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COMPOSITION AND ENERGY SPECTRA OF COSMIC RAYS BETWEEN 0.6 AND 24 MEV PER NUCLEON DURING QUIET TIMES: TRANSITION FROM A SOLAR TO THE ANOMALOUS COMPONENT.

Author
KLECKER B; HOVESTADT D; GLOECKLER G; FAN CY
MAX-PLANCK-INST. PHYS. ASTROPHYS., 8046 GARCHING B. MUNICH, WEST GER.
Source
ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 212; NO 1 PART. 1; PP. 290-299; BIBL. 24 REF.
Document type
Article
Language
English
Keyword (fr)
RAYONNEMENT COSMIQUE ABONDANCE ISOTOPIQUE SPECTRE ENERGIE SOLEIL CALME ORIGINE GEOPHYSIQUE EXTERNE
Keyword (en)
COSMIC RAYS ENERGY SPECTRUM QUIET SUN ORIGIN PROVENANCE EXTERNAL GEOPHYSICS
Keyword (es)
GEOFISICA EXTERNA
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E02 External geophysics

Discipline
External geophysics
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
PASCAL7730285612

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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