Abundances and spectra for cosmic-ray nuclei from lithium to iron for 2 to 150 GeV per nucleon
Journal Article
·
· Astrophys. J.; (United States)
We report measurements of the absolute and relative abundances, differential energy spectra, and spectral indices for cosmic-ray nuclei from Li to Fe for 2--150 GeV per nucleon. These measurements were made using a balloon-borne superconducting magnetic spectrometer with scintillators and optical spark chambers. The abundances of Li, Be, and B for rigidities below 10 GV/c are consistent with an energy-independent mean interstellar pathlength of 41/2 +- 1/2 g cm/sup -2/ for the ''leaky-box'' propagation model. The abundances of all elements above 10 GV/c are consistent with an interstellar path length that decreases with rigidity as R/sup -n/ with an index n=0.6(+0.4, -0.3). All differential source spectra can be fitted by power laws in total energy per nucleon with the same spectral index, which is between 2.5 and 2.6 depending on n. If n is near 0.5 (as for simple diffusion), the source index is 2.54 +- 0.03. Relative abundances at the sources are thus independent of energy, and have ratios to solar abundances as a function of first ionization potential which indicate a source temperature between 10/sup 4/ and 5 x 10/sup 4/ K depending on the equilibrium nature of the injection environment.
- Research Organization:
- Spaces Sciences Laboratory and Lawrence Berkeley Laboratory, University of California, Berkeley
- OSTI ID:
- 6389184
- Journal Information:
- Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 226:3; ISSN ASJOA
- Country of Publication:
- United States
- Language:
- English
Similar Records
Abundances and Spectra for Cosmic-Ray Nuclei from Li to Fe For 2to 150 GeV/n
Abundances and energy spectra of cosmic ray iron and nickel at energies from 1 to 10 GeV PER amu
Isotopic composition of helium in the cosmic radiationabove 11 Gigavolts
Journal Article
·
Sun Mar 26 23:00:00 EST 1978
· Astrophysical Journal
·
OSTI ID:893057
Abundances and energy spectra of cosmic ray iron and nickel at energies from 1 to 10 GeV PER amu
Journal Article
·
Tue Sep 01 00:00:00 EDT 1981
· Astrophys. J.; (United States)
·
OSTI ID:5817248
Isotopic composition of helium in the cosmic radiationabove 11 Gigavolts
Journal Article
·
Sun Mar 31 23:00:00 EST 1985
· Astrophys. J.; (United States)
·
OSTI ID:5640797
Related Subjects
640101* -- Astrophysics & Cosmology-- Cosmic Radiation
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ABUNDANCE
CHEMICAL COMPOSITION
COSMIC NUCLEI
COSMIC RADIATION
ENERGY SPECTRA
FRAGMENTATION
GAS TRACK DETECTORS
INTERSTELLAR SPACE
IONIZING RADIATIONS
MEASURING INSTRUMENTS
NUCLEI
PRIMARY COSMIC RADIATION
RADIATION DETECTORS
RADIATIONS
SCINTILLATION COUNTERS
SPACE
SPARK CHAMBERS
SPECTRA
SPECTROMETERS
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ABUNDANCE
CHEMICAL COMPOSITION
COSMIC NUCLEI
COSMIC RADIATION
ENERGY SPECTRA
FRAGMENTATION
GAS TRACK DETECTORS
INTERSTELLAR SPACE
IONIZING RADIATIONS
MEASURING INSTRUMENTS
NUCLEI
PRIMARY COSMIC RADIATION
RADIATION DETECTORS
RADIATIONS
SCINTILLATION COUNTERS
SPACE
SPARK CHAMBERS
SPECTRA
SPECTROMETERS