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Cosmic ray zenith angle distribution at low geomagnetic latitude

Journal Article:

Abstract

The intensity of secondary charged cosmic rays at different zenith angles was measured by narrow angle Geiger-Mueller telescopes up to an atmospheric depth of 2 g cm/sup -2/. The angular distribution observed at high altitudes is nearly flat at small angles around the vertical and suggests that the particle intensity peaks at large zenith angles, close to the horizon.
Authors:
Aragon, G; [1]  Gagliardini, A; Ghielmetti, H S
  1. Instituto de Astronomia y Fisica del Espacio, Buenos Aires, Argentina
Publication Date:
Dec 01, 1977
Product Type:
Journal Article
Reference Number:
AIX-10-458524; EDB-80-024942
Resource Relation:
Journal Name: SBARMO Bull.; (France); Journal Volume: 6:4
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; SECONDARY COSMIC RADIATION; ANGULAR DISTRIBUTION; COSMIC RAY DETECTION; GEOMAGNETIC EQUATOR; COSMIC RADIATION; DETECTION; DISTRIBUTION; IONIZING RADIATIONS; RADIATION DETECTION; RADIATIONS; 640101* - Astrophysics & Cosmology- Cosmic Radiation
OSTI ID:
5792532
Country of Origin:
France
Language:
English
Other Identifying Numbers:
Journal ID: CODEN: SBBUD
Submitting Site:
INIS
Size:
Pages: 243-261
Announcement Date:

Journal Article:

Citation Formats

Aragon, G, Gagliardini, A, and Ghielmetti, H S. Cosmic ray zenith angle distribution at low geomagnetic latitude. France: N. p., 1977. Web.
Aragon, G, Gagliardini, A, & Ghielmetti, H S. Cosmic ray zenith angle distribution at low geomagnetic latitude. France.
Aragon, G, Gagliardini, A, and Ghielmetti, H S. 1977. "Cosmic ray zenith angle distribution at low geomagnetic latitude." France.
@misc{etde_5792532,
title = {Cosmic ray zenith angle distribution at low geomagnetic latitude}
author = {Aragon, G, Gagliardini, A, and Ghielmetti, H S}
abstractNote = {The intensity of secondary charged cosmic rays at different zenith angles was measured by narrow angle Geiger-Mueller telescopes up to an atmospheric depth of 2 g cm/sup -2/. The angular distribution observed at high altitudes is nearly flat at small angles around the vertical and suggests that the particle intensity peaks at large zenith angles, close to the horizon.}
journal = {SBARMO Bull.; (France)}
volume = {6:4}
journal type = {AC}
place = {France}
year = {1977}
month = {Dec}
}