dc.contributor.author |
Krishan, V |
|
dc.date.accessioned |
2008-08-12T09:28:20Z |
|
dc.date.available |
2008-08-12T09:28:20Z |
|
dc.date.issued |
2000-12 |
|
dc.identifier.citation |
Pramana - Journal of Physics, Vol. 55, No. 5 - 6, pp. 655 – 663 |
en |
dc.identifier.issn |
0304-4289 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3091 |
|
dc.description.abstract |
A variety of satellite missions to observe the high energy universe are currently operating and some more with more versatility and capability are on the anvil. In this paper, after giving a brief introduction to the constituents of the high energy universe and the related plasma physical problems, general as well as specific features of the current and future x-ray and gamma-ray satellite missions are described. |
en |
dc.format.extent |
88145 bytes |
|
dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
en |
dc.publisher |
Indian Academy of Sciences |
en |
dc.relation.uri |
http://www.ias.ac.in/pramana/v55/p655/abs.htm |
en |
dc.subject |
Gamma Ray Astronomy |
en |
dc.subject |
X-Ray Astronomy |
en |
dc.subject |
Satellite Missions |
en |
dc.subject |
Active Galactic Nuclei |
en |
dc.subject |
Gamma Ray Bursts |
en |
dc.title |
High energy universe -- Satellite missions |
en |
dc.type |
Article |
en |