Frequency dependence of the periodicity of the intensity of the non-magnetic component of solar radio emission

Details Frequency dependence of the periodicity of the intensity of the non-magnetic component of solar radio emission Frequency dependence of the periodicity of the intensity of the non-magnetic component of solar radio emission

Feb 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999mnras.303..221d&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 303, Issue 2, pp. 221-226.

Astronomy and Astrophysics

Astronomy

4

Sun: Radio Radiation

Scientific paper

The values of the intensity of the non-magnetic component of solar radio emission, delineated after subtracting the contributions of sunspots and the mean magnetic field of the Sun from the observed radio flux, have been determined in the frequency band 245-15 400 MHz for the solar maxima (1980 and 1991), as well as for the solar minimum periods (1975, 1986 and 1996). The periodicity in the non-magnetic component has been found by applying the Fourier integral method and the frequency dependence of the periodicity has been studied.

Affiliated with

Also associated with

No associations

Rating

Frequency dependence of the periodicity of the intensity of the non-magnetic component of solar radio emission 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 Frequency dependence of the periodicity of the intensity of the non-magnetic component of solar radio emission, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Frequency dependence of the periodicity of the intensity of the non-magnetic component of solar radio emission will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-945749