Other
Scientific paper
Dec 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..358..137c&link_type=abstract
Solar Polarization 4, ASP Conference Series, Vol. 358, Proceedings of the conference held 19-23 September, 2005, in Boulder, Col
Other
1
Scientific paper
The characteristic size of penumbral structures are still below the current resolution limit of modern solar telescopes. Though we have seen a significant progress in theoretical work over the last decades no tight constraints can be placed on the size of penumbral structures in order to favor models with relatively large and thick magnetic flux elements, just at or below the current resolution limit, or on the other hand, clusters of optically thin micro-structures.
Based on a macroscopic 2-component inversion and the approach of polarized radiative transfer in stochastic media, we have estimated the characteristic length scale of the magnetic fluctuation in a sunspot penumbra from observed Stokes spectra. The results yield a coherent picture for the entire magnetic neutral line of the penumbra and indicate that the magnetic fluctuations have a typical length scale between 30 km and 70 km.
Carroll Andrew T.
Staude Jakob
No associations
LandOfFree
The Characteristic Length Scale of the Magnetic Fluctuation in a Sunspot Penumbra: A Stochastic Polarized Radiative Transfer Approach 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 Characteristic Length Scale of the Magnetic Fluctuation in a Sunspot Penumbra: A Stochastic Polarized Radiative Transfer Approach, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Characteristic Length Scale of the Magnetic Fluctuation in a Sunspot Penumbra: A Stochastic Polarized Radiative Transfer Approach will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1240961