The three-dimensional structure of the solar corona

Details The three-dimensional structure of the solar corona The three-dimensional structure of the solar corona

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sowi.conf...68z&link_type=abstract

Max-Planck-Inst. für Aeronomie, International Solar Wind 8 Conference, p. 68

Computer Science

2

Sun, Solar Corona, Emissivity, Solar Magnetic Field, Three Dimensional Bodies, Visual Observation, Rotation, Computer Aided Tomography, Magnetic Field Configurations

Scientific paper

Due to the rotation of the sun the solar corona can be observed under different directions at different times. Using methods of computer tomography the three-dimensional structure of the emissivity of the solar corona can be reconstructed. We discuss the feasibility of this method for stationary and for non-stationary corona and also for incomplete and finite resolution data. As example we present reconstructions based on YOHKOH-images, and we compare the results with ground-based optical corona observations. Structures are interpreted in terms of the solar magnetic field topology.

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