Tomographic inversion of coronagraph images

Details Tomographic inversion of coronagraph images Tomographic inversion of coronagraph images

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..382..165z&link_type=abstract

Proceedings of the eigth international solar wind conference: Solar wind eight. AIP Conference Proceedings, Volume 382, pp. 165

Computer Science

4

Image Processing, Magnetohydrodynamics And Plasmas, Solar Instruments

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 electron density in 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 a reconstruction based on images of the Mark III K-coronameter on Hawaii.

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