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A spacecraft going behind the Sun will support SOHOThe problems that can be solved by combining the Solar and Heliospheric Observatory (SOHO) and the magnetic structures on and around the sun (MagSonas) observations are discussed. A magneto-Doppler imager and X and Ka band linearly polarized radio signals sent to the other side of the sun can support extended SOHO mission. This is the purpose of the MagSonas mission. The MagSonas radio system, designed to serve as spacecraft communications and a sounding coronal magnetic field, is described.
Document ID
19990028139
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
Authors
Ruzmaikin, A.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Anderson, J. D.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Asmar, S.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Bird, M.
(Bonn Univ. Germany)
Cacciani, A.
(La Sapienza Univ. Rome, Italy)
Coles, W.
(California Univ. San Diego, CA United States)
Feynman, J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Harvey, J.
(National Solar Observatory Tucson, AZ United States)
Harvey, K.
(National Solar Observatory Tucson, AZ United States)
Hollweg, J.
(New Hampshire Univ. Durham, NH United States)
Linker, J.
(Science Applications International Corp. San Diego, CA United States)
Mikic, Z.
(Science Applications International Corp. San Diego, CA United States)
Paezold, M.
(Leipzig Univ. German Democratic Republic)
Smith, E. J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Date Acquired
August 19, 2013
Publication Date
September 1, 1997
Subject Category
Solar Physics
Distribution Limits
Public
Copyright
Other
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