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High energy gamma ray results from the second small astronomy satellite
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Fichtel, C. E. Hartman, R. C. Oezel, M. F. Thompson, D. J. Tuemer, T. Kniffen, D. A. Bignami, G. F. Oegelman, H. |
| Copyright Year | 1974 |
| Description | A high energy (35 MeV) gamma ray telescope employing a thirty-two level magnetic core spark chamber system was flown on SAS 2. The high energy galactic gamma radiation is observed to dominate over the general diffuse radiation along the entire galactic plane, and when examined in detail, the longitudinal and latitudinal distribution seem generally correlated with galactic structural features, particularly with arm segments. The general high energy gamma radiation from the galactic plane, explained on the basis of its angular distribution and magnitude, probably results primarily from cosmic ray interactions with interstellar matter. |
| File Size | 1803264 |
| Page Count | 81 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19740027105 |
| Archival Resource Key | ark:/13960/t02z60r25 |
| Language | English |
| Publisher Date | 1974-10-01 |
| Access Restriction | Open |
| Subject Keyword | Space Radiation Gamma Rays Galactic Structure Sas Magnetic Cores Satellite Instruments Telescopes Spark Chambers Interstellar Matter Cosmic Rays Galactic Radiation Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |