Hostname: page-component-8448b6f56d-c4f8m Total loading time: 0 Render date: 2024-04-23T23:47:24.424Z Has data issue: false hasContentIssue false
  • English
  • Français

Thermal and Non-Thermal Soft X-Ray Bursts

Published online by Cambridge University Press:  12 April 2016

M. Landini ,
B. C. Monsignori Fossi  and
R. Pallavicini
M. Landini
Affiliation:
Osservatorio Astrofisico di Arcetri, Firenze, Italy
B. C. Monsignori Fossi
Affiliation:
Osservatorio Astrofisico di Arcetri, Firenze, Italy
R. Pallavicini
Affiliation:
Osservatorio Astrofisico di Arcetri, Firenze, Italy

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Soft X-ray enhancements of solar radiation are on many occasions recorded by Solrad 9 which is instrumented with several photometers sensitive to X-ray emission in the range 2–25 keV. A non-thermal interpretation of X-ray bursts for energy larger than 10–20 keV is usually given in the literature, while for the soft X-ray region below 10 keV the common interpretation is a thermal one.

Type
Section V / The Solar Flare Plasma
Information
International Astronomical Union Colloquium , Volume 14: Special Issue: Ultraviolet and X-Ray Spectroscopy of Astrophysical and Laboratory Plasmas , November 1972 , pp. 825 - 826
Copyright
Copyright © Reidel 1972