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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References
Chapman, G. A. and Sheeley, N. R.: 1968,Solar Phys. 5, 442.
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Herschel, J. F. W.: 1840,Phil. Trans. 131, 1.
Schmahl, G.: 1967,Z. Astrophys. 66, 81.
Sheeley, N. R.: 1967,Solar Phys. 1, 171.
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Jayanthan, R. The Herschel effect and solar photography. Sol Phys 12, 163–166 (1970). https://doi.org/10.1007/BF02276575
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DOI: https://doi.org/10.1007/BF02276575