Fabry-Perot interferometric observations of the coronal red and green lines during the 1983 Indonesian eclipse

Details Fabry-Perot interferometric observations of the coronal red and green lines during the 1983 Indonesian eclipse Fabry-Perot interferometric observations of the coronal red and green lines during the 1983 Indonesian eclipse

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apopt..23..508c&link_type=abstract

Applied Optics (ISSN 0003-6935), vol. 23, Feb. 1, 1984, p. 508-511. Research supported by the Department of Space of India, U.S.

Physics

Optics

12

Fabry-Perot Interferometers, Solar Corona, Solar Eclipses, Solar Instruments, Solar Spectra, Collimation, Emission Spectra, Image Filters

Scientific paper

A dual-channel Fabry-Perot interferometric system was used to study simultaneously the coronal emission lines at 5303 Å (Fe XIV) and at 6374 Å (Fe X). Initial results indicate an emission corona confined largely within 1.2 R_sun;. Doppler temperatures derived from the width of the 5303-Å line appear to be appreciably lower than similar temperatures determined during the solar-maximum eclipse of 1980.

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