Hostname: page-component-586b7cd67f-g8jcs Total loading time: 0 Render date: 2024-11-20T09:26:38.362Z Has data issue: false hasContentIssue false
  • English
  • Français

Detection of H- and He-like resonance lines of chlorine in solar flare spectra

Published online by Cambridge University Press:  14 March 2005

B. Sylwester ,
J. Sylwester ,
M. Siarkowski ,
K.J.H. Phillips  and
E. Landi
B. Sylwester
Affiliation:
Space Research Centre, Polish Academy of Sciences, Wroclaw ul. Kopernika 11, Poland email: bs@cbk.pan.wroc.pl
J. Sylwester
Affiliation:
Space Research Centre, Polish Academy of Sciences, Wroclaw ul. Kopernika 11, Poland email: bs@cbk.pan.wroc.pl
M. Siarkowski
Affiliation:
Space Research Centre, Polish Academy of Sciences, Wroclaw ul. Kopernika 11, Poland email: bs@cbk.pan.wroc.pl
K.J.H. Phillips
Affiliation:
NASA Goddard Space Flight Center, Greenbelt, MD 20771, U. S. A.
E. Landi
Affiliation:
E. O. Hulburt Center for Space Research, US NRL, Washington, DC 20375
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.

Preliminary analysis of spectra collected with the RESIK Bragg bent crystal X-ray spectrometer aboard CORONAS-F indicates the presence of many spectral features which until recently were unidentified. We present RESIK spectra in which the H-like Cl XVII Ly$\alpha$ line at 4.182 Å and He-like Cl XVI triplet components in the range 4.43 Å-4.45 Å are identified.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. 671 - 674
Copyright
© 2004 International Astronomical Union