Accretion Rate of Cosmic Dust estimated from Cosmogenic Aluminium-26

Details Accretion Rate of Cosmic Dust estimated from Cosmogenic Aluminium-26 Accretion Rate of Cosmic Dust estimated from Cosmogenic Aluminium-26

Dec 1968

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1968natur.220.1016y&link_type=abstract

Nature, Volume 220, Issue 5171, pp. 1016-1017 (1968).

Physics

1

Scientific paper

A GOOD criterion for recognizing particles of cosmic dust on the Earth
is the detection of radionuclides such as aluminium-26, formed by the
action of cosmic rays on dust in free space1,2. Terrestrial
dust is protected by the atmosphere.

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