Solar Wind Effects of a Persistent, High Latitude Coronal Brightness Enhancement

Details Solar Wind Effects of a Persistent, High Latitude Coronal Brightness Enhancement Solar Wind Effects of a Persistent, High Latitude Coronal Brightness Enhancement

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agufmsh53a1074p&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SH53A-1074

Physics

2102 Corotating Streams, 2169 Solar Wind Sources, 7509 Corona, 7524 Magnetic Fields

Scientific paper

An analysis of SOHO LASCO C2 images over 1996-2005 defines the years and latitudes at which bright, white light coronal structures are most persistent from rotation to rotation. In the northern hemisphere, these features are most notable for the years 2002-2003 and the latitudes 40-60 degrees. This time interval overlaps that of a north pole passage of Ulysses. As Ulysses passes overhead, solar rotation sweeps the interplanetary extensions of these persistent coronal features over the spacecraft, thereby revealing the interplanetary effects of very bright and recurrent K-corona at high solar latitudes.

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