entry #3846. The data are combined from the SECCHI instrument, which includes an ultraviolet image of the Sun (EUVI), two coronographs (COR-1 & COR-2), and the wide-angle Heliospheric Imagers (HI-1 & HI-2).Because the enhancement process for the CME involves computing differences from a number of sequential HI-1 and HI-2 images, the Earth (left side) and Venus (middle) are masked and oversized icons are installed to mark their position. The dark shape on the left of the field of view is created by an occulting tab that was installed to (occasionally) hide the bright Earth in the view.The little cross markers label three other planets in the view of STEREO. Uranus is almost invisible in the scale of this imagery, but is visible in full-resolution datasets. || ",
            "hits": 42
        },
        {
            "id": 10821,
            "url": "https://svs.gsfc.nasa.gov/10821/",
            "result_type": "Produced Video",
            "release_date": "2011-09-13T00:00:00-04:00",
            "title": "Sun's Weather Encompasses Earth",
            "description": "The sun regularly spews forth bursts of particles and magnetic fields known as a coronal mass ejection, or, CME. A CME starts small in solar terms—just a few hundred times the size of the Earth—but it grows and changes as it travels toward the edges of the solar system. Scientists have been observing these events with satellites for decades, but tracking the details of an ejection's growth from original seed to complex structure near Earth has been more challenging. In fact, scientists recently used three NASA spacecraft—STEREO-A, WIND and ACE—to create the first visual record of a CME's path from the sun to the Earth. The orbiting instruments captured the CME's birth on Dec. 12, 2008 at the sun's surface, its exponential growth and its ultimate engulfing of the Earth about three days later. These ejections are common but large solar events can alter our magnetic atmosphere to such a degree that communications signals from GPS or telecom satellites are temporarily degraded beyond recognition. This visualization allowed scientists to watch how features early in the CME ultimately create the form seen closer to Earth, with a bright leading edge and trailing evacuated cavity. || ",
            "hits": 33
        },
        {
            "id": 3847,
            "url": "https://svs.gsfc.nasa.gov/3847/",
            "result_type": "Visualization",
            "release_date": "2011-08-18T14:00:00-04:00",
            "title": "From the Sun to the Earth: STEREO tracks a CME",
            "description": "For many years, the idea that coronal mass ejections (CME) launched from the Sun and could strike the Earth was inferred from an indirect chain of evidence collected from multiple satellites. Now the Heliospheric Imagers aboard the STEREO-A spacecraft has managed to view a CME propagate from the surface of the Sun to the Earth.This visualization shows the position of the STEREO spacecraft during the event, as well as the positions of the inner solar system planets, Venus and Mercury. A faint cone illustrates the field-of-view (FOV) of the HI-2 imager on STEREO-A. The position of the front of the CME is computed from STEREO data. || ",
            "hits": 104
        },
        {
            "id": 10809,
            "url": "https://svs.gsfc.nasa.gov/10809/",
            "result_type": "Produced Video",
            "release_date": "2011-08-18T13:00:00-04:00",
            "title": "NASA Spacecraft Track Solar Storms From Sun To Earth",
            "description": "NASA's STEREO spacecraft and new data processing techniques have succeeded in tracking space weather events from their origin in the Sun's ultrahot corona to impact with the Earth 93 million miles away, resolving a 40-year mystery about the structure of the structures that cause space weather: how the structures that impact the Earth relate to the corresponding structures in the solar corona.Despite many instruments that monitor the Sun and a fleet of near-earth probes, the connection between near-Earth disturbances and their counterparts on the Sun has been obscure, because CMEs and the solar wind evolve and change during the 93,000,000 mile journey from the Sun to the Earth.STEREO includes \"heliospheric imager\" cameras that monitor the sky at large angles from the Sun, but the starfield and galaxy are 1,000 times brighter than the faint rays of sunlight reflected by free-floating electron clouds inside CMEs and the solar wind; this has made direct imaging of these important structures difficult or impossible, and limited understanding of the connection between space storms and the coronal structures that cause them.Newly released imagery reveals absolute brightness of detailed features in a large geoeffective CME in late 2008, connecting the original magnetized structure in the Sun's corona to the intricate anatomy of an interplanetary storm as it impacted the Earth three days later. At the time the data were collected, in late 2008, STEREO-A was nearly 45 degrees ahead of the Earth in its orbit, affording a very clear view of the Earth-Sun line.For the press conference Visual 1, a visualization of the STEREO orbits and the 2008 CME, go here.For Visual 7, a CME and reconnection animation, go here.For Visual 8, footage of the October 2003 solar storms, go here. || ",
            "hits": 149
        },
        {
            "id": 2921,
            "url": "https://svs.gsfc.nasa.gov/2921/",
            "result_type": "Visualization",
            "release_date": "2005-03-08T12:00:00-05:00",
            "title": "Solar Tsunamis",
            "description": "Push-in to a region of the Sun to witness a 'solar tsunami' after a flare event.  The tsunami moves hot gas (bright) out of the region, revealing cooler regions (darker) below. || ",
            "hits": 30
        },
        {
            "id": 2922,
            "url": "https://svs.gsfc.nasa.gov/2922/",
            "result_type": "Visualization",
            "release_date": "2005-03-08T12:00:00-05:00",
            "title": "Solar Tsunamis - View with a Spin",
            "description": "Push-in to a region of the Sun to witness a 'solar tsunami' after a flare event.  The tsunami moves hot gas (bright) out of the region, revealing cooler regions (darker) below.  This view rotates on the push-in to keep the region of the flare event visible (to the left in the final frame). || ",
            "hits": 18
        },
        {
            "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": 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": 23
        }
    ]
}