Mathematics – Probability
Scientific paper
Dec 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsh41b1622i&link_type=abstract
American Geophysical Union, Fall Meeting 2008, abstract #SH41B-1622
Mathematics
Probability
7511 Coronal Holes, 7524 Magnetic Fields, 7529 Photosphere
Scientific paper
We present the magnetic landscape of the polar region of the Sun as observed with Hinode (Tsuneta et al 2008). We found many vertically-oriented magnetic flux tubes with field strength as strong as 1 kG that are scattered in the whole polar region. They all have the same polarity. Probability distribution function, that is number of pixels as a function of the magnetic field strength, for the unsigned vertical field strength is exactly the same as that for the quiet Sun. Uni-polarity of the polar region differentiates it from the quiet Sun, which has mixed polarity. Difference and similarity between the quiet sun and the polar regions are summarized (Ito and Tsuneta, 2008), and its implication for the solar wind acceleration will be discussed.
Fujiki Ken'ichi
Ito Hiroyuki
Shiota Daikou
Tokumaru Munetoshi
Tsuneta Saku
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