How bright is the (Si X) 1431 NM coronal emission line?

Details How bright is the (Si X) 1431 NM coronal emission line? How bright is the (Si X) 1431 NM coronal emission line?

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..151...51p&link_type=abstract

Solar Physics, vol. 151, no. 1, p. 51-56

Astronomy and Astrophysics

Astronomy

3

Brightness, Emission Spectra, Line Spectra, Solar Corona, Solar Spectra, Spectroscopic Analysis, Astronomical Photography, Coronagraphs, Infrared Radiation, Silicon, Spaceborne Astronomy, Spectrographs

Scientific paper

Airborne eclipse observations of the (Si X) 1430.5 nm coronal emission line are reviewed, and new ground-based out-of-eclipse coronagraph observations obtained at NSO/Sacramento Peak are reported. We find that the (Si X) 1430.5 nm coronal emission line brightness is less than 8 x 10-6 B in small active region corona which showed (Fe XIII) 1074.7 nm emission (corrected for sky background) of about 20 x 10-6 B.

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