Origin and Dynamical Behaviour of Thermal Protons in the Venusian Ionosphere
- 1 March 1970
- journal article
- Published by Springer Nature in Nature
- Vol. 225 (5236), 924-926
- https://doi.org/10.1038/225924a0
Abstract
An important source of thermal H(+) and/or D(+) has been overlooked in the ionosphere of Venus which supports the choice of H(+) and/or D(+) as the dominant light ion at high altitudes.Keywords
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