Solar flare x-ray spectra between 7. 8 and 23. 0 angstroms. Technical report
Technical Report
·
OSTI ID:5757358
We present high resolution x-ray spectra taken during a large solar flare on 10 June 1979. Many lines of highly ionized iron are resolved and identified for the first time in solar spectra. Lines with a wide range of excitation temperatures are found to have a similar time development during the flare's rapid rise phase. We discuss density-sensitive line ratios in Fe XXI and Fe XXII.
- Research Organization:
- Aerospace Corp., El Segundo, CA (USA). Space Sciences Lab.
- OSTI ID:
- 5757358
- Report Number(s):
- AD-A-098779/2
- Country of Publication:
- United States
- Language:
- English
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