Terrestrial Accretion from the Solar Wind

Details Terrestrial Accretion from the Solar Wind Terrestrial Accretion from the Solar Wind

Sep 1961

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1961natur.191.1182h&link_type=abstract

Nature, Volume 191, Issue 4794, pp. 1182-1183 (1961).

Physics

Scientific paper

DE TURVILLE1 has suggested that the Earth is gaining hydrogen
from the Sun at the rate of 1.5 tons a second, and points out that this
rate of accretion will account for all the hydrogen in the oceans in the
course of 3 × 109 years. His idea is that the
geomagnetic field captures the protons of an incident solar wind.

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