NASA NTRS · 19720050961
The solar wind H and He/+/ content.
Abstract
Computation of the expected fluxes of He(+) ions and neutral H atoms in the solar wind. A simple model is used to compute the intensity of resonantly backscattered solar He II (304 A) and Lyman alpha radiation.
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Gregory, C. T.. 1972-06-01. The solar wind H and He/+/ content.. https://ntrs.nasa.gov/citations/19720050961
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