Published April 1975 | Version v1
Report Restricted

Measurement of the fluxes of galactic cosmic ray H-2 and He-3 in 1972--1973

Creators

Description

If a nearby source of low-energy helium is present, which has traversed a relatively small amount of matter and thus has not caused the production of a significant amount of H-2 or He-3, then these abundance ratios will be suppressed, particularly at low energies. This seems to be the most likely explanation for low ratios. (Author)

Availability note (English)

MF available from INIS under the Report Number.

Files

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Additional details

Publishing Information

Imprint Pagination
22 p.
Report number
N--75-25812

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
8288523
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
CHEMICAL COMPOSITION; COSMIC RADIATION; HELIUM; HYDROGEN; ISOTOPE RATIO
Descriptors DEC
ELEMENTS; IONIZING RADIATIONS; NONMETALS; RADIATIONS; RARE GASES

Optional Information

Notes
Submitted for Publication.. Available from NTIS. $3.25.
Secondary number(s)
NASA-TM-X--70901; X--661-75-100.