Doppler shift measurements on the green coronal line - Evidence for largescale macroscopic mass motion

Details Doppler shift measurements on the green coronal line - Evidence for largescale macroscopic mass motion Doppler shift measurements on the green coronal line - Evidence for largescale macroscopic mass motion

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982japa....3...69d&link_type=abstract

Journal of Astrophysics and Astronomy, vol. 3, Mar. 1982, p. 69-77. Research supported by the Department of Space of India.

Astronomy and Astrophysics

Astrophysics

6

Doppler Effect, Solar Corona, Solar Eclipses, Solar Spectra, Fabry-Perot Interferometers, Light (Visible Radiation), Mass Flow, Temperature Distribution

Scientific paper

Fabry-Perot interferometric observations on the green coronal line (5303
A) carried out during the total solar eclipse of 1980 February 16 have
yielded relative Doppler shift velocities with an accuracy of plus or
minus 7 km/s. The values show a peak in the 30-50 km/s range indicating
largescale macroscopic mass motion in the solar maximum corona.

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