Computer Science
Scientific paper
Oct 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001kfnt...17..389b&link_type=abstract
Kinematika i Fizika Nebesnykh Tel, vol. 17, no. 5, p. 389-402
Computer Science
Scientific paper
A possibility that solar flares cause high-amplitude fast variations of spectral lines in Comet Halley is considered. Daily numbers of solar spots and proton fluxes with energies more than 1 MeV are compared with spectral variation of these lines. It is shown that in the observation periods the comet was projected onto an active region of the Sun, but, among all the kinds of solar activity, chiefly the solar proton flows with energies less than 4 MeV coincide in time with fast intensity variations in the spectral lines. An algorithm of cross-correlation analysis of discrete sampling series with gaps is built, average cross-correlation coefficients are calculated. Cross-correlation functions and Fourier spectra which were obtained within the scope of the SOPROG program in November-December of 1985 are presented.
Borysenko S. A.
Shulman L. M.
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