| 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 |