Transient Coronal Holes: EUV and IR HeI 1083nm Observations

Details Transient Coronal Holes: EUV and IR HeI 1083nm Observations Transient Coronal Holes: EUV and IR HeI 1083nm Observations

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agufmsh53b0328d&link_type=abstract

American Geophysical Union, Fall Meeting 2004, abstract #SH53B-0328

Physics

7507 Chromosphere, 7509 Corona, 7511 Coronal Holes, 7513 Coronal Mass Ejections, 7549 Ultraviolet Emissions

Scientific paper

We present cases of transient coronal holes following a CME observed simultaneously by SOHO/EIT and the instruments at Mauna Loa Solar Observatory (MLSO). We describe the formation of the transient coronal holes and their relationship to the flare evolution, filament eruption, and CME taking advantage of the high 3-minute temporal cadence of the MLSO observations. We find that transient coronal holes in HeI 1083nm correspond well to the EUV ones, both spatially and temporally

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