Slow Mesons in Cosmic Radiation

S. V. Chandrashekhar Aiya and R. C. Saxena
Phys. Rev. 66, 183 – Published 1 October 1944
PDFExport Citation

Abstract

Using Bhabha's method, the intensity of slow mesons is determined. The intensity of mesons of energy greater than 108 ev and less than 2.7 × 108 ev is 6 percent of the total meson intensity. Near the geomagnetic equator, the total intensity increases by 54.4 percent, the meson intensity by 21.7 percent, and the electron intensity by 162.1 percent when the altitude increases from 3100 ft. to 7200 ft. The electron intensity, which is about 25 percent of the meson intensity at 3100 ft., increases to 50 percent of the meson intensity at 7200 ft.

  • Received 2 June 1944

DOI:https://doi.org/10.1103/PhysRev.66.183

©1944 American Physical Society

Authors & Affiliations

S. V. Chandrashekhar Aiya and R. C. Saxena

  • Cosmic-Ray Research Unit, Indian Institute of Science, Bangalore, India

References (Subscription Required)

Click to Expand
Issue

Vol. 66, Iss. 7-8 — October 1944

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review Journals Archive

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×