Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-26T20:28:45.733Z Has data issue: false hasContentIssue false
  • English
  • Français

Bragg spectroscopy from CORONAS-F

Published online by Cambridge University Press:  14 March 2005

J. Sylwester
J. Sylwester
Affiliation:
Space Research Centre, Polish Academy of Sciences, Wroclaw ul. Kopernika 11, Poland email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

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.

There are dozen instruments successfully operating aboard the solar satellite CORONAS-F, which was launched in the summer of 2001. Among them are two (Polish-led) Bragg crystal spectrometers – RESIK and Diogeness – recording solar flare and active region spectra. A short description of the CORONAS-F satellite operation is presented together with that of the two Polish spectrometers, stressing their unique characteristics. The average spectra have been derived and shown here, covering the wavelength range between 3 Å and 7 Å. Future steps in the analysis of the large database collected are outlined.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS223 , June 2004 , pp. 409 - 416
Copyright
© 2004 International Astronomical Union