Solar line profiles of He I 584 A and He II 304 A

Author:

Cushman G. W.,Farwell L.,Godden G.,Rense W. A.

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference11 articles.

1. The solar spectrum: Wavelengths and identifications from 60 to 385 angstroms;Behring;Astrophys. J.,1972

2. Pioneer 10 ultraviolet photometer observations at Jupiter encounter;Carlson;J. Geophys. Res.,1974

3. An observation of the helium I 584-A dayglow radiations between 400 and 1000 km;Donahue;J. Geophys. Res.,1971

4. Donnelly , R. F. J. H. Pope The 1-3000 A solar flux for a moderate level of solar activity for use in modeling the ionosphere and upper atmosphere Boulder, Colo. 1973

5. The widths of the solar HeI and HeII lines at 584, 537, and 304A;Doschek;Astrophys. J.,1974

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