Semiempirical rates of formation of cosmic ray tracks in spherical objects exposed in space: Preatmospheric and postatmospheric depth profiles-Reference-Cited by-同舟云学术

Semiempirical rates of formation of cosmic ray tracks in spherical objects exposed in space: Preatmospheric and postatmospheric depth profiles

Published:1973-12-01 Issue:34 Volume:78 Page:8356-8363
ISSN:0148-0227
Container-title:Journal of Geophysical Research
language:en
Short-container-title:J. Geophys. Res.

Author:

Bhattacharya S. K.,Goswami J. N.,Lal D.

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Link

http://www.agu.org/journals/ja/v078/i034/JA078i034p08356/JA078i034p08356.pdf

Reference24 articles.

1. Solar flares, the lunar surface, and gas-rich meteorites;Barber;Geochim. Cosmochim. Acta,1971

2. High resolution time averaged (millions of years) energy spectrum and chemical composition of iron-group cosmic ray nuclei at 1 AU based on fossil tracks in Apollo samples;Bhandari;Geochim. Cosmochim. Acta,1971

3. Collision controlled radiation history of the lunar regolith;Bhandari;Geochim. Cosmochim. Acta,1972

4. Kinetic energy spectra of 5-1500 Mev/n VH nuclei- Long term averaged flux at 1-3 AU;Bhandari;Proc. Int. Conf. Cosmic Rays 13th,1973

5. Surface irradiation and evolution of the lunar regolith;Bhandari;Geochim. Cosmochim. Acta,1973

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