The scattering effect of p and g modes due to magnetic structure of solar spots and flares in the chromosphere

Details The scattering effect of p and g modes due to magnetic structure of solar spots and flares in the chromosphere The scattering effect of p and g modes due to magnetic structure of solar spots and flares in the chromosphere

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996r%26qe...39..815k&link_type=abstract

Radiophysics and Quantum Electronics, Volume 39, Issue 10, pp.815-816

Physics

Scientific paper

We present the results of the processing of flare location data in the coordinate system of bipolar spot groups rotating with proper angular velocity ω(ϕ) in 20 active regions (AR). The polar diagrams R=R(ψ) show the spatial modulation of flares which are seen as the lines of preferred density with two scattering centers in the leader (p) and tail (f) spot. The number of flares per unit area I(ψ) is similar to the indicatrix of the Rayleigh wave scattering. It is not excluded that the banded structure of the flare distribution in bipolar groups (spatial modulation) is defined by polarization-interferential phenomena when p and g modes pass through the magnetic structure of the chromosphere.

Affiliated with

Also associated with

No associations

Rating

The scattering effect of p and g modes due to magnetic structure of solar spots and flares in the chromosphere 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 The scattering effect of p and g modes due to magnetic structure of solar spots and flares in the chromosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The scattering effect of p and g modes due to magnetic structure of solar spots and flares in the chromosphere will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1140317