CYlindrical GAmma-ray Monitor  

 WHAT RESULTS MAY ONE EXPECT AFTER A YEAR OF 
CYGAM FLIGHT IN THE HIGH APOGEE ORBIT?   

  • Distribution of the Galaxy diffuse emission with high angular resolution allowing to refine the spatial distribution of the cosmic-ray protons in the Galaxy. 

  • More than 1000 compact sources with the fraction of degree location accuracy and continuouse monitoring of their flux time variation. 

  • Up to 10 new gamma-ray pulsars emitting in the very high energy range. 

  • Several high energy gamma-ray bursts with the fraction of degree localization accuracy. 

  • In the years of high solar activity up to 10 solar flares with very high energy gamma emission. 

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CYGAM (PDF, 450 Kb)

Space Research Institute,  2002- 2003
 

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Last updated on 10.06.03