Quantitative analysis of SKYLAB X-ray pictures of the sun by means of iterative deconvolution

Details Quantitative analysis of SKYLAB X-ray pictures of the sun by means of iterative deconvolution Quantitative analysis of SKYLAB X-ray pictures of the sun by means of iterative deconvolution

Apr 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981soph...70..273m&link_type=abstract

Solar Physics, vol. 70, Apr. 1981, p. 273-291.

Physics

2

Convolution Integrals, Iteration, Quantitative Analysis, Solar Corona, Solar Temperature, X Ray Imagery, Fourier Analysis, Point Spread Functions, Skylab Program, Solar Magnetic Field, X Ray Telescopes

Scientific paper

Because of the broad wings of the point spread function of the Wolter telescopes used in the Skylab mission for taking X-ray pictures of the solar corona, the images are blurred around bright emission regions. Consequently, the maps of temperature and emission measure are distorted. This paper presents a procedure for the iterative deconvolution of X-ray pictures and examines its application to Skylab images of McMath 488 and McMath 427 and 417.

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