Luminosity conditions of CR IX and Fe XI in the corona

Details Luminosity conditions of CR IX and Fe XI in the corona Luminosity conditions of CR IX and Fe XI in the corona

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974amap.nasa...69a&link_type=abstract

"In its Astrometrics and Astrophysics, No. 17 (NASA-TT-F-15768) p 69-74 (SEE N75-21164 12-88) Transl. into ENGLISH from the boo

Astronomy and Astrophysics

Astrophysics

Line Spectra, Luminous Intensity, Solar Corona, Electron Density (Concentration), Electron Energy, Ion Distribution, Photometers, Transition Probabilities

Scientific paper

Coronal lines of wavelength 4566 A Cr IX and wavelength 3986 A Fe XI
were studied. The electron temperature in the corona was found along
with the electron density, and calculations were performed for Cr IX ion
populations of levels. The lines were scanned photometrically within the
limits of altitudes of 48,000-110,000 km.

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