Apr 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aps..aprh14001h&link_type=abstract
American Physical Society, April Meeting, April 29-May 2, 2000 Long Beach, CA, abstract #H14.001
Physics
Scientific paper
Our understanding of the acceleration of the solar wind is based largely on E. N. Parker’s work more than three decades ago. With steadily improving observations (and concomitant theoretical research) of the outer solar atmosphere and the solar wind, however, this understanding has progressed significantly. Nevertheless, we have yet to answer certain fundamental questions concerning the origin, transport, and dissipation of energy required to heat the solar corona and drive the solar wind. This talk will outline our present understanding of solar wind acceleration and some of the questions that remain to be answered.
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