THE MOMENTUM SPECTRUM OF COSMIC RAYS AT 3.4 KILOMETERS

Abstract

An experiment was conducted, by means of a cloud chamber in a magnetic field, to determine the momentum spectrum and to make some qualitative observations on the nucleonic component. No assumptions were made concerning the particles involved. The momentum spectrum of the nonelectronic ionizing component of cosmic radiation was obtained for the momenta of positive and negative particles between 100 Mev/c and 2.5 Bev/c. The radiation was filtered through 5 cm of lead. Results indicated that the ratio of particles of momentum greater than 2.5 Bev/c to those less than this value is equal to that found at sea level. For the range of momenta considered, the electron contribution extended to about 1 Bev/c. Enough protons were found at the lower momenta to account for the increase in the positive excess from sea level to 3.4 km. It was concluded that there are enough protons at slightly higher momenta to account completely for the positive excess. No evidence was obtained for the existence at 3.4 of a particle of 100 electron masses.

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Document Details

Document Type
Technical Report
Publication Date
Jan 01, 1953
Accession Number
AD0018442

Entities

People

  • A. W. Wotring
  • Catherine E. Miller
  • D. S. Potter
  • J. E. Henderson
  • Jane Todd

Organizations

  • University of Washington

Tags

Communities of Interest

  • Energy and Power Technologies

DTIC Thesaurus Topics

  • Altitude
  • Cloud Chambers
  • Control Systems
  • Cosmic Rays
  • Diagrams
  • Electronic Components
  • Energy
  • Geiger Counters
  • Ionization
  • Magnetic Fields
  • Measurement
  • Navy
  • New York
  • Particles
  • Physics Laboratories
  • Radiation
  • Sea Level

Fields of Study

  • Physics

Readers

  • Solar Physics

Technology Areas

  • Microelectronics