The Spectroscopic Footprint of the Fast Solar Wind

Details The Spectroscopic Footprint of the Fast Solar Wind The Spectroscopic Footprint of the Fast Solar Wind

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsh41a1612m&link_type=abstract

American Geophysical Union, Fall Meeting 2008, abstract #SH41A-1612

Other

7511 Coronal Holes, 7546 Transition Region, 7836 Mhd Waves And Instabilities (2149, 2752, 6050), 7924 Forecasting (2722)

Scientific paper

We explore a large, complex equatorial coronal hole (ECH) and its immediate surroundings through the temperature dependence of the non-thermal line widths of three transition region emission lines observed by SOHO/SUMER, placing them in context with recent studies of the other spectroscopic measures taken. Using a recent semi-empirical model of the solar wind as a basis, we explore the structure of the solar wind during the observing period and seek to gain a better understanding of the interaction of this region with the nascent solar wind.

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