The Portales Valley meteorite fell as a large shower on 13 June 1998. About 50 specimens have been recovered. These various fragments located at different depth within the meteoroid provide an opportunity to study cosmogenic effects also as a function of shielding. Portales Valley was classified as a H6 ordinary chondrite. It consists of large silicate-rich regions crosscut by unusual thick veins of metallic Fe-Ni. We measured the gamma-activity and the nuclear tracks in a fragment weighing about 600 g. Twelve cosmogenic radioisotopes were revealed with high accuracy of counting. Measurements in other fragments are in progress. Cosmogenic 22Na (T1/2 = 2.6 y) shows an exposure to GCR during the last years of low solar activity, similar to those measured in our Laboratory in other chondrites which fell in similar phase of the solar activity.

Cosmic ray effects in the fresh-fall Portales Valley

CINI, Giuliana;BONINO, Giuseppe;TARICCO, Carla;
1999-01-01

Abstract

The Portales Valley meteorite fell as a large shower on 13 June 1998. About 50 specimens have been recovered. These various fragments located at different depth within the meteoroid provide an opportunity to study cosmogenic effects also as a function of shielding. Portales Valley was classified as a H6 ordinary chondrite. It consists of large silicate-rich regions crosscut by unusual thick veins of metallic Fe-Ni. We measured the gamma-activity and the nuclear tracks in a fragment weighing about 600 g. Twelve cosmogenic radioisotopes were revealed with high accuracy of counting. Measurements in other fragments are in progress. Cosmogenic 22Na (T1/2 = 2.6 y) shows an exposure to GCR during the last years of low solar activity, similar to those measured in our Laboratory in other chondrites which fell in similar phase of the solar activity.
1999
26th ICRC-International Cosmic Ray Conference
Salt Lake City, Utah, USA
August 17-25, 1999
Proceedings of ICRC
-
7
346
-
http://adsabs.harvard.edu/full/1999ICRC....7..346B
Meteorites; cosmogenic radioisotopes; cosmic rays
Cini Castagnoli G.; Bonino G.; Bhandari N.; Taricco C.; Killgore M.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2318/122947
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