2D_JPG_Images_Comp_Rendering.tar	contains various resolutions of the composite rendering of the STEREO spacecraft, Comet McNaught, the Sun and the Earth
Stereo-McNaught_HR_2k1k.jpg 329K	annotated 2000 by 1000 pixels version of composite rendering
Stereo-McNaught_HR_4k2k.jpg 1110K	annotated 4000 by 2000 pixels version of composite rendering
Stereo-McNaught_HR_8k4k.jpg 2605K	annotated 8000 by 4000 pixels version of composite rendering
Stereo-McNaught_HR_NoText_2k1k.jpg 322K	2000 by 1000 pixels version of composite rendering without annotation
Stereo-McNaught_HR_NoText_4k2k.jpg 1093K	4000 by 2000 pixels version of composite rendering without annotation
Stereo-McNaught_HR_NoText_8k4k.jpg 2565K	8000 by 4000 pixels version of composite rendering without annotation
2D_and_3D_tif_images.tar	includes 2D and 3D images at both full resolution (2k x 2k) and HD resolution (1920 x 1080) Two different color tables were used in the processing of the images.
ACTIVE_20070323_fullres_fulldisk-Cglyph.tif 2605K	Full resolution full disk image that includes view of an active region region on the Sun March 23, 2007. The anaglyph image was created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm
ACTIVE_20070323_fullres_fulldisk-LFT.tif 2140K	Full resolution full disk image that includes view of an active region region on the Sun March 23, 2007. The image was created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm
active_HD_Cglyph.tif 2148K	HD resolution full disk image that includes view of an active region region on the Sun March 23, 2007. The anaglyph image was created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm
active_HD-LFT.tif 1710K	HD resolution full disk image that includes view of an active region region on the Sun March 23, 2007. The image was created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm
Active.Left.tif 2107K	HD resolution full disk image that includes view of an active region region on the Sun March 23, 2007. The image was created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm (different color table)
BOTTOM-RIGHT_20070320_fullres_fulldisk_Cglyph.tif 3315K	Full resolution full disk anaglyph image that includes right limb of south pole of the Sun on March 18, 2007, created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm. A prominence is clearly visible.
BOTTOM-RIGHT_20070320_fullres_fulldisk-LFT.tif 2408K	Full resolution full disk image that includes right limb of south pole of the Sun on March 18, 2007, created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm. A prominence is clearly visible.
bottomRight_HD-Cglyph.tif 1475K	HD resolution image of right limb of south pole of the Sun on March 18, 2007, created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm. A prominence is clearly visible. (Anaglyph)
bottomRight_HD-LFT.tif 1173K	HD resolution image of right limb of south pole of the Sun on March 18, 2007, created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm. A prominence is clearly visible.
BottomRight.Left.tif 1549K	HD resolution image of right limb of south pole of the Sun on March 18, 2007, created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm. A prominence is clearly visible. (Second color table)
FULL_20070326_fullres_fulldisk-Cglyph.tif 2827K	Full resolution full disk ANAGLYPH image of the Sun on March 26, 2007, created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm. The structure of the corona shows well in this image.
FULL_20070326_fullres_fulldisk-LFT.tif 2155K	Full resolution full disk image of the Sun on March 26, 2007, created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm. The structure of the corona shows well in this image.
full_HD_Cglyph.tif 6087K	HD resolution image of full disk ANAGLYPH image of the Sun on March 26, 2007, created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm. The structure of the corona shows well in this image.
full_HD-LFT.tif 1077K	HD resolution image of full disk image of the Sun on March 26, 2007, created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm. The structure of the corona shows well in this image.
Full.Left.tif 6087K	HD resolution image of full disk image of the Sun on March 26, 2007, created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm. The structure of the corona shows well in this image. (Second color table)
HOLE_20070324_fullres_fulldisk-Cglyph.tif 2910K	Full resolution full disk image that includes view of the equatorial region of the Sun on March 24, 2007. The anaglyph image was created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm.
HOLE_20070324_fullres_fulldisk-LFT.tif 2321K	Full resolution full disk image that includes view of the equatorial region of the Sun on March 24, 2007. The image was created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm.
hole_HD_Cglyph.tif 2488K	HD resolution image containing a closer view of the equatorial region of the Sun on March 24, 2007. The anaglyph image was created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm.
hole_HD-LFT.tif 2033K	HD resolution image containing a closer view of the equatorial region of the Sun on March 24, 2007. The image was created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm.
Hole.Left.tif 2329K	HD resolution image containing a closer view of the equatorial region of the Sun on March 24, 2007. The image was created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm. (second color table used)
NORTH-POLE_20070320_fullres_fulldisk-Cglyph.tif 2964K	Full resolution full disk image that includes north pole of the Sun on March 20, 2007, anaglyph created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm. A large spicule can be seen.
NORTH-POLE_20070320_fullres_fulldisk-LFT.tif 2357K	Full resolution full disk image that includes north pole of the Sun on March 20, 2007, created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm. A large spicule can be seen.
northPole_HD_Cglyph.tif 1785K	HD resolution image of the north pole of the Sun on March 20, 2007, anaglyph created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm. A large spicule can be seen.
northPole-HD_LFT.tif 1369K	HD resolution image of the north pole of the Sun on March 20, 2007, created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm. A large spicule can be seen.
NorthPole.Left.tif 1692K	HD resolution image of the north pole of the Sun on March 20, 2007, created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm. A large spicule can be seen. (second color table used)
SOUTH-POLE_20070320_fullres_fulldisk-Cglyph.tif 3008K	Full resolution full disk image that includes south pole of the Sun on March 20, 2007, anaglyph created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm.
SOUTH-POLE_20070320_fullres_fulldisk-LFT.tif 2405K	Full resolution full disk image that includes south pole of the Sun on March 20, 2007, created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm.
southPole_HD-Cglyph.tif 1646K	HD resolution anaglyph image of the south pole of the Sun on March 20, 2007, created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm.
southPole_HD-LFT.tif 1440K	HD resolution image of the  south pole of the Sun on March 20, 2007, created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm.
SouthPole.Left.tif 1713K	HD resolution image of the  south pole of the Sun on March 20, 2007, created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm. (second color table)
TOP-LEFT_20070318_fullres_fulldisk-Cglyph.tif 2909K	Full resolution full disk image that includes left limb of north pole  of the Sun on March 18, 2007, anaglyph created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm.
TOP-LEFT_20070318_fullres_fulldisk-LFT.tif 2310K	Full resolution full disk image that includes left limb of north pole  of the Sun on March 18, 2007, created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm.
top_left_HD_Cglyph.tif 1250K	HD resolution anaglyph image of left limb of north pole  of the Sun on March 18, 2007, created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm.
top_left_HD-LFT.tif 1019K	HD resolution image of left limb of north pole  of the Sun on March 18, 2007, created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm.
TopLeft.Left.tif 1603K	HD resolution image of left limb of north pole  of the Sun on March 18, 2007, created by combining images in three of the four EUVI wavelengths: 304, 171 and 195 nm. (second color table)
3D_animations.tar	3D Anaglyph animations of data from STEREO spacecraft, to be viewed with red-cyan glasses
171_Active_Region_Ana.mov	3D HD resolution animation showing sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO A & B in the 171 nm wavelength, showing a portion of the equatorial region of the solar disk to provide a close up view of the active region.
171_Full_Disk_Ana.mov	3D HD resolution animation showing full disk sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO A & B in the 171 nm wavelength.
195_Full_Disk_Ana.mov	3D HD resolution animation showing full disk sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO B in the 195 nm wavelength
195_Left_Limb_Ana.mov	3D HD resolution animation showing sequence of images from February 24, 2007 taken by the EUVI telescope from STEREO A & B in the 195 nm wavelength, showing a close up of an active region eruption at the limb.
284_Active_Region_Ana.mov	3D HD resolution animation showing sequence of images covering Mar 17-27, 2007 taken by the EUVI telescope from STEREO A & B in the 284 nm 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.
284_Full_Disk_Ana.mov	3D HD resolution animation showing full disk sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO A & B in the 284 nm wavelength. The aftermath of the eruption of a prominence which occurred on March 24, 2007 is evident in the sequence.
304_Active_Region_Ana.mov	3D HD resolution animation showing sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO A & B in the 304 nm wavelength, showing a portion of the equatorial region of the solar disk.
304_Full_Disk_Ana.mov	3D HD resolution animation showing full disk sequence of images covering Mar. 17-27, 2007 taken by the EUVI telescope from STEREO A & B in the 304 nm wavelength. Two promience eruptions are visible in this segment. The one on the lower right limb occurred on Mar. 20 and the one barely visible on the disk occurred on Mar. 24.
Solar_Model_Ana.mov	3D HD resolution animation showing 1)Results from a three dimensional computation of the magnetic field structure of an active region extrapolating the fields from measurements of the magnetic field on the surface of the Sun. This model assumes there are no electrical currents in the corona, leading to a very simple magnetic configuration.  From Tahar Amari, Centre de Physique Theorique, Ecole Polytechnique, Paris. 2)Results from a three dimensional computation of the magnetic field structure of an active region extrapolating the fields from measurements of the magnetic field on the surface of the Sun. This model allows currents to flow and assumes force balance, leading to a more complex magnetic configuration for the same surface magnetic fields. From Tahar Amari. 3)Results from a three dimensional computation of the magnetic field structure of the corona extrapolating the fields from measurements of the magnetic field on the surface of the Sun. This models the corona for February 2007. Model from Pete Riley, SAIC, San Diego.
2D_STEREO_B_animations.tar	2D animations of data from STEREO B spacecraft
171_Active_Region_Left.mov	HD resolution animation showing sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO B in the 171 nm wavelength, showing a portion of the equatorial region of the solar disk to provide a close up view of the active region.
171_Full_Disk_Left.mov	HD resolution animation showing full disk sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO B in the 171 nm wavelength.
195_Full_Disk_Left.mov	HD resolution animation showing full disk sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO B in the 195 nm wavelength
195_Left_Limb_Left.mov	HD resolution animation showing sequence of images from February 24, 2007 taken by the EUVI telescope from STEREO B in the 195 nm wavelength, showing a close up of an active region eruption at the limb.
284_Active_Region_Left.mov	HD resolution animation showing sequence of images covering Mar 17-27, 2007 taken by the EUVI telescope from STEREO B in the 284 nm 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.
284_Full_Disk_Left.mov	HD resolution animation showing full disk sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO B in the 284 nm wavelength. The aftermath of the eruption of a prominence which occurred on March 24, 2007 is evident in the sequence.
304_Active_Region_Left.mov	HD resolution animation showing sequence of images covering March 17-March 27, 2007 taken by the EUVI telescope from STEREO B in the 304 nm wavelength, showing a portion of the equatorial region of the solar disk.
304_Full_Disk_Left.mov	HD resolution animation showing full disk sequence of images covering Mar. 17-27, 2007 taken by the EUVI telescope from STEREO B in the 304 nm wavelength. Two promience eruptions are visible in this segment. The one on the lower right limb occurred on Mar. 20 and the one barely visible on the disk occurred on Mar. 24.
FOV_Earth_Fixed_Left.mov	HD resolution 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.
FOV_Sun_Fixed_Left.mov	HD resolution 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.
Solar_Model_Left.mov	HD resolution animation showing 1)Results from a three dimensional computation of the magnetic field structure of an active region extrapolating the fields from measurements of the magnetic field on the surface of the Sun. This model assumes there are no electrical currents in the corona, leading to a very simple magnetic configuration.  From Tahar Amari, Centre de Physique Theorique, Ecole Polytechnique, Paris. 2)Results from a three dimensional computation of the magnetic field structure of an active region extrapolating the fields from measurements of the magnetic field on the surface of the Sun. This model allows currents to flow and assumes force balance, leading to a more complex magnetic configuration for the same surface magnetic fields. From Tahar Amari. 3)Results from a three dimensional computation of the magnetic field structure of the corona extrapolating the fields from measurements of the magnetic field on the surface of the Sun. This models the corona for February 2007. Model from Pete Riley, SAIC, San Diego.
Spacecraft_Deploy_Left.mov	HD resolution 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.
Other_2D_animations.tar	animations not included in previous tar files, overview of STEREO mission and a recent highlights animation
Spacecraft_Animations.mov	HD resolution 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.
stereo capture_vga_h264.mov	NTSC resolution animation giving an overview of the STEREO mission.