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<title>STEREO COR1 | Movie Gallery</title>
<link>http://cor1.gsfc.nasa.gov/movies/</link>
<description>STEREO COR1 | Movie Gallery</description>

<image>
<url>http://cor1.gsfc.nasa.gov/images/site_images/COR1logo.jpg</url>
<title>STEREO COR1</title>
<link>http://cor1.gsfc.nasa.gov/movies/</link>
</image>

  
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<item>
<title>Halo CME observed by COR1-B</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/cor1_halo_20091115.mpg</link>
<description><![CDATA[Most coronal mass ejections (CMEs) observed by the COR1 telescopes are seen to 
be traveling outside on one side or the other of the Sun.  However, if a CME 
happens to be traveling directly toward (or in this case away from) the telescope, it will appear on all 
sides of the Sun at once.  Such events are called halo CMEs, because they form a 
halo around the Sun.  Just such an event was seen by the COR1 telescope on the 
STEREO Behind spacecraft on 15 November 2009.]]></description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/cor1_halo_20091115_thumb.jpg</guid>
</item>

<item>
<title>Jupiter and Galilean moons observed</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/JupiterCOR1zm_best.mov</link>
<description><![CDATA[No one has been able to observe Jupiter and its moons for some time as it is too close to the Sun, 
but that did not stop the STEREO (Behind) COR1 coronagraph from capturing it and its four major moons over a 30-hour period (March 15-16, 2009).  
If you look carefully, you can identify three of its moons close to Jupiter, and even discern how their positions change as the movie progresses.  
Those with keen eyes can see the fourth moon, Callisto, as a fainter object well to the right of the others.  These four moons are known as 
the Galilean moons, because they were first discovered by Galileo Galilei in 1610.  Jupiter itself is largely saturated in the movie,  
to bring out the moons and the faint solar corona.  The solid dark green area on the right is the coronagraph?s occulting disk that blocks 
out the Sun and some of its bright atmosphere to that our instrument can see fainter structure just beyond the Sun.  The thin, white line 
inside of that indicates the actual size of the Sun.   By coincidence, a coronal mass ejection is seen blasting a white cloud of charged 
particles out into space during much of the clip.  We have not seen many solar storms of late as the Sun is near its low point in its 
solar activity cycle.]]></description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/JupiterCOR1zm_thumb.jpg</guid>
</item>

<item>
<title>Bright sungrazing comet observed by COR1 on May 23, 2008</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/comet20080523.mpg</link>
<description><![CDATA[An extremely bright sungrazing comet was seen by COR1 on May 23, 2008 on both Ahead and Behind. Because of the separation of the two spacecraft, the comet appears quite differently in each. This is the brightest comet yet seen by COR1. The comet does not survive its approach to the Sun, and is not seen to come back out.]]></description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/comet20080523_thumb.jpg</guid>
</item>

<item>
<title>Sungrazing comet observed by COR1 on June 16, 2008</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/comet20080616_rd.mpg</link>
<description><![CDATA[A sungrazing comet is seen by COR1 as it approaches the Sun and is destroyed. This movie is shown in the "running difference" format, where each image has an earlier image subtracted from it, to make the faint comet stand out from the much brighter solar corona. This makes it appear as if the comet is followed by its shadow, which is actually the negative image of the comet 20 minutes earlier. Because the two STEREO spacecraft are looking at the Sun from different directions, the appearance of the comet is quite different in each. The comet appears first coming up from below in the Behind view. Later, it is seen in Ahead approaching from the right. Combining these two viewpoints give us a three-dimensional view of the comet tail.]]></description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/comet20080616_rd_thumb.jpg</guid>
</item>

<item>
<title>Prominence Eruption on April 9, 2008</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/COR1cme.mov</link>
<description><![CDATA[It is a combination of COR1A and SECCHI EUVI 304 Angstrom images showing a spectacular prominence eruption on 2008-04-09.  This event was also seen by the Hinode soft X-ray imager, and joint analysis of this interesting event is underway.]]></description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/COR1cme_thumb.jpg</guid>
</item>

<item>
<title>Jupiter System Spotted by COR 1 - November 29, 2007</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/jupiter.mpg</link>
<description><![CDATA[Jupiter entered the field of view of the COR1 telescope on the STEREO Ahead spacecraft on November 29th, 2007.  Along with the planet itself, one can clearly make out some of the major Jovian moons.  The first moons to enter the COR1 field are Ganymede and Callisto, which start out very close to each other.  These are followed closely by Jupiter itself, which is heavily saturated in the COR1 images.  As time progresses, and the moons revolve about Jupiter, Ganymede and Callisto separate from each other, and become visible as separate moons.  One also sees Io and Europa come out from in front of Jupiter, so that there's a period when all four major moons are visible.  Io is the hardest of the four moons to see, because it spends much of its time very close to Europa.  The feature on the right side of the movie is the occulter which is used to block out the bright sunlight.]]></description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/jupiter_thumb.jpg</guid>
</item>

<item>
<title>CME - August 1, 2007</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/20070802-euvicor1a_grids.avi</link>
<description><![CDATA[A CME appears in the NE on August 1, 2007, as seen by EUVI and COR1. The image processing software that produced this movie and some others in the Gallery is &#34;Festival&#34;  which is available at: <a href="http://www.ias.u-psud.fr/stereo/festival">http://www.ias.u-psud.fr/stereo/festival</a>]]></description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/20070802-cor1a_grids_thumb.jpg</guid>
</item>

<item>
<title>Lunar Transit</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/euvicor1_moon.avi</link>
<description>Combined data from EUVI and COR1 showing the lunar transit on 02/24/2007</description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/euvicor1_moon_thumb.jpg</guid>
</item>

<item>
<title>CME on February 9, 2007</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/20070209_euvicor1.avi</link>
<description>CME on February 9, 2007</description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/20070209_euvicor1_thumb.jpg</guid>
</item>

<item>
<title>CME on February 9, 2007</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/20070209_euvicor1_zoom.avi</link>
<description>CME on February 9, 2007</description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/20070209_euvicor1_zoom_thumb.jpg</guid>
</item>

<item>
<title>CME on February 9, 2007</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/20070209_euvicor1cor2.avi</link>
<description>CME on February 9, 2007</description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/20070209_euvicor1cor2_thumb.jpg</guid>
</item>

<item>
<title>A CME seen by STEREO A &#38; B and SOHO</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/20070802-abs-euvicor1cor2.avi</link>
<description>This movie show a CME lifting off the East limb as seen simultaneously by STEREOB (left), SOHO (center) and STEREOA (right).</description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/20070802-abs-euvicor1cor2_thumb.jpg</guid>
</item>

<item>
<title>Sungrazer Comet in 3D</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/sungrazer_stereopair.mpg</link>
<description>The measured 3D position of the comet tail is overplotted in anaglyph format. Use red-blue glasses to see the effect.</description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/sungrazer_stereopair_thumb.jpg</guid>
</item>

<item>
<title>Sungrazer Comet Approaching the Sun</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/sungrazer_singleview.mpg</link>
<description>This movie shows a sungrazer comet approaching the Sun as seen by the COR1 Ahead telescope on June 8, 2007.  The comet was seen by both the STEREO Ahead and Behind spacecraft, allowing the position and shape of the comet tail to be measured in three dimensions.</description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/sungrazer_singleview_thumb.jpg</guid>
</item>

<item>
<title>An unusual event observed by STEREO</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/050107.mpg</link>
<description>Here is an unusual event observed by STEREO on May 1, 2007, off the northeast limb of the Sun. There was the &#34;tornadic&#34; motion of the prominence seen in Helium II (304 Angstrom); then what can only be described as a &#34;blob&#34; moved extremely slowly (&#60;10 km/s) through the low corona, with non-radial motions through the MLSO MK4 and COR1. The &#34;blob&#34; seemed to &#34;evaporate&#34; at the trailing portion of what appeared to be an elongated fluxrope CME without any clear front. More study necessary to explain this one!</description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/050107_thumb.jpg</guid>
</item>

<item>
<title>Wavelet-enhanced images</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/May2007_COR1_AB.mov</link>
<description>Wavelet-enhanced images from May 2007, taken every six hours from COR1-A
and COR1-B.</description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/May2007_COR1_AB_thumb.jpg</guid>
</item>

<item>
<title>June 2007 from COR1-A</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/June2007_COR1A.mov</link>
<description>Assembled and image-processed using a wavelet enhancement technique by Dr. Guillermo Stenborg. The frames are four images per day for the month of June 2007 from COR1-A.</description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/June2007_COR1A_thumb.jpg</guid>
</item>

<item>
<title>Halo CME</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/COR1_CME070730_512.mpg</link>
<description>The COR1 coronagraph instrument on STEREO caught a nice "halo" CME (coronal mass ejection) as it expanded out into space on July 30, 2007.  It is named "halo" CME when the leading edge of the particle cloud appears as an expanding arc around the Sun, something we can see, though faintly, in this video. The ejected material is either heading more or less directly towards or away from the viewer. In this case, the event was judged to have occurred on the backside of the Sun as we saw no evidence of an event on the front side. The video clip cover about 8 hours of activity.</description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/20070730_stillB.jpg</guid>
</item>

<item>
<title>An apparent "halo" CME</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/2007-May-20.mpg</link>
<description>An apparent "halo" CME detected in Total Brightness on 20-May-2007</description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/2007-May-20_thumb.jpg</guid>
</item>

<item>
<title>TotalB Movie</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/2007-May-22.mpg</link>
<description>TotalB movie of a multipart CME(s) on the West limb on 22-May-2007</description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/2007-May-22_thumb.jpg</guid>
</item>

<item>
<title>COR1 detection of a CME off the SE limb</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/2007-Jul-08.mpg</link>
<description>COR1 detection of a CME off the SE limb on 08-July-2007. It was difficult to detect the leading edge of this event, but there was a strong "concave-out" trailing feature, remniscent of a flux rope morphology.</description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/2007-Jul-08_thumb.jpg</guid>
</item>

<item>
<title>A large CME off the northeast limb</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/2007-May-15b.mpg</link>
<description>A large CME off the northeast limb of the Sun detected on May 15, 2007, by
both COR1-A and -B.</description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/2007-May-15b_thumb.jpg</guid>
</item>

<item>
<title>2007-02-24 Lunar Transit</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/cor1_lunar_transit_halfres.mpg</link>
<description>2007-02-24 The STEREO-B spacecraft was treated to a lunar transit of the solar disk.  This is what the Moon looked like in the COR1 coronagraph as it headed toward the Sun and onward the following day.</description>
<guid>http://cor1.gsfc.nasa.gov/images/thumbnails/cor1_lunar_transit_thumb.jpg</guid>
</item>

<item>
<title>COR1-B North-East Quadrant showing CME</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/20070124_FullRes.avi</link>
<description>2007-01-24 COR1-B North-East Quadrant showing CME at full spatial resolution in polarized brightness (pB)</description>
<guid>http://cor1.gsfc.nasa.gov/images/gallery_images/I1.jpg</guid>
</item>

<item>
<title>CME in polarized brightness (pB)</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/20070124B.avi</link>
<description>2007-01-24 COR1-B full-field images showing CME in polarized brightness (pB)</description>
<guid>http://cor1.gsfc.nasa.gov/images/gallery_images/I2.jpg</guid>
</item>

<item>
<title>Mercury Passage</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/20070503COR1AB_pB256.avi</link>
<description>2007-05-03 COR1-A and COR1-B polarized brightness (pB) movies showing Mercury passage when spacecraft were separated by 6.3 degrees</description>
<guid>http://cor1.gsfc.nasa.gov/images/gallery_images/I3.jpg</guid>
</item>

<item>
<title>COR1-B North-East Quadrant showing CME</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/20070501_FullRes.avi</link>
<description>2007-05-01 COR1-B North-East Quadrant showing CME at full spatial resolution in polarized brightness (pB)</description>
<guid>http://cor1.gsfc.nasa.gov/images/gallery_images/I4.jpg</guid>
</item>

<item>
<title>Comparing various methods of studying CMEs</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/analysis_techniques.gif</link>
<description>A comparison of various methods of studying CMEs From top to bottom, left top right: the polarized brightness movie; the same data, but with the first frame used as a base difference; the same data, this time with the previous frame subtracted (running difference); the wavelet decomposed (atrous wavelet, scale 2) of the same data (25 January 2007, COR1-B).</description>
<guid>http://cor1.gsfc.nasa.gov/images/gallery_images/movie_3.gif</guid>
</item>

<item>
<title>The multiscale canny decomposed data</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/gradient_modulus.gif</link>
<description>The canny decomposition runs a 'Mexican hat' wavelet in each direction and then creates the modulus (plotted here) and the angle of maximum gradient (25 January 2007, COR1-B).</description>
<guid>http://cor1.gsfc.nasa.gov/images/gallery_images/movie_2.gif</guid>
</item>

<item>
<title>Angle of maximum gradient</title>
<link>http://cor1.gsfc.nasa.gov/images/movies/gradient_direction.gif</link>
<description>Angle of maximum gradient, in degrees clockwise from pointing right (black): up is red; left is green; down is blue (25 January 2007, COR1-B).</description>
<guid>http://cor1.gsfc.nasa.gov/images/gallery_images/movie_1.gif</guid>
</item>

<item>
<title>2007-01-24 Polarized Brightness Images</title>
<link>http://cor1.gsfc.nasa.gov/images/gallery_images/20070124_COR1B_animated.gif</link>
<description>2007-01-24 Polarized Brightness images from COR1-B (click on images for larger image)</description>
<guid>http://cor1.gsfc.nasa.gov/images/gallery_images/20070124_1413_COR1B_pB.jpg</guid>
</item>

<item>
<title>2007-01-25 Polarized Brightness Images</title>
<link>http://cor1.gsfc.nasa.gov/images/gallery_images/20070125_COR1B_animated.gif</link>
<description>2007-01-25 Polarized Brightness images from COR1-B (click on images for larger image)</description>
<guid>http://cor1.gsfc.nasa.gov/images/gallery_images/20070124_1413_COR1B_pB.jpg</guid>
</item>

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