Published October 1985
| Version v1
Journal article
Improved excitation rate coefficients for the n = 2 and n = 3 levels of Ca XIX and Fe XXV including fine structure
Description
Reently calculated collision strengths, including relativistic and resonance effects, are employed to compute Maxwellian averaged collision strengths for 78 transitions involving states of principal quantum numbers 2-1 and 3-1 in Ca XIX and Fe XXV. These rate parameters are tabulated at temperatures of interest in astrophysical and labortory plasmas with radiation in the hard X-ray wavelength range. For some transitions, significant differences are found with the earlier calculations of Pradhan, Norcross, and Hummer (1981). 10 references
Additional details
Publishing Information
- Journal Title
- Astrophys. J., Suppl. Ser.
- Journal Volume
- 59
- Series
- Astrophys. J., Suppl. Ser.
- Journal Page Range
- 183-195
- ISSN
- 0067-0049
- CODEN
- APJSA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 17079650
- Subject category
- S74: ATOMIC AND MOLECULAR PHYSICS;
- Descriptors DEI
- CALCIUM IONS; FINE STRUCTURE; HARD X RADIATION; IRON; IRON IONS; OSCILLATOR STRENGTHS; X-RAY SPECTRA
- Descriptors DEC
- ATOMIC IONS; CHARGED PARTICLES; ELECTROMAGNETIC RADIATION; ELEMENTS; IONIZING RADIATIONS; IONS; METALS; RADIATIONS; SPECTRA; TRANSITION ELEMENTS; X RADIATION