The Temperature and Density Structure of the Quiet Solar Corona

Details The Temperature and Density Structure of the Quiet Solar Corona The Temperature and Density Structure of the Quiet Solar Corona

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sh31a02w&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SH31A-02

Physics

7509 Corona, 7524 Magnetic Fields

Scientific paper

The temperature and density structure of the quiet solar corona remains unclear. In this poster, we will present a preliminary analysis of a quiet solar coronal loop structure observed with SOHO and TRACE. After determining the magnetic field structure from potential field extrapolation, we attempt to model this loop using RTV scaling laws with various heating functions. This work is in preparation for a full-scale statistical study of SOHO/TRACE data to determine the structure of the quiet solar corona.

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