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Science 22 November 1968:
Vol. 162. no. 3856, pp. 891 - 895
DOI: 10.1126/science.162.3856.891
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Articles

X-Ray Line and Continuum Spectra of Solar Flares from 0.5 to 8.5 Angstroms

John F. Meekins 1, Robert W. Kreplin 1, Talbot A. Chubb 1, and Herbert Friedman 1

1 E. O. Hulburt Center for Space Research, Naval Research Laboratory, Washington, D.C. 20390

Two crystal spectrometers aboard the orbiting solar observatory OSO-4 cover the wavelength ranges 0.5 to 3.9 angstroms and 1.0 to 8.5 angstroms. Within this range, there appear emission lines from hydrogen-like and helium-like states of calcium, sulfur, silicon, magnesium, and aluminum. The Mg XII Lyman-agr is present strongly in all x-ray flares. The most intense flares (such as class 3) produce strong Si XIV Lyman-agr and often S XVI Lyman-agr. Emission, in the form of Ka lines of highly ionized states of calcium, iron, aluminum, and silicon is usually present. The continuum from 1 to 10 angstroms always dominates the line emission by more than an order of magnitude. Electron temperatures derived from the slope of the continuum spectrum are in the range of 107 to 108 °K, considerably higher than theoretical ionization equilibrium temperatures.


THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
X-ray Integrated Reflection Coefficient of Litium Fluoride.
F. W. Lytle (1969)
Science 165, 416
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Science. ISSN 0036-8075 (print), 1095-9203 (online)