Effects of Strong Regular Refraction in the Solar Radio Pulse Structure in Spike Events

Details Effects of Strong Regular Refraction in the Solar Radio Pulse Structure in Spike Events Effects of Strong Regular Refraction in the Solar Radio Pulse Structure in Spike Events

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006soph..234..151a&link_type=abstract

Solar Physics, Volume 234, Issue 1, pp.151-167

Physics

4

Scientific paper

We examine the problem related to the scattering of a solar radio pulse in a turbulent coronal plasma, taking into account strong regular refraction. Based on an integral representation of the wave field as an interference integral, we analyze the distortions of the mean profile of the radio pulse in spike events, for the case of the sources located in high coronal arches. It is shown that strong regular refraction of radio emission in the coronal arch plays an important role for pulse structuring during spike events.

Affiliated with

Also associated with

No associations

Rating

Effects of Strong Regular Refraction in the Solar Radio Pulse Structure in Spike Events 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 Effects of Strong Regular Refraction in the Solar Radio Pulse Structure in Spike Events, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Effects of Strong Regular Refraction in the Solar Radio Pulse Structure in Spike Events will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-983624