Structure and Dynamics of Sunspots

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

12 pages, 4 figures, conference proceedings

Scientific paper

The physics of Sunspots is a fascinating and demanding field of research in solar astronomy. Interaction of magnetic fields and plasma flows takes place in a tangled magnetic geometry and occurs on spatial scales that pose a continuous challenge for existing instrumentation and for the unambiguous interpretation of spectropolarimetric observations. Thus, the main properties of sunspots are well established but its fine structure is not yet fully understood. In this contribution we summarize the current knowledge of the magnetic and dynamic properties of sunspots at the photospheric level based on selected observations featuring the highest possible spatial and spectral resolution. We concentrate on light bridges, umbral dots, penumbral filaments and the notorious dark cores in penumbral filaments. We report on the morphology of the fine structure elements but mostly focus on observations of their line-of-sight velocities and magnetic field parameters. We briefly comment on results from recent radiative MHD simulations and more schematic model ideas that attempt to rationalize observations of the penumbra.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Structure and Dynamics of Sunspots 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 Structure and Dynamics of Sunspots, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Structure and Dynamics of Sunspots will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-670573

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.