Astronomy and Astrophysics – Astronomy
Scientific paper
May 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009spd....40.1405k&link_type=abstract
American Astronomical Society, SPD meeting #40, #14.05; Bulletin of the American Astronomical Society, Vol. 41, p.834
Astronomy and Astrophysics
Astronomy
Scientific paper
We analyze the physical properties in an equatorial coronal hole that was observed by Hinode/EIS in two consecutive solar rotations in February and March of 2009. This coronal hole is the obvious source region for the solar wind measured in-situ by ACE and STEREO that exhibits the typical fast-to-slow characteristics in proton speed. We determine the electron density and temperature structures at several locations in the coronal hole that may correspond to the footpoints of the solar wind measured in-situ. We discuss the variations of such properties between locations as well as between the two rotations. We compare and discuss such variations in the coronal hole with the properties in the solar wind, in particular, the ion charge composition.
Ko Yuan-Kuen
Laming Martin J.
Lepri Stefano
Muglach Karin
Popecki Mark
No associations
LandOfFree
Physical Properties In An Equatorial Coronal Hole And Its Connection To The Solar Wind Properties does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Physical Properties In An Equatorial Coronal Hole And Its Connection To The Solar Wind Properties, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Physical Properties In An Equatorial Coronal Hole And Its Connection To The Solar Wind Properties will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1112441