Coronal temperature measurements near a helmet structure base at the 1973 solar eclipse

Details Coronal temperature measurements near a helmet structure base at the 1973 solar eclipse Coronal temperature measurements near a helmet structure base at the 1973 solar eclipse

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...94..239b&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 94, Sept. 1984, p. 239-247. NSF-supported research.

Physics

7

Solar Corona, Solar Eclipses, Solar Spectra, Solar Temperature, Emission Spectra, Spectral Line Width, Visible Spectrum

Scientific paper

Observations of coronal Fe XIV emission lines from the NE quadrant
during the 1973 solar eclipse are reported. Temperatures are deduced
from a pure thermal broadening model, and, in the region near an
observed white-light enhancement, an alternative interpretation of
halfwidth as being in part due to turbulent velocities is suggested.

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