Reconstruction of the coronal electron density at heights from 1.5 to 4 Rsun

Details Reconstruction of the coronal electron density at heights from 1.5 to 4 Rsun Reconstruction of the coronal electron density at heights from 1.5 to 4 Rsun

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agusmsp31d..01k&link_type=abstract

American Geophysical Union, Spring Meeting 2008, abstract #SP31D-01

Astronomy and Astrophysics

Astrophysics

7500 Solar Physics, Astrophysics, And Astronomy, 7509 Corona, 7524 Magnetic Fields

Scientific paper

We present a reconstruction of the electron density structure in the solar corona from 1.5 to 4 Rsun. The reconstruction is performed by the regularized tomography inversion method and based on the STEREO COR1 pB-images. The reconstruction is made for the period of relatively quite Sun. The reconstructed density structure of the equatorial streamer belt in a most of the reconstructed domain is consistent with the variation of the current sheet derived from a potential magnetic field model. However, there are also regions where this correlation is less clear.

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