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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3091
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dc.contributor.authorKrishan, V-
dc.date.accessioned2008-08-12T09:28:20Z-
dc.date.available2008-08-12T09:28:20Z-
dc.date.issued2000-12-
dc.identifier.citationPramana - Journal of Physics, Vol. 55, No. 5 - 6, pp. 655 – 663en
dc.identifier.issn0304-4289-
dc.identifier.urihttp://hdl.handle.net/2248/3091-
dc.description.abstractA 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.extent88145 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://www.ias.ac.in/pramana/v55/p655/abs.htmen
dc.subjectGamma Ray Astronomyen
dc.subjectX-Ray Astronomyen
dc.subjectSatellite Missionsen
dc.subjectActive Galactic Nucleien
dc.subjectGamma Ray Burstsen
dc.titleHigh energy universe -- Satellite missionsen
dc.typeArticleen
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