Abstract
A white-light-flare (WLF) was recorded on March 27, 1991 at Tashkent. The WLF occurred at the penumbra of a large, complex sunspot group. The energy released by the WLF per unit time was 2.4 × 1028 erg s-1.
Similar content being viewed by others
References
Slonim Yu. M. and Korobova Z. B.: 1975, Solar Phys.40, 397.
Švestka Z.: 1970, Solar Phys.13, 471.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Korobova, Z.B. The white-light solar flare of March 27, 1991. Sol Phys 139, 205–207 (1992). https://doi.org/10.1007/BF00147891
Issue Date:
DOI: https://doi.org/10.1007/BF00147891