Localization of Solar X-ray Emission at Energies above 3 keV

Details Localization of Solar X-ray Emission at Energies above 3 keV Localization of Solar X-ray Emission at Energies above 3 keV

Jul 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970natur.227...55c&link_type=abstract

Nature, Volume 227, Issue 5253, pp. 55-56 (1970).

Physics

1

Scientific paper

SOLAR, X-ray emission becomes increasingly localized to active regions as the photon energy increases. Photographs of the Sun at X-ray energies less than 0.5 keV show emission from the entire corona, while those sensitive in the 1-3 keV interval show the X-ray emission to be concentrated in condensed regions1,2 which are correlated with features apparent at both optical and radio wavelengths. If this trend were to continue as expected, X-rays at energies above 3 keV would be emitted exclusively from active regions with little or no contribution from the general corona.

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