Published August 1985
| Version v1
Report
SMM detection of interstellar Al-26 gamma radiation
- 1. New Hampshire Univ., Garching, West Germany
Description
The gamma ray spectrometer on the Solar Maximum Mission Satellite has detected the interstellar Al-26 line when the Galactic center traversed its aperture. The center of the emission is consistent with the location of the Galactic center, but the spatial distribution is presently not well defined. The total flux in the direction of the Galactic center is 4.3 + or - 0.4) x .0001 gamma/sq cm-s-rad for an assumed population I distribution
Additional details
Publishing Information
- Imprint Title
- Ninteenth International Cosmic Ray Conference. OG sessions, volume 1
- Journal Page Range
- vp.
- Report number
- NASA-CP--2376-VOL-1
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 17080593
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Non-conventional Literature
- Descriptors DEI
- ALUMINIUM 26; COSMIC RADIATION; FLUX DENSITY; GALAXY NUCLEI; GAMMA RADIATION; MAGNETIC RIGIDITY; SOLAR FLARES; SPATIAL DISTRIBUTION
- Descriptors DEC
- ALUMINIUM ISOTOPES; BETA DECAY RADIOISOTOPES; BETA-PLUS DECAY RADIOISOTOPES; DISTRIBUTION; ELECTROMAGNETIC RADIATION; IONIZING RADIATIONS; ISOTOPES; LIGHT NUCLEI; NUCLEI; ODD-ODD NUCLEI; RADIATIONS; RADIOISOTOPES; SECONDS LIVING RADIOISOTOPES; SOLAR ACTIVITY; STELLAR ACTIVITY; STELLAR FLARES; YEARS LIVING RADIOISOTOPES