Sensitivity of the curve-of-growth technique utilized in rocket experiments to determine the line shape of solar He I resonance lines

Author:

Wu C. Y. Robert,Ogawa H. S.

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

Reference29 articles.

1. Aller, L. H., , The Atmosphere of the Sun and Stars, 322 Ronald, New York, 1963,

2. Solar line profiles of He I 584 Å and He II 304 Å;Cushman;J. Geophys. Res.,1975

3. The profile of the helium I 584 Å line from the sun;Delaboudiniere,1975

4. An observation of the helium I 584 Å dayglow radiation between 400 and 1000 km;Donahue;J. Geophys. Res.,1971

5. The widths of the solar He I and He II lines at 584, 537, and 304 Å;Doschek;Astrophys. J.,1974

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