Astrophysics with HESSI

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dc.creatorSmith, D. M.
dc.creatorLin, R. P.
dc.creatorMcTiernan, J.
dc.creatorSlassi-Sennou, A. S.
dc.date1998-12-09
dc.date.accessioned2026-07-07T02:29:34Z
dc.date.available2026-07-07T02:29:34Z
dc.descriptionIn the summer of the year 2000, a NASA Small Explorer satellite, the High Energy Solar Spectroscopic Imager (HESSI), will be launched. It will consist of nine large, coaxial germanium detectors viewing the Sun through a set of Rotation Modulation Collimators and will accomplish high-resolution imaging and spectroscopy of solar flares in the x-ray and gamma-ray bands. Here we describe some of the astrophysical observations HESSI will also perform in addition to its solar mission.
dc.descriptionTo be published in Astrophysical Letters and Communications, in the Proceedings of the 3rd INTEGRAL Workshop, Taormina, Sicily, September 1998
dc.identifierhttps://arxiv.org/abs/astro-ph/9812184
dc.identifierhttp://arxiv.org/abs/astro-ph/9812184
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13521
dc.subjectAstrophysics
dc.titleAstrophysics with HESSI
dc.typetext

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