On three-dimensional reconstruction of optically thin solar emission sources

Details On three-dimensional reconstruction of optically thin solar emission sources On three-dimensional reconstruction of optically thin solar emission sources

May 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977stin...7727056k&link_type=abstract

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Mathematics

Lattices (Mathematics), Linear Transformations, Solar Corona, Solar Spectra, Ultraviolet Radiation, Astronomical Coordinates, Matrices (Mathematics), Oso-7, Solar Activity, Spectroheliographs

Scientific paper

Calculations are given for constructing the three dimensional distribution of optically thin EUV emission sources associated with solar active regions, from two dimensional observations (projections) recorded by the spectroheliograph on the OSO 7 satellite. The relation of the method to other image reconstruction methods is briefly discussed as well as the special requirements imposed in the solar case such as a knowledge of the true solar rotation function. A useful correlation criterion for establishing the physical validity of solutions is given.

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