ISOTOPIC COMPOSITION OF THE LO ENERGY HELIUM NUCLEI IN THE PRIMARY COSMIC RADIATION
Journal Article
·
· Physical Review (U.S.) Superseded in part by Phys. Rev. A, Phys. Rev. B: Solid State, Phys. Rev. C, and Phys. Rev. D
The isotopic composition of low-energy helium nuclei in the primary cosmic radiation is determined by using the "constant sagitta" scattering method on tracks of helium nuclei stopping in a nuclear-emulsion stack flown at a geomagnetic latitude of 55 deg N and at a mean atmospheric depth of 8.5 g/cm/sup 2/; tracks with zenith angles less than 30 deg are accepted. The ratio of He/ sup 3//(He/sup 3/ + He4) for the same energy per nucleon (between 200 and 400 Mev) is found to be 0.41 plus or minus 0.09 at flight altitude. The correction for production of secondary He/sup 3/ in the residual atmosphere is calculated to be 4%. If one assumes that no He/sup 3/ nuclei are present at the source, the observed ratio corresponds to a traversal of 14 plus or minus 3 g of interstellar matter by the lowenergy helium nuclei. The value of He/sup 3//(He/ sup 3/ + He/sup 4/) corresponding to the same magnetic rigidity (between 1.3 and 1.6 Bv) is found to be 0.36 plus or minus 0.11 which corresponds to a traversal of 12.2 plus or minus 3.5 g of interstellar matter. The observed ratio may indicate the presence of He/sup 3/ at the source of cosmic rays, or may be a reflection of local production within the solar system. (auth)
- Research Organization:
- Univ. of Rochester, N.Y.
- NSA Number:
- NSA-15-024198
- OSTI ID:
- 4029703
- Report Number(s):
- NYO-9553; 0031-899X
- Journal Information:
- Physical Review (U.S.) Superseded in part by Phys. Rev. A, Phys. Rev. B: Solid State, Phys. Rev. C, and Phys. Rev. D, Journal Name: Physical Review (U.S.) Superseded in part by Phys. Rev. A, Phys. Rev. B: Solid State, Phys. Rev. C, and Phys. Rev. D Vol. Vol: 123; ISSN PHRVA
- Country of Publication:
- Country unknown/Code not available
- Language:
- English
Similar Records
He$sup 3$ NUCLEI IN THE PRIMARY COSMIC RADIATION
Isotopic composition of cosmic-ray helium from 123 279 MeV per nucleon: a new measurement and analysis
The He 3 /(He 3 +He 4 ) ratio in primary cosmic radiation
Journal Article
·
Mon Dec 31 23:00:00 EST 1962
· Nuovo Cimento (Italy) Divided into Nuovo Cimento A and Nuovo Cimento B
·
OSTI ID:4752736
Isotopic composition of cosmic-ray helium from 123 279 MeV per nucleon: a new measurement and analysis
Journal Article
·
Mon May 01 00:00:00 EDT 1978
· Astrophys. J.; (United States)
·
OSTI ID:6816111
The He 3 /(He 3 +He 4 ) ratio in primary cosmic radiation
Journal Article
·
Sat Mar 31 23:00:00 EST 1962
· Journal of Geophysical Research
·
OSTI ID:4819508
Related Subjects
ANGULAR DISTRIBUTION
BALLOONS
COSMIC RADIATION
EARTH
ENERGY RANGE
FISSION
GEOMAGNETIC COORDINATES
HELIUM 3
HELIUM 4
HELIUM ISOTOPES
HYDROGEN
INTERACTIONS
LEVELS
MAGNETIC FIELDS
MEASURED VALUES
MOMENTUM
NUCLEAR EMULSIONS
NUCLEI
PARTICLE TRACKS
PHYSICS
PRIMARY COSMIC RADIATION
QUANTITY RATIO
RADIATION SOURCES
SCATTERING
SPACE
STARS
STRATOSPHERE
BALLOONS
COSMIC RADIATION
EARTH
ENERGY RANGE
FISSION
GEOMAGNETIC COORDINATES
HELIUM 3
HELIUM 4
HELIUM ISOTOPES
HYDROGEN
INTERACTIONS
LEVELS
MAGNETIC FIELDS
MEASURED VALUES
MOMENTUM
NUCLEAR EMULSIONS
NUCLEI
PARTICLE TRACKS
PHYSICS
PRIMARY COSMIC RADIATION
QUANTITY RATIO
RADIATION SOURCES
SCATTERING
SPACE
STARS
STRATOSPHERE