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Animation showing (1) the separation of the two STEREO spacecraft after launch, and (2) the deployment of the solar panels and the high gain antenna for communicating with Earth. Animation produced by SSV Project at JPL.
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Animations of two STEREO events: a lunar eclipse and an encounter with Comet McNaught.
The first animation shows the relative positions of Sun, the two STEREO spacecraft and Earth as the moon passed in front of the Sun from STEREO B's vantage point. The approximate fields of view of the EUVI telescope is shown in yellow. This sequence ends with the EUVI data capture during STEREO B's lunar eclipse; EUVI images in three wavelengths have been combined to create this sequence.
The second animation shows STEREO A's encounter with Comet McNaught showing the relative locations of the Sun, Earth, comet and spacecraft. The image of the comet captured by the heliospheric imager is also shown. Animation produced by SSV Project at JPL.
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Animation showing the fields of view of the 5 STEREO/SECCHI telescopes and the overlaps of the fields of view of the two spacecraft as the orbit evolves. The smaller fields of view (the EUVI telescope and the two coronagraphs) are centered on the Sun. The much large fields of view of the two heliospheric images are design to follow a coronal mass ejection from the Sun to the Earth. View in a frame fixed to Earth. Animation produced by SSV Project at JPL.
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Animation showing the fields of view of the 5 STEREO/SECCHI telescopes and the overlaps of the fields of view of the two spacecraft as the orbit evolves. The smaller fields of view (the EUVI telescope and the two coronagraphs) are centered on the Sun. The much large fields of view of the two heliospheric images are design to follow a coronal mass ejection from the Sun to the Earth. View in a an inertial frame. Animation produced by SSV Project at JPL.
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Full disk sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO A in the 171 angstroms wavelength.
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Full disk sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO A in the 195 angstroms wavelength.
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Full disk sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO A in the 284 angstroms wavelength. The aftermath of the eruption of a prominence which occurred on March 24, 2007 is evident in the sequence.
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Full disk sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO A in the 304 angstroms wavelength. Two promience eruptions are visible in this segment. The one on the lower right limb occurred on March 20 and the one barely visible on the disk occurred on March 24.
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Sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO A in the 171 angstroms wavelength, showing a portion of the equatorial region of the solar disk to provide a close up view of the active region.
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Sequence of images from February 24, 2007 taken by the EUVI telescope from STEREO A in the 195 angstroms wavelength, showing a close up of an active region eruption at the limb.
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Sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO A in the 284 angstroms wavelength, showing only the equatorial region of the solar disk. This provides a close up view of an large equatorial coronal hole and an active region.
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Sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO A in the 304 angstroms wavelength, showing a portion of the equatorial region of the solar disk.
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Full disk sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO B in the 171 angstroms wavelength.
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Full disk sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO B in the 195 angstroms wavelength.
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Full disk sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO B in the 284 angstroms wavelength. The aftermath of the eruption of a prominence which occurred on March 24, 2007 is evident in the sequence.
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Full disk sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO B in the 304 angstroms wavelength. Two promience eruptions are visible in this segment. The one on the lower right limb occurred on March 20 and the one barely visible on the disk occurred on March 24. .
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Sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO B in the 171 angstroms wavelength, showing a portion of the equatorial region of the solar disk to provide a close up view of the active region.
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Sequence of images from February 24, 2007 taken by the EUVI telescope from STEREO B in the 195 angstroms wavelength, showing a close up of an active region eruption at the limb.
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Sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO B in the 284 angstroms wavelength, showing only the equatorial region of the solar disk. This provides a close up view of an large equatorial coronal hole and an active region.
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Sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO B in the 304 angstroms wavelength, showing a portion of the equatorial region of the solar disk.
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STEREO Mission Overview Animation
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Comet McNaught Animation
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Stereo Spacecraft Flight Path Animation
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