Modification of solar lines propagating through the interplanetary medium

Details Modification of solar lines propagating through the interplanetary medium Modification of solar lines propagating through the interplanetary medium

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979jgr....84..979w&link_type=abstract

Journal of Geophysical Research, vol. 84, Mar. 1, 1979, p. 979-982.

Other

8

H Alpha Line, Interplanetary Medium, Line Spectra, Lyman Alpha Radiation, Solar Radiation, Solar Spectra, Absorption Spectra, Helium, Saturn (Planet), Ultraviolet Spectra, Uranus (Planet)

Scientific paper

The optical depths of the solar H Lyman-alpha and the He 584-A lines in interplanetary space are calculated. From these the solar line profiles at Saturn and Uranus are determined. It is found that the solar H Lyman-alpha line can be diminished strongly within a spectral region of less than 0.2 A from the line center. On the other hand, there is no significant absorption of the He 584-A line except in the downwind region, where absorption occurs within a spectral region of about 0.04 A. The effects of solar line modification on planetary and interplanetary glow observations are discussed.

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