On the phase shift between solar radio emission at the wavelength 10.7 cm and Lα-emission.

Details On the phase shift between solar radio emission at the wavelength 10.7 cm and Lα-emission. On the phase shift between solar radio emission at the wavelength 10.7 cm and Lα-emission.

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990bsold..10...71i&link_type=abstract

Byulletin Solnechnye Dannye Akademie Nauk USSR, No. 10/90, p. 71 - 75

Computer Science

Solar Radio Radiation: Intensities, Solar Spectrum: Lyman Alpha

Scientific paper

A comparison of daily intensities of the solar Lα-emission and solar radio flux at the wavelength 10.7 cm (F10.τ) for the period January 1982 - June 1988 has been made. It is shown that the lag of 27-day maxima of Lα-emission relative to those of F10.τ is equal to 24 hours on the average and can be explained as due to a different velocity of the decrease of the active region of intensity at different intervals of the solar spectrum.

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