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STEREO SCIENCE CENTER

Latest SECCHI beacon images

Shown here are the latest SECCHI beacon images. The STEREO space weather beacon telemetry mode is a very low rate, highly compressed data stream broadcast by the spacecraft 24 hours per day. These data are used for space weather forecasting. Because of the large compression factors used, these beacon images are of much lower quality than the actual science data.

Realtime resources:     Browse resources:

EUVI 195 heliographic
map
Same data as rotating GIF movie

STEREO Behind SOHO / MLSO STEREO Ahead
/browse/2010/02/10/behind/euvi/195/256/20100210_020530_n7euB_195.jpg soho_eit_195.jpg /browse/2010/02/10/ahead/euvi/195/256/20100210_051530_n7euA_195.jpg
2048,1024,512,256,128 2048,1024,512,256,128
MPEG: 512,256 MPEG: 512,256
/browse/2010/02/10/behind/cor1/256/20100210_020518_s7c1B.jpg latest.mk4.gif /browse/2010/02/09/ahead/cor1/256/20100209_110518_s7c1A.jpg
1024,512,256,128 1024,512,256,128
MPEG: 512,256
/browse/2010/02/10/behind/cor2/256/20100210_020935_n7c2B.jpg soho_c2.jpg /browse/2010/02/10/ahead/cor2/256/20100210_050935_n7c2A.jpg
2048,1024,512,256,128 2048,1024,512,256,128
MPEG: 512,256 MPEG: 512,256

The images above are shown in the order of the relative positions of the three viewpoints, Behind, Earth, and Ahead. For the Heliospheric Imager (HI) images below, the order is reversed to reflect the fact that the HI Ahead telescopes look to the left of the Sun, and those on Behind look to the right. Also, the HI images are not rotated to put solar north up.

STEREO Ahead STEREO Behind
/browse/2010/02/10/ahead/hi1/256/20100210_051801_s7h1A.jpg /browse/2010/02/10/behind/hi1/256/20100210_011801_s7h1B.jpg
1024,512,256,128 1024,512,256,128
MPEG: 512,256
/browse/2010/02/09/ahead/hi2/256/20100209_094721_s7h2A.jpg /browse/2010/02/09/behind/hi2/256/20100209_214721_s7h2B.jpg
1024,512,256,128 1024,512,256,128

The data on this page include telemetry collected by the following organizations:

  • NASA Deep Space Network
  • National Institute of Information and Communications Technology: Koganei, Japan
  • Centre National d'Etudes Spatiales: Toulouse, France
  • Amateur station DL0SHF, Kiel-Ronne, Germany
  • AMSAT-DL/Bochum Observatory, Germany
We would also like to acknowlege the past assistance from the following organizations:
  • Rutherford Appleton Laboratory: Chilbolton, UK


Last Revised: Wednesday, 10-Feb-2010 00:42:06 EST
Responsible NASA Official: Joseph B. Gurman
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