An explanation for the Stokes V asymmetry in solar faculae

Details An explanation for the Stokes V asymmetry in solar faculae An explanation for the Stokes V asymmetry in solar faculae

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...201l..37s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 201, no. 2, Aug. 1988, p. L37-L40.

Astronomy and Astrophysics

Astrophysics

28

Faculae, Magnetic Field Configurations, Magnetohydrodynamics, Solar Magnetic Field, Stokes Law Of Radiation, Astronomical Models, Circular Polarization, Photosphere, Wavelengths

Scientific paper

The asymmetry in the Stokes V profile observed in solar faculae can be
explained by assuming that the magnetic field increases with height
while downflow speed decreases. The MHD compatibility of such solution
is briefly discussed together with an observational test for that
possibility.

Affiliated with

Also associated with

No associations

Rating

An explanation for the Stokes V asymmetry in solar faculae 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 An explanation for the Stokes V asymmetry in solar faculae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An explanation for the Stokes V asymmetry in solar faculae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1692908