Gamma-Ray Line Observations with RHESSI

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dc.creatorSmith, David M.
dc.date2004-04-30
dc.date.accessioned2026-07-07T02:13:02Z
dc.date.available2026-07-07T02:13:02Z
dc.descriptionThe Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) has been observing gamma-ray lines from the Sun and the Galaxy since its launch in February 2002. Here I summarize the status of RHESSI observations of solar lines (nuclear de-excitation, neutron capture, and positron annihilation), the lines of $^{26}$Al and $^{60}$Fe from the inner Galaxy, and the search for positron annihilation in novae.
dc.description6 pages, 6 figures, accepted for the proceedings of the 5th INTEGRAL workshop, "The INTEGRAL Universe", ESA
dc.identifierhttps://arxiv.org/abs/astro-ph/0404594
dc.identifierhttp://arxiv.org/abs/astro-ph/0404594
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7674
dc.subjectAstrophysics
dc.titleGamma-Ray Line Observations with RHESSI
dc.typetext

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