Nonlinear analysis of decimetric solar bursts

Details Nonlinear analysis of decimetric solar bursts Nonlinear analysis of decimetric solar bursts

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010iaus..264..279r&link_type=abstract

Solar and Stellar Variability: Impact on Earth and Planets, Proceedings of the International Astronomical Union, IAU Symposium,

Astronomy and Astrophysics

Astronomy

Turbulence, Sun: Radio Radiation, Solar-Terrestrial Relations, Methods: Data Analysis

Scientific paper

The solar radio emissions in the decimetric frequency range (above 1 GHz) are very rich in temporal and spectral fine structures due to nonlinear processes occurring in the magnetic structures on the corresponding active regions. In this paper we characterize the singularity spectrum, f(α), for solar bursts observed at 1.6, 2.0 and 3 GHz. We interpret our findings as evidence of inhomogeneous plasma turbulence driving the underlying plasma emission process and discuss the nonlinear multifractal approach into the context of geoeffective solar active regions.

Affiliated with

Also associated with

No associations

Rating

Nonlinear analysis of decimetric solar bursts 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 Nonlinear analysis of decimetric solar bursts, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Nonlinear analysis of decimetric solar bursts will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1095791