Solar flare irradiation records in Antarctic meteorites
The observation of tracks from solar flare heavy nuclei in Antarctic meteorite samples is reported. In an analysis of nuclear track densities in eight L and H chondrites of low metamorphic grade, it was found that two interior specimens of sample 77216, an L-3 chondrite, contain olivine grains with...
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ftnasantrs:oai:casi.ntrs.nasa.gov:19810063258 2023-05-15T13:46:48+02:00 Solar flare irradiation records in Antarctic meteorites Goswami, J. N. Unclassified, Unlimited, Publicly available Sep 10, 1981 http://ntrs.nasa.gov/search.jsp?R=19810063258 unknown http://ntrs.nasa.gov/search.jsp?R=19810063258 Accession ID: 81A47662 Copyright Other Sources 91 Nature; 293; Sept. 10 1981 ftnasantrs 2012-02-15T14:43:49Z The observation of tracks from solar flare heavy nuclei in Antarctic meteorite samples is reported. In an analysis of nuclear track densities in eight L and H chondrites of low metamorphic grade, it was found that two interior specimens of sample 77216, an L-3 chondrite, contain olivine grains with track densities much higher than the average track densities, indicating precompaction irradiation by solar flares in different shielding conditions. Preliminary data from mass spectroscopic analyses show a large excess of noble gases, with a Ne-20/Ne-22 ratio of greater than or equal to 10, indicating the presence of solar-type noble gas. Results of track density measurements in the other Antarctic meteorites range from 10,000 to 4,000,000/sq cm, which is within the range observed in non-Antarctic L-group meteorites Other/Unknown Material Antarc* Antarctic NASA Technical Reports Server (NTRS) Antarctic |
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Open Polar |
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NASA Technical Reports Server (NTRS) |
op_collection_id |
ftnasantrs |
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unknown |
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91 |
spellingShingle |
91 Goswami, J. N. Solar flare irradiation records in Antarctic meteorites |
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91 |
description |
The observation of tracks from solar flare heavy nuclei in Antarctic meteorite samples is reported. In an analysis of nuclear track densities in eight L and H chondrites of low metamorphic grade, it was found that two interior specimens of sample 77216, an L-3 chondrite, contain olivine grains with track densities much higher than the average track densities, indicating precompaction irradiation by solar flares in different shielding conditions. Preliminary data from mass spectroscopic analyses show a large excess of noble gases, with a Ne-20/Ne-22 ratio of greater than or equal to 10, indicating the presence of solar-type noble gas. Results of track density measurements in the other Antarctic meteorites range from 10,000 to 4,000,000/sq cm, which is within the range observed in non-Antarctic L-group meteorites |
format |
Other/Unknown Material |
author |
Goswami, J. N. |
author_facet |
Goswami, J. N. |
author_sort |
Goswami, J. N. |
title |
Solar flare irradiation records in Antarctic meteorites |
title_short |
Solar flare irradiation records in Antarctic meteorites |
title_full |
Solar flare irradiation records in Antarctic meteorites |
title_fullStr |
Solar flare irradiation records in Antarctic meteorites |
title_full_unstemmed |
Solar flare irradiation records in Antarctic meteorites |
title_sort |
solar flare irradiation records in antarctic meteorites |
publishDate |
1981 |
url |
http://ntrs.nasa.gov/search.jsp?R=19810063258 |
op_coverage |
Unclassified, Unlimited, Publicly available |
geographic |
Antarctic |
geographic_facet |
Antarctic |
genre |
Antarc* Antarctic |
genre_facet |
Antarc* Antarctic |
op_source |
Other Sources |
op_relation |
http://ntrs.nasa.gov/search.jsp?R=19810063258 Accession ID: 81A47662 |
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Copyright |
_version_ |
1766245228051693568 |