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James Van Allen journal, 1951?-December 1954
Page 31
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Regener, Nature 131, page 130 (1933) Total energy integrals -----> ((2 x (10 exponent 11)) ev)/((cm exponent 2) minutes) at high latitudes --------------------------------------------------------------------- Stormer Zeitschr of Astr. Phys. 1, page 237 (1930) -------------------------------------------------------------------- "The Cut-Off in the Energy Spectrum of Primary Cosmic Radiation". Philosophical Magazine 41, page 495 (1950) P. J. D. Gething Department of Math Department of Science Imperial College London e = proton charge M = Jun's [moment? movement?] d = distance of earth to sun (P sub 1) = ((3 - (2 (square root of 2)))(e)(M))/(d exponent 2) (P sub 2) = (((e)(M))/(d exponent 2)) Momentum below which none reach earth's orbit Between (P sub 1) and (P sub 2) some are able to reach the earth from certain directions only if earth in equatorial plane of sun's field
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Regener, Nature 131, page 130 (1933) Total energy integrals -----> ((2 x (10 exponent 11)) ev)/((cm exponent 2) minutes) at high latitudes --------------------------------------------------------------------- Stormer Zeitschr of Astr. Phys. 1, page 237 (1930) -------------------------------------------------------------------- "The Cut-Off in the Energy Spectrum of Primary Cosmic Radiation". Philosophical Magazine 41, page 495 (1950) P. J. D. Gething Department of Math Department of Science Imperial College London e = proton charge M = Jun's [moment? movement?] d = distance of earth to sun (P sub 1) = ((3 - (2 (square root of 2)))(e)(M))/(d exponent 2) (P sub 2) = (((e)(M))/(d exponent 2)) Momentum below which none reach earth's orbit Between (P sub 1) and (P sub 2) some are able to reach the earth from certain directions only if earth in equatorial plane of sun's field
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