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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
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
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Abstract

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
Copyright
© 2004 International Astronomical Union

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