Relating X-ray Luminosity of Flares Observed by XRT to Magnetic Flux and the Solar Wind

Details Relating X-ray Luminosity of Flares Observed by XRT to Magnetic Flux and the Solar Wind Relating X-ray Luminosity of Flares Observed by XRT to Magnetic Flux and the Solar Wind

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..397..106k&link_type=abstract

First Results From Hinode ASP Conference Series, Vol. 397, Proceedings of the conference held 20-24 August, 2007, at Trinity Col

Astronomy and Astrophysics

Astronomy

Scientific paper

The X-ray Telescope (XRT) on-board Hinode shows stunning images of reconnection events associated with flares. These flares release a large fraction of their energy in the EUV and X-rays. In a recent paper by Schwadron et al. (2006), the relationship between x-ray luminosity, magnetic flux and the power available for solar wind acceleration was explored. Using Hinode XRT data from AR 10960 and complementary magnetic field data, we examine the x-ray luminosity with respect to the magnetic field flux. These results are compared with the predicted power of the solar wind and measurements taken at the ACE spacecraft at 1AU.

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