Relative coronal abundances derived from x-ray observations. III. The effect of cascades on the relative intensity of Fe xcii line fluxes, and a revised iron abundance
Journal Article
·
· Astrophys. J., v. 194, no. 2, pp. 471-482
OSTI ID:4211326
- Research Organization:
- Institute for Plasma Research, and Department of Applied Physics, Stanford University
- NSA Number:
- NSA-31-023673
- OSTI ID:
- 4211326
- Journal Information:
- Astrophys. J., v. 194, no. 2, pp. 471-482, Other Information: Orig. Receipt Date: 30-JUN-75
- Country of Publication:
- United States
- Language:
- English
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OSTI ID:4211326