Published February 1975
| Version v1
Report
Kα x-rays from cosmic ray oxygen
Description
Equilibrium charge fractions are calculated for subrelativistic cosmic ray oxygen ions in the interstellar medium. These are used to determine the expected flux of Kα rays arising from atomic processes for a number of different postulated interstellar oxygen spectra. Relating these results to the diffuse x-ray background measured at the appropriate energy (i.e. approximately 0.6 keV) suggests an observable broadened line feature
Availability note (English)
MF available from INIS under the Report Number.Additional details
Publishing Information
- Imprint Pagination
- 24 p.
- Report number
- N--75-22250
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 8304787
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMIC RADIATION; COSMIC RAY FLUX; COSMOCHEMISTRY; ELECTRIC CHARGES; INTERSTELLAR SPACE; LINE BROADENING; OXYGEN IONS; SPATIAL DISTRIBUTION; SPECTRA; X RADIATION
- Descriptors DEC
- CHARGED PARTICLES; CHEMISTRY; DISTRIBUTION; ELECTROMAGNETIC RADIATION; IONIZING RADIATIONS; IONS; RADIATION FLUX; RADIATIONS; SPACE
Optional Information
- Notes
- Submitted for Publication. Available from NTIS. $3.25.
- Secondary number(s)
- NASA-TM-X--70870 X--661-75-39.