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Solar Maximum MissionThe paper considers the objectives of the Solar Maximum Mission (SMM), and describes its spacecraft, the scientific planning, the observing program, and the guest investigator programs. The SMM observatory will be injected into a circular orbit with an altitude of 574 km and it is designed for a minimum of one year of operational life; its observing program is directed at the physics of solar flares, and includes studies of thermalization, the nature of electron acceleration, the flare energy budget, and the flare decay. Finally, the SMM Guest Investigator program is discussed, including ground-based synoptic and atomic data investigations and SMM data interpretation.
Document ID
19800041017
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Bohlin, J. D.
(NASA Office of Space Sciences Washington, D.C., United States)
Frost, K. J.
(NASA Goddard Space Flight Center Laboratory for Astronomy and Solar Physics, Greenbelt, Md., United States)
Burr, P. T.
(NASA Headquarters Washington, DC United States)
Guha, A. K.
(NASA Goddard Space Flight Center Projects Management Directorate, Greenbelt, MD., United States)
Withbroe, G. L.
(Harvard-Smithsonian Center for Astrophysics Cambridge, Mass., United States)
Date Acquired
August 10, 2013
Publication Date
February 1, 1980
Publication Information
Publication: Solar Physics
Volume: 65
Subject Category
Astronautics (General)
Accession Number
80A25187
Distribution Limits
Public
Copyright
Other

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