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Stereo Science Results at Solar MinimumThe magnetic fields that drive solar activity are complex and inherently three-dimensional structures. Twisted flux ropes, magnetic reconnection and the initiation of solar storms, as well as space weather propagation through the heliosphere, are just a few of the topics that cannot properly be observed or modeled in only two dimensions. Examination of this three-dimensional complex has been hampered by the fact that solar remote sensing observations have occurred only from the Earth-Sun line, and in situ observations, while available from a greater variety of locations, have been sparse throughout the heliosphere.
Document ID
20100033360
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
Authors
Christian, Eric R.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Kaiser, Michael L.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Kucera Therese A.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
St. Cyr, O. C.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
van Driel-Gesztelyi, Lidia
(Observatoire de Paris-Meudon France)
Mandrini, Cristina H.
(Instituto de Astronomia y Fisica del Espacio Buenos Aires, Argentina)
Date Acquired
August 25, 2013
Publication Date
April 21, 2009
Publication Information
Publication: Solar Physics
Volume: 256
Issue: 1-2
Subject Category
Solar Physics
Distribution Limits
Public
Copyright
Other

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