skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Semi-cubical G.M. counter telescope system for underground registration of the meson intensity of the cosmic radiation

Abstract

A semicubical telescope system is described which was built for the registration of the high-energy-meson component of the cosmic radiation. A method elaborated to check the stability was applied to the data obtained during the period Mar. 1958 to Feb. 1959. (auth)

Authors:
; ;
Publication Date:
Research Org.:
Central Research Inst. of Physics, Budapest
Sponsoring Org.:
USDOE
OSTI Identifier:
4148374
NSA Number:
NSA-15-002842
Resource Type:
Journal Article
Journal Name:
Nuovo Cimento
Additional Journal Information:
Journal Volume: 16; Journal Issue: S2; Other Information: Orig. Receipt Date: 31-DEC-61; Journal ID: ISSN 0029-6341
Country of Publication:
Country unknown/Code not available
Language:
English
Subject:
ENGINEERING AND EQUIPMENT; COSMIC RADIATION; GEIGER-MUELLER COUNTERS; MESONS; OPTICAL SYSTEMS; TELESCOPES

Citation Formats

Sándor, T., Somogyi, A., and Telbisz, F. Semi-cubical G.M. counter telescope system for underground registration of the meson intensity of the cosmic radiation. Country unknown/Code not available: N. p., 1960. Web. doi:10.1007/BF02833799.
Sándor, T., Somogyi, A., & Telbisz, F. Semi-cubical G.M. counter telescope system for underground registration of the meson intensity of the cosmic radiation. Country unknown/Code not available. doi:10.1007/BF02833799.
Sándor, T., Somogyi, A., and Telbisz, F. Thu . "Semi-cubical G.M. counter telescope system for underground registration of the meson intensity of the cosmic radiation". Country unknown/Code not available. doi:10.1007/BF02833799.
@article{osti_4148374,
title = {Semi-cubical G.M. counter telescope system for underground registration of the meson intensity of the cosmic radiation},
author = {Sándor, T. and Somogyi, A. and Telbisz, F.},
abstractNote = {A semicubical telescope system is described which was built for the registration of the high-energy-meson component of the cosmic radiation. A method elaborated to check the stability was applied to the data obtained during the period Mar. 1958 to Feb. 1959. (auth)},
doi = {10.1007/BF02833799},
journal = {Nuovo Cimento},
issn = {0029-6341},
number = S2,
volume = 16,
place = {Country unknown/Code not available},
year = {1960},
month = {9}
}