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James Van Allen journal, 1951?-December 1954
Page 67
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Number of primaries through sphere of unit cross-section at top of atmosphere (2 pi)(0.045) = 0.283 / (cm exponent 2) second (pi)(r exponent 2) = 1 r = (square root of (1/pi)) Volume = ((4/3) (pi) (r exponent 3)) = (0.755 (cm exponent 3)) ------------------------------------------------------------------------ Number of stars expected at top of atmosphere = 0.283/28 = (2(pi)j)/lambda = (0.0101 / (cm exponent 3) second) observed: 0.00256 / ((cm exponent 3) second) therefore, observed / expected = 0.25 -------------------------------------------------------------- Some good books to own: J. H. Jeans "The Dynamical Theory of Gases" Cambridge 4th Edition (1925) ----------------------------------------------------------------- L. [I? J?]. Schiff "Quantum Mechanics" MacGraw Hill Book Company, New Jersey, 1st Edition (1949) --------------------------------------------------------------- E. H. Kennard "Kinetic Theory of Gases" McGraw Hill (1938)
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Number of primaries through sphere of unit cross-section at top of atmosphere (2 pi)(0.045) = 0.283 / (cm exponent 2) second (pi)(r exponent 2) = 1 r = (square root of (1/pi)) Volume = ((4/3) (pi) (r exponent 3)) = (0.755 (cm exponent 3)) ------------------------------------------------------------------------ Number of stars expected at top of atmosphere = 0.283/28 = (2(pi)j)/lambda = (0.0101 / (cm exponent 3) second) observed: 0.00256 / ((cm exponent 3) second) therefore, observed / expected = 0.25 -------------------------------------------------------------- Some good books to own: J. H. Jeans "The Dynamical Theory of Gases" Cambridge 4th Edition (1925) ----------------------------------------------------------------- L. [I? J?]. Schiff "Quantum Mechanics" MacGraw Hill Book Company, New Jersey, 1st Edition (1949) --------------------------------------------------------------- E. H. Kennard "Kinetic Theory of Gases" McGraw Hill (1938)
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