
doi: 10.1063/1.51466
handle: 11858/00-001M-0000-0014-D6DF-2
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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