The composition of cosmic rays at high energies

Advances in Space Research

Volumn 9, Issue 12, 1989, Pages 31-43

  Müller, Dietrich ^a  

^a UNIVERSITY OF CHICAGO   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 33947508175     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/0273-1177(89)90306-2     Document Type: Article

References (47)

1. Tracks of heavy primary cosmic rays in meteorites
2. The Charge Spectrum of Very Heavy Cosmic Ray Nuclei
3. Charge Composition and Energy Spectrum of Primary Cosmic-Ray Electrons
4. The age of the galactic cosmic rays derived from the abundance of Be-10
5. A cosmic-ray age based on the abundance of Be-10
6. The energy spectrum of electrons and cosmic-ray confinement A new measurement and its interpretation
7. Energy spectra of cosmic-ray nuclei to above 100 GeV per nucleon
8. Cosmic-ray energy spectra between 10 and several hundred GeV per atomic mass unit for elements from Ar-18 to Ni-28 - Results from HEAO 3
9. Energy spectra of cosmic-ray nuclei from 50 to 2000 GeV per AMU
10. Charge composition and energy spectra of cosmic-ray nuclei at energies above 5 GeV per nucleon
11. Charge Composition and Energy Spectra of Cosmic-Ray Nuclei at Energies above 20 GeV Per Nucleon
12. Abundances and spectra for cosmic-ray nuclei from lithium to iron for 2 to 150 GeV per nucleon
13. The energy spectrum of cosmic ray electrons between 9 and 300 GeV
14. A measurement of the absolute flux of cosmic-ray electrons
15. Cosmic-ray positrons from 10 to 20 GeV - A balloon-borne measurement using the geomagnetic east-west asymmetry
16. Measurement of primary cosmic-ray electrons and positrons from 4 to 50 GeV
17. A measurement of cosmic-ray positron and negatron spectra between 50 and 800 MV
18. On the nature of the cosmic ray positron spectrum
19. The isotopes of neon in the galactic cosmic rays
20. High resolution measurements of galactic cosmic-ray neon, magnesium, and silicon isotopes
21. Astromag