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Coronal Holes and Solar Wind Acceleration (Hardcover, 1999 ed.)
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Discovery Miles 46 430
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Coronal Holes and Solar Wind Acceleration (Hardcover, 1999 ed.)
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The SOHO-7 Workshop was held from 28 September through 1 October
1998 at the Asticou Inn in Northeast Harbor, Maine. The primary
topic of this Workshop was the impact of SOHO observations on our
understanding of the nature and evolution of coronal holes and the
acceleration and composition of the solar wind. The presentations
and discussions occasionally went beyond this topic to include the
impact of the reported research on other solar structures and the
heliosphere. SOHO (the Solar and Heliospheric Observatory), a
project of international cooperation between ESA and NASA, was
launched in December 1995 and began its science operations during
the first few months of 1996. To many solar and space physicists,
it was a great advantage that SOHO began itscomprehensive look at
the Sun during the 1996 solar minimum. The qualitatively simple
two-phase corona, with polar coronal holes expanding into the
high-speed solar wind, and a steady equatorial streamer belt
related somehow to the stochastic slow-speed solar wind, allowed
various SOHO diagnostics to be initiated with a reasonably well
understoodcircumsolar geometry. The analysis of subsequentSOHO
measurements made during the rising phase of solar cycle 23 will
continue to benefit from what has been learned from the first two
years of data.
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