{
    "count": 5,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 20187,
            "url": "https://svs.gsfc.nasa.gov/20187/",
            "result_type": "Animation",
            "release_date": "2011-02-09T12:00:00-05:00",
            "title": "STEREO Sun360 Animations",
            "description": "Animations created for STEREO Sun360 teaser and visuals release.For more on the STEREO Sun360 event go to #10713 and #10718. || ",
            "hits": 40
        },
        {
            "id": 10720,
            "url": "https://svs.gsfc.nasa.gov/10720/",
            "result_type": "Produced Video",
            "release_date": "2011-02-07T12:00:00-05:00",
            "title": "From Stonehenge to STEREO: A One Minute History of How We See the Sun",
            "description": "Humans have always wanted to learn about the Sun, but our understanding of our favorite star has changed through the centuries. In prepartion for Sun360, when the STEREO spacecrafts will provide the first uninterrupted view of the Sun, this video is a condensed history of how we have studied the Sun over time. || ",
            "hits": 38
        },
        {
            "id": 3809,
            "url": "https://svs.gsfc.nasa.gov/3809/",
            "result_type": "Visualization",
            "release_date": "2011-02-06T11:00:00-05:00",
            "title": "STEREO Achieves Full Solar Coverage: All the Sun. All the Time",
            "description": "When the two STEREO spacecraft move into positions on opposite sides of the Sun, we will have the capability to see a full 360 degrees around the solar sphere (there will probably still be some gaps in visibility near the poles of the Sun). Combined with solar observing satellites near the Earth, such as SDO and SOHO, this coverage will last for about eight years and the STEREO spacecraft move along in their orbits.This movie illustrates the orbital motions of the two STEREO spacecraft relative to the Earth (and noting the positions of the planets Mercury & Venus for reference). The camera occupies a position fixed relative to the Earth and Sun, so the distant starfield appears to spin around the observer. Because the frames are sampled at one per solar day, the Earth does not appear to rotate, but patient observation reveals that the tilt of the planet relative to the Sun, varies throughout the year, with the northern hemisphere tilted towards the Sun in northern hemisphere summer and away from the Sun in northern hemisphere winter. || ",
            "hits": 128
        },
        {
            "id": 3819,
            "url": "https://svs.gsfc.nasa.gov/3819/",
            "result_type": "Visualization",
            "release_date": "2011-02-06T11:00:00-05:00",
            "title": "STEREO Achieves Full Solar Coverage: View from the Farside",
            "description": "When the two STEREO spacecraft move into positions on opposite sides of the Sun, we will have the capability to see a full 360 degrees around the solar sphere (there will probably still be some gaps in visibility near the poles of the Sun). Combined with solar observing satellites near the Earth, such as SDO and SOHO, this coverage will last for about eight years and the STEREO spacecraft move along in their orbits.In this movie, we zoom in towards the Sun, fading from a visible light view to data from the 304 Ångstrom filters aboard SDO and both STEREO spacecraft. We swing the camera around to a view of the side of the Sun NOT visible from the Earth. With the STEREO and SDO data mapped to the sphere representing the Sun, we see the dark sliver of \"No Data\" which slowly shrinks as the STEREO spacecraft move into position 180 degrees apart on opposite sides of the Sun (and 90 degrees from Earth). STEREO data near the edge of the solar disk get stretched when projected onto a sphere and is responsible for the streaking on either side of the dark sliver. These data are sampled roughly six hours apart for each frame of the movie. Slight differenences in the six hour time step creates a slight 'jitter' of the dark sliver. || ",
            "hits": 34
        },
        {
            "id": 10718,
            "url": "https://svs.gsfc.nasa.gov/10718/",
            "result_type": "Produced Video",
            "release_date": "2011-02-06T10:00:00-05:00",
            "title": "STEREO Sun360",
            "description": "Launched in October 2006, STEREO traces the flow of energy and matter from the sun to Earth. It also provides unique and revolutionary views of the sun-Earth system. The mission observed the sun in 3-D for the first time in 2007. In 2009, the twin spacecraft revealed the 3-D structure of coronal mass ejections which are violent eruptions of matter from the sun that can disrupt communications, navigation, satellites and power grids on Earth.Seeing?the whole sun front and back simultaneously will enable significant advances in space weather forecasting for Earth and for planning for future robotic and manned spacecraft missions throughout the solar system.These views are the result of observations by NASA's two Solar TErrestrial Relations Observatory (STEREO) spacecraft. The duo are on diametrically opposite sides of the sun, 180 degrees apart. One is ahead of Earth in its orbit, the other trailing behind.For the STEREO Sun360 Teaser, go here.For the full visualization showing STEREO's path go here.For the visualization showing STEREO's increasing coverage of the sun (visual 3) go here.For animations from the STEREO Teaser and stages of coverage, go here.For animations showing STEREO's 3D coverage of a CME go here. || ",
            "hits": 105
        }
    ]
}