Diffusion of cosmic-ray nuclei in the atmosphere: Spectra and composition

Summary The diffusion equations of primary cosmic-ray nuclei in the atmosphere have been solved, assuming different shapes of the prmary energy spectra, and deriving a new simple analytical form of the solutions. Variations in the upper atmosphere of the spectra and charge ratios of the different gr...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Alessio, S. [verfasserIn] Dardo, M.

Format:	Artikel
Sprache:	Englisch

Erschienen:	1979

Schlagwörter:	Diffusion Equation Charge Ratio Fragmentation Parameter Primary Spectrum Primary Nucleus

Anmerkung:	© Societá Italiana di Fisica 1979

Übergeordnetes Werk:	Enthalten in: Il Nuovo Cimento C - Kluwer Academic Publishers, 1978, 2(1979), 4 vom: Juli, Seite 465-472
Übergeordnetes Werk:	volume:2 ; year:1979 ; number:4 ; month:07 ; pages:465-472

Links:	Volltext

DOI / URN:	10.1007/BF02558287

Katalog-ID:	OLC2055362887

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title	Diffusion of cosmic-ray nuclei in the atmosphere: Spectra and composition
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title_sort	diffusion of cosmic-ray nuclei in the atmosphere: spectra and composition
title_auth	Diffusion of cosmic-ray nuclei in the atmosphere: Spectra and composition
abstract	Summary The diffusion equations of primary cosmic-ray nuclei in the atmosphere have been solved, assuming different shapes of the prmary energy spectra, and deriving a new simple analytical form of the solutions. Variations in the upper atmosphere of the spectra and charge ratios of the different groups of nuclei are derived. © Societá Italiana di Fisica 1979
abstractGer	Summary The diffusion equations of primary cosmic-ray nuclei in the atmosphere have been solved, assuming different shapes of the prmary energy spectra, and deriving a new simple analytical form of the solutions. Variations in the upper atmosphere of the spectra and charge ratios of the different groups of nuclei are derived. © Societá Italiana di Fisica 1979
abstract_unstemmed	Summary The diffusion equations of primary cosmic-ray nuclei in the atmosphere have been solved, assuming different shapes of the prmary energy spectra, and deriving a new simple analytical form of the solutions. Variations in the upper atmosphere of the spectra and charge ratios of the different groups of nuclei are derived. © Societá Italiana di Fisica 1979
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up_date	2024-07-04T02:01:35.070Z
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Diffusion of cosmic-ray nuclei in the atmosphere: Spectra and composition

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