Chromospheric Flare Enhancements in the Extreme Ultraviolet and their Relationship with Solar Abundances

Details Chromospheric Flare Enhancements in the Extreme Ultraviolet and their Relationship with Solar Abundances Chromospheric Flare Enhancements in the Extreme Ultraviolet and their Relationship with Solar Abundances

Oct 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969natur.224..352b&link_type=abstract

Nature, Volume 224, Issue 5217, pp. 352-353 (1969).

Physics

Scientific paper

Hall and Hinteregger1 have discussed the enhancement of the
extreme ultraviolet (EUV) intensities of spectral lines during the
near-maximum stage of a class 3 flare. Here I suggest a relationship
between the enhancement of a given line and the abundance of the element
from which it is radiating.

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