Published 1985
| Version v1
Report
Solar photospheric and coronal abundances from solar energetic particle measurements. Ph.D. Thesis
Description
Observations of solar energetic particles (SEP) from 22 solar flares in the 1977 to 1982 time period are reported. SEP abundances were obtained for all elements with 3 approximately less than Z approximately less than 30 except Li, Be, B, F, Sc, v, Co and Cu for which upper limits were obtained. Statistically meaningful abundances of several rare elements (P, Cl, K, Ti, and Mn) were determined for the first time, and the average abundance of the more abundant elements were determined with improved precision
Availability note (English)
Available from NTIS, PC A09/MF A01.Additional details
Publishing Information
- Imprint Pagination
- 177 p.
- Report number
- NASA-CR--176029
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 19020254
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ASTROPHYSICS; CHEMICAL COMPOSITION; HEAVY IONS; PHOTOSPHERE; SOLAR ATMOSPHERE; SOLAR CORONA; SOLAR FLARES; SOLAR PARTICLES; SOLAR WIND
- Descriptors DEC
- ATMOSPHERES; CHARGED PARTICLES; IONS; RADIATIONS; SOLAR ACTIVITY; SOLAR RADIATION; STELLAR ACTIVITY; STELLAR ATMOSPHERES; STELLAR CORONAE; STELLAR FLARES; STELLAR RADIATION; STELLAR WINDS
Optional Information
- Notes
- Thesis (Ph.D.).