On the Flux of Low-Energy Particles in the Solar System During the Last 10 Million Years View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

1969

AUTHORS

B. S. Amin , D. Lal , J. C. Lorin , P. Pellas , R. S. Rajan , A. S. Tamhane , V. S. Venkatavaradan

ABSTRACT

The work presented here provides, for the first time, conclusive evidence for the presence of an appreciable flux of low-energy particles (10Saint-Séverin, was carried out in two successive stages: regions of least ablation are pin-pointed by measurements of the density of cosmic-ray fossil tracks made visible by chemical etching of hypersthene and oligoclase crystals; and results of non-destructive analyses for total Al26 + Na22, as well as for Al26 and Na22 separately in two samples are presented. The data on the observed depth variation of these nuclides are discussed in relation to the expected production rates for the case of present-day galactic cosmic radiation, as seen at distances of 1 AU from sun and for the case of ‘low-energy’ cosmic radiation accelerated by the sun during solar cycle 19.The implications of this study to the flux of low-energy cosmic radiation in the solar system during prehistoric era, and its origin (which is closely linked to the orbit of Saint-Séverin) are discussed. More... »

PAGES

316-327

Book

TITLE

Meteorite Research

ISBN

978-94-010-3413-5
978-94-010-3411-1

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-94-010-3411-1_26

DOI

http://dx.doi.org/10.1007/978-94-010-3411-1_26

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1037744113


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