Abstract
A flare-loop prominence appeared over a complex sunspot group in McMath region No. 11895, on May 24,1972. The evolution of the loop prominence and its relation to a flare were observed using Hα and Ca K filters. Soft X-ray emission between 0.5–20 Å was found to be emitted from the flare-loop prominence system.
Similar content being viewed by others
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Dizer, M. A loop prominence system observed on May 24, 1972. Sol Phys 59, 357–360 (1978). https://doi.org/10.1007/BF00951840
Received:
Revised:
Issue Date:
DOI: https://doi.org/10.1007/BF00951840