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

Creators

  • 1. Joint Institute for Lab. Astrophysics, Boulder, CO

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