Hostname: page-component-745bb68f8f-cphqk Total loading time: 0 Render date: 2025-01-31T01:59:10.705Z Has data issue: false hasContentIssue false
  • English
  • Français

Observation of the Annular Solar Eclipse of May 31 2003 in far ultraviolet spectral region

Published online by Cambridge University Press:  14 March 2005

V. V. Katyushina ,
T. V. Kazachevskaya  and
A. A. Nusinov
V. V. Katyushina
Affiliation:
Institute of Applied Geophysics, Russian Hydrometeorological Service, Moscow email: geophys@hydromet.ru
T. V. Kazachevskaya
Affiliation:
Institute of Applied Geophysics, Russian Hydrometeorological Service, Moscow email: geophys@hydromet.ru
A. A. Nusinov
Affiliation:
Institute of Applied Geophysics, Russian Hydrometeorological Service, Moscow email: geophys@hydromet.ru
Rights & Permissions [Opens in a new window]

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.

Changes of extreme ultraviolet (EUV) Solar flux were registered during the Annular Solar eclipse of May 31 2003, when CORONAS-F satellite (Oraevsky et al., 2002) intersected thrice a zone of the Solar eclipse. During these periods the solar emission was measured in visible and extreme UV spectral regions (near $L_{\alpha} = 121.6$ nm by VUSS instrument). Records by VUSS ($\sim 120$ nm) and the optical (visible) channel of EOS instruments on UTC scale for May 31, 2003 are given on Fig. 1.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. 389 - 390
Copyright
© 2004 International Astronomical Union