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Panasyuk 1999

Panasyuk, A.V. (1999). Three-dimensional reconstruction of UV emissivities in the solar corona using Ultraviolet Coronagraph Spectrometer data from the Whole Sun Month. Journal of Geophysical Research 104: doi: 10.1029/1998JA900118. issn: 0148-0227.

UV coronal intensity data collected by the Ultraviolet Coronagraph Spectrometer on SOHO in a daily synoptic program during the Whole Sun Month are used to reconstruct the three-dimensional distribution of emissivities in the solar corona for H I Ly &agr; and the O VI doublet at 1032 and 1037 ¿. We discuss the specifics that complicate a tomographic reconstruction of the solar corona and estimate the uncertainties introduced in the reconstruction by them. ¿ 1999 American Geophysical Union

BACKGROUND DATA FILES

	Abstract

Keywords
Solar Physics, Astrophysics, and Astronomy, Space Plasma Physics, Nonlinear phenomena

Journal
Journal of Geophysical Research
http://www.agu.org/journals/jb/

Publisher
American Geophysical Union
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