Solar Flare X-Ray Spectra between 7.8 and 23.0 Angstroms.
Abstract
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. (Author)
Document Details
- Document Type
- Technical Report
- Publication Date
- Apr 01, 1981
- Accession Number
- ADA098779
Entities
People
- D. L. Mckenzie
- H. R. Rugge
- P. B. Landecker
- R. M. Broussard
- R. M. Young
Organizations
- The Aerospace Corporation