The Herschel effect and solar photography |
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| Authors: | R. Jayanthan |
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| Affiliation: | (1) Math-Hulbert Observatory, The University of Michigan, USA |
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| Abstract: | A method of photographing the solar image in the UV part of the solar spectrum is described. The resulting images show the bright photospheric network of Sheeley and Chapman; these have been recorded at the small central distance of 20°. During a flare of importance 1b near a spot group, no detectable changes in the spots, their relative positions or the bright photospheric network could be observed. |
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