On Magnetic Fields of Active Regions at Coronal Heights

Details On Magnetic Fields of Active Regions at Coronal Heights On Magnetic Fields of Active Regions at Coronal Heights

Feb 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012soph..276...61b&link_type=abstract

Solar Physics, Volume 276, Issue 1-2, pp. 61-73

Physics

Coronal Magnetic Fields, Microwave Emission, Polarization, Solar Radio Radiation, Spectral Data

Scientific paper

This paper analyzes the magnetic field structure of active regions at coronal heights determined by means of multi-wavelength observations of polarized radio emission in the microwave range, and compares it with the force-free magnetic field extrapolation into the corona from the photospheric magnetograms. Our method of one-dimensional radio stereoscopy indicates higher magnetic field strength compared with the field reconstructed from photospheric magnetograms. It is shown that the sense of inclinations of the field lines we obtained from the radio data matches the shape of the reconstructed magnetic field lines, although the degree of the inclinations is very different.

Affiliated with

Also associated with

No associations

Rating

On Magnetic Fields of Active Regions at Coronal Heights 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 On Magnetic Fields of Active Regions at Coronal Heights, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On Magnetic Fields of Active Regions at Coronal Heights will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1381030