Absorption mean free path of the nucleonic component of cosmic radiation
The absorption mean free path L of star-producing radiation was determined by means of the local production of neutrons in condensed materials; for that purpose a neutron monitor was installed in an aircraft, and two flights were performed at the geomagnetic latitudes 23.3°S (Buenos Aires, Repúblic...
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todo:paper_0031899X_v124_n4_p1201_Cicchini2023-10-03T14:41:56Z Absorption mean free path of the nucleonic component of cosmic radiation Cicchini, A. Chagalj, J. The absorption mean free path L of star-producing radiation was determined by means of the local production of neutrons in condensed materials; for that purpose a neutron monitor was installed in an aircraft, and two flights were performed at the geomagnetic latitudes 23.3°S (Buenos Aires, República Argentina) and 15°S (Asunción, República del Paraguay). The results show an increase in L of about 20% for an altitude increase of 6000 m in Buenos Aires, and of 40% in Asunción, for the same altitude increase; the total L value in Asunción was found to be 175 g cm-2, while in Buenos Aires it was 163 g cm-2, that is, approximately 8% lower. © 1961 The American Physical Society. Fil:Cicchini, A. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_0031899X_v124_n4_p1201_Cicchini |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
description |
The absorption mean free path L of star-producing radiation was determined by means of the local production of neutrons in condensed materials; for that purpose a neutron monitor was installed in an aircraft, and two flights were performed at the geomagnetic latitudes 23.3°S (Buenos Aires, República Argentina) and 15°S (Asunción, República del Paraguay). The results show an increase in L of about 20% for an altitude increase of 6000 m in Buenos Aires, and of 40% in Asunción, for the same altitude increase; the total L value in Asunción was found to be 175 g cm-2, while in Buenos Aires it was 163 g cm-2, that is, approximately 8% lower. © 1961 The American Physical Society. |
format |
JOUR |
author |
Cicchini, A. Chagalj, J. |
spellingShingle |
Cicchini, A. Chagalj, J. Absorption mean free path of the nucleonic component of cosmic radiation |
author_facet |
Cicchini, A. Chagalj, J. |
author_sort |
Cicchini, A. |
title |
Absorption mean free path of the nucleonic component of cosmic radiation |
title_short |
Absorption mean free path of the nucleonic component of cosmic radiation |
title_full |
Absorption mean free path of the nucleonic component of cosmic radiation |
title_fullStr |
Absorption mean free path of the nucleonic component of cosmic radiation |
title_full_unstemmed |
Absorption mean free path of the nucleonic component of cosmic radiation |
title_sort |
absorption mean free path of the nucleonic component of cosmic radiation |
url |
http://hdl.handle.net/20.500.12110/paper_0031899X_v124_n4_p1201_Cicchini |
work_keys_str_mv |
AT cicchinia absorptionmeanfreepathofthenucleoniccomponentofcosmicradiation AT chagaljj absorptionmeanfreepathofthenucleoniccomponentofcosmicradiation |
_version_ |
1807316410641154048 |