Atmospheric effects on the underground muon intensity

Details Atmospheric effects on the underground muon intensity Atmospheric effects on the underground muon intensity

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..308f&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 308 (SEE N85-34991 23-93)

Physics

Atmospheric Effects, Atmospheric Pressure, Muons, Particle Telescopes, Atmospheric Attenuation, Correlation, Cosmic Rays, Temperature Effects

Scientific paper

It has previously been reported that the barometric pressure coefficient observed for muons at Poatina (vertical absorber depth 357 hg/sq cm) appears to be appreciably higher than would be expected from atmospheric absorption alone. There is a possibility that the effect is due to an upper atmospheric temperature effect arising from an inverse correlation of surface pressure with stratospheric temperature. A new proportional telescope is discussed which has been operating at Poatina since about the beginning of 83 and which has a long term stability suitable for studying variations of atmospheric origin.

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