Cosmic Rays and the Magnetic Field of the Sun

Details Cosmic Rays and the Magnetic Field of the Sun Cosmic Rays and the Magnetic Field of the Sun

Mar 1950

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1950natur.165..353d&link_type=abstract

Nature, Volume 165, Issue 4192, pp. 353-354 (1950).

Computer Science

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Scientific paper

THE variation of the cosmic-ray intensity at sea-level with geomagnetic latitude shows a sharp change in slope in the region of 50°, the intensity remaining very nearly constant between this latitude and the pole. This latitude cut-off is present at a height of 30,000 ft.1 and, according to Cosyns2, still occurs at the same latitude at a pressure-level of 7 cm. mercury. Carmichael and Dymond's balloon flights3, when compared with those of Pfotzer, also indicate no increase in intensity between 50° N. and 88° N.

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