Atmospheric effects on the cosmic ray intensity at a depth of 60 m.w.e. underground at London

Details Atmospheric effects on the cosmic ray intensity at a depth of 60 m.w.e. underground at London Atmospheric effects on the cosmic ray intensity at a depth of 60 m.w.e. underground at London

Mar 1965

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1965jatp...27..349d&link_type=abstract

Journal of Atmospheric and Terrestrial Physics, vol. 27, no. 3, pp. 349-358

Physics

2

Scientific paper

The effects of changes in atmospheric parameters on the meson intensity recorded by two semi-cubical telescopes located at an equivalent depth of 60 m of water below ground have been investigated by the method of correlation analysis. The cosmic ray intensity showed significant correlations with sea-level pressure and the upper air temperature (in the range 200-70 mb) but the negative temperature effect due to [mu]-e decay was too small to lead to significant correlation. The weighted average values of the two regression coefficients were as follows: "Total" Barometer Coefficient: -0·037 ± 0·002%/mb (-0·495 ± 0·026%/cmHg) Positive Temperature Coefficient: +0·041 ± 0·006%/°C These results are discussed in relation to earlier measurements and theoretical estimates.

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