Expressions to determine temperatures and emission measures for solar X-ray events from GOES measurements
- 1 February 1985
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 95 (2) , 323-329
- https://doi.org/10.1007/bf00152409
Abstract
No abstract availableKeywords
This publication has 8 references indexed in Scilit:
- Radiation from a hot, thin plasma from 1 to 250 AThe Astrophysical Journal Supplement Series, 1976
- Dielectronic Satellite Spectra for Highly - Charged Helium - like Ions -- II IMPROVED CALCULATIONSMonthly Notices of the Royal Astronomical Society, 1975
- Relative coronal abundances derived from X-ray observations. III - The effect of cascades on the relative intensity of Fe XVII line fluxes, and a revised iron abundanceThe Astrophysical Journal, 1974
- Relative Coronal Abundances Derived from X-Ray Observations. IL Nitrogen, Oxygen, Neon, Magnesium, and IronThe Astrophysical Journal, 1974
- Relative Coronal Abundances Derived from X-Ray Observations. I. Sodium, Magnesium, Aluminum, Silicon, Sulfur, and ArgonThe Astrophysical Journal, 1974
- Radiation from a High-Temperature Low-Density Plasma: the X-Ray Spectrum of the Solar CoronaThe Astrophysical Journal, 1971
- Ionization Equilibria for High Ions of Fe and NiMonthly Notices of the Royal Astronomical Society, 1970
- The Ionization Equilibrium of Elements Between Carbon and NickelMonthly Notices of the Royal Astronomical Society, 1969