Quasi-biennial oscillations of the green corona intensity

Details Quasi-biennial oscillations of the green corona intensity Quasi-biennial oscillations of the green corona intensity

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985baicz..36..199a&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 36, July 1985, p. 199-205.

Astronomy and Astrophysics

Astronomy

15

Solar Corona, Solar Cycles, Solar Oscillations, Amplitude Distribution Analysis, Autocorrelation, Cross Correlation, Periodic Variations

Scientific paper

An analysis of the quasi-biennial oscillations in the intensity of the green solar corona is presented. Oscillation amplitude and period variations in green corona activity over the period 1947-1976 were obtained according to spectral data for latitudes between + and - 60 degrees. It is shown that the averaged coronal activities are almost equivalent to those of sunspots. The velocity of the green corona emission above the photosphere is estimated based on the period of the oscillations. Monthly values for the biennial component of green corona intensities for individual latitudes are given in a table. The obtained oscillations are discussed within the framework of Gnevyshev's (1977) two maximum models of the solar cycle.

Affiliated with

Also associated with

No associations

Rating

Quasi-biennial oscillations of the green corona intensity does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Quasi-biennial oscillations of the green corona intensity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Quasi-biennial oscillations of the green corona intensity will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1231573