Spectrum of Fluctuations of Solar Noise Storms

Details Spectrum of Fluctuations of Solar Noise Storms Spectrum of Fluctuations of Solar Noise Storms

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007soph..246..415y&link_type=abstract

Solar Physics, Volume 246, Issue 2, pp.415-418

Physics

Sun:&Nbsp, Noise Storm

Scientific paper

The calculation of the Fourier transform of noise storm (NS) fluctuations showed that the power spectrum was adequately described by the expression G( F)˜1/ F. Our results rule out the possibility that NS radiation is formed from random, short-term bursts (so-called type I bursts), since the spectrum of the sum of random short fluctuations is flat, but the real NS has a hyperbolic spectrum. This spectrum is monotonic and does not contain any components that exceed the level of the statistical fluctuations ( i.e., the results of observations do not reveal the presence of periodic or resonant properties of the emission source). The hyperbolic shape of the spectrum shows that the main energy of a NS is contained in the slower temporal fluctuations.

Affiliated with

Also associated with

No associations

Rating

Spectrum of Fluctuations of Solar Noise Storms 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 Spectrum of Fluctuations of Solar Noise Storms, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectrum of Fluctuations of Solar Noise Storms will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1027577