Magnetohelioseismic Analysis of AR10720 Using Helioseismic Holography

Details Magnetohelioseismic Analysis of AR10720 Using Helioseismic Holography Magnetohelioseismic Analysis of AR10720 Using Helioseismic Holography

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..354..168m&link_type=abstract

Solar MHD Theory and Observations: A High Spatial Resolution Perspective ASP Conference Series, Vol. 354, Proceedings of the Con

Astronomy and Astrophysics

Astronomy

4

Scientific paper

We report on the recent discovery of one of the most powerful sunquakes detected to date produced by the January 15, 2005 X1.2 solar flare in active region 10720. We used helioseismic holography to image the acoustic source of the seismic waves produced by the flare. Egression power maps at 6 mHz with a 2 mHz bandwidth reveal a strong, compact acoustic source correlated with the footpoints of a coronal loop that hosted the flare. Using data from various solar observatories, we present a comprehensive analysis of the acoustic properties of the sunquake and investigate the role played by the configuration of the photospehric magnetic field in the production of flare generated sunquakes.

Affiliated with

Also associated with

No associations

Rating

Magnetohelioseismic Analysis of AR10720 Using Helioseismic Holography 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 Magnetohelioseismic Analysis of AR10720 Using Helioseismic Holography, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magnetohelioseismic Analysis of AR10720 Using Helioseismic Holography will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1239998