A More Accurate and More Extended Cosmic-ray Ionization-Depth Curve, and the Present Evidence for Atom-Building
- 1 February 1931
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review B
- Vol. 37 (3) , 235-252
- https://doi.org/10.1103/PhysRev.37.235
Abstract
The cosmic-ray ionization-depth curve has been extended at both its upper and lower ends and made more accurate throughout. The absorption coefficients obtained directly from the slope of the curve run from per m. of water at the top (Pike's Peak) to at the bottom (80 m. or 262 ft. of water below the top of the atmosphere, thus bringing to light both softer and harder components than the authors had before found. Strong quantitative evidence is presented, on the basis of the Klein-Nishina formula, that the strongest and most absorbable cosmic-ray band arises from the act of formation of helium out of hydrogen. Striking qualitative evidence is found that the three more penetrating bands are due to the formation out of hydrogen of the only other abundant elements oxygen (C, N, O) silicon (Mg, Al, Si, S) and iron (Iron group). Two independent proofs are given that the cosmic-rays enter the earth's atmosphere as photons, namely, (1) they are quite uninfluenced by the earth's magnetic field, and (2) the ionization produced by them in a closed vessel does not increase continually in going to the top of the atmosphere but passes through a maximum. It is shown to follow that the cosmic rays, in coming from their place of origin to the earth have not passed through an amount of matter that is appreciable in comparison with the thickness of the earth's atmosphere and that they must therefore originate in interstellar space rather than in the atmospheres of the stars. Some participation of the nucleus in the absorption of cosmic-rays is brought to light.
Keywords
This publication has 13 references indexed in Scilit:
- On the Question of the Constancy of the Cosmic Radiation and the Relation of these Rays to MeteorologyPhysical Review B, 1930
- Scattering of Hard-RaysPhysical Review B, 1930
- Über die Prüfung der Streuungsformel von Klein und Nishina an kurzwelliger γ-StrahlungThe Science of Nature, 1930
- Das Wesen der HöhenstrahlungThe European Physical Journal A, 1929
- On the Composition of the Sun's AtmosphereThe Astrophysical Journal, 1929
- Messungen über das kurzwellige Ende der durchdringenden HöhenstrahlungThe Science of Nature, 1929
- Neue Untersuchungen über die durchdringende Hesssehe StrahlungThe European Physical Journal A, 1928
- High Altitude Tests on the Geographical, Directional, and Spectral Distribution of Cosmic RaysPhysical Review B, 1928
- Über die durchdringende Strahlung im MeeresniveauThe European Physical Journal A, 1927
- The isothermal layer of the atmosphere and atmospheric radiationProceedings of the Royal Society of London. Series A, Containing Papers of a Mathematical and Physical Character, 1909