Magnetic fine-structures and granular velocities

Details Magnetic fine-structures and granular velocities Magnetic fine-structures and granular velocities

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ssrv...29..373c&link_type=abstract

(Schweizerische Naturforschende Gesellschaft and Eidgenoessische Technische Hochschule Zuerich, Conference on Solar Physics from

Physics

Fine Structure, Magnetic Flux, Photosphere, Solar Granulation, Spatial Resolution, Grist (Telescope), Solar Magnetic Field, Spacelab Payloads, Stellar Models, Stellar Structure

Scientific paper

Existing models of magnetic fine structures can be improved by repeated observations with a resolution of less than or equal to 0.1 arcsec over a wide range of wavelengths. The retrieval of the granular velocity gradient in photospheric line asymmetry is possible only if observations with extremely high spatial (less than or equal to 0.2 arcsec) and spectral (Lambda/delta Lambda equals 400,000) resolution are available for the lifetime of a supergranule. Ground-based observations only allow a resolution of 0.3 arcsec within a very limited range of wavelengths; using SOT and GRIST on Spacelab may provide data of the required quality.

Affiliated with

Also associated with

No associations

Rating

Magnetic fine-structures and granular velocities 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 Magnetic fine-structures and granular velocities, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magnetic fine-structures and granular velocities will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1265850