Reconstruction of the solar corona from STEREO COR1 observations

Details Reconstruction of the solar corona from STEREO COR1 observations Reconstruction of the solar corona from STEREO COR1 observations

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsh13b1534k&link_type=abstract

American Geophysical Union, Fall Meeting 2008, abstract #SH13B-1534

Astronomy and Astrophysics

Astrophysics

7500 Solar Physics, Astrophysics, And Astronomy, 7509 Corona, 7511 Coronal Holes, 7513 Coronal Mass Ejections (2101), 7524 Magnetic Fields

Scientific paper

The COR1 instruments provide white light observations of the solar corona from 1.5 to 4 Rsun where the transition from closed to open coronal structures takes a place. The reconstruction is performed by the regularized tomography inversion method and gives a 3D distribution of the electron density in the corona from 1.5 to 4 Rsun. The method allows to reconstruct only structures which are stationary during an observation period, i.e. from quarter to half a solar rotation.

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