Source Region of the Solar Wind Identified with Hinode X-Ray Telescope

Details Source Region of the Solar Wind Identified with Hinode X-Ray Telescope Source Region of the Solar Wind Identified with Hinode X-Ray Telescope

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008asthe.101..491s&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 101, No. 9, p. 491 - 496 (2008)

Astronomy and Astrophysics

Astronomy

X-Ray Telescope, Solar Wind, Coronal Holes

Scientific paper

A possible source region for the slow solar wind was identified with the X-Ray Telescope aboard Hinode satellite. Continuous outflow of hot (~ 1 MK) plasmas was found to emanate from the edge of a solar active region adjacent to a coronal hole. Magnetic field lines along which outflowing plasmas propagate are most likely opened toward the interplanetary space. Hence the observed outflow would constitute a part of the solar wind.

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