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History of Geo- and Space Sciences An open-access journal
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Volume 5, issue 2
Hist. Geo Space. Sci., 5, 175-182, 2014
https://doi.org/10.5194/hgss-5-175-2014
© Author(s) 2014. This work is distributed under
the Creative Commons Attribution 3.0 License.
Hist. Geo Space. Sci., 5, 175-182, 2014
https://doi.org/10.5194/hgss-5-175-2014
© Author(s) 2014. This work is distributed under
the Creative Commons Attribution 3.0 License.

Short note 18 Dec 2014

Short note | 18 Dec 2014

Erich Regener and the ionisation maximum of the atmosphere

P. Carlson and A. A. Watson
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Cited articles
Alvarez, L. and Compton, A. H.: A Positively Charged Component of the Cosmic Rays, Phys. Rev., 43, 835–836, 1933.
Baade, W. and Zwicky, F.: Cosmic Rays from Super-Novae, P. Natl. Acad. USA, 20, 259–263, 1934.
Bethe, H. A., Kerr, D. M., and Jeffries, R. A.: Obituary H. W. Hoerlin, Phys. Today, 82–83, 1984.
Bhabha, H. J. and Heitler, W.: The Passage of fast Electrons and the Theory of Cosmic Showers, Proc. Roy. Soc. A, 159, 432–458, 1937.
Blackett, P. M. S.: Obituary: Erich Regener, Nature, 175, 1107–1108, 1959.
Publications Copernicus
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Short summary
In 1912 Hess found that the rate of production of ions in the atmosphere grows with altitude. In 1933 Regener observed a maximum rate of production above 20 km, a result later confirmed with his student, Pfotzer (Nature 1935). Final results were published in German by Pfotzer alone, probably because Regener had difficulties with the National Socialist government, and the maximum has become known as the Pfotzer maximum. An argument is made for renaming the maximum the Regener--Pfotzer maximum.
In 1912 Hess found that the rate of production of ions in the atmosphere grows with altitude. In...
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