Resolution of magnetic flux tubes on the sun

Details Resolution of magnetic flux tubes on the sun Resolution of magnetic flux tubes on the sun

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992natur.359..307k&link_type=abstract

Nature (ISSN 0028-0836), vol. 359, no. 6393, p. 307, 308.

Physics

97

Magnetic Field Configurations, Magnetic Flux, Solar Magnetic Field, Late Stars, Solar Activity, Solar Atmosphere, Solar Granulation, Spatial Resolution, Speckle Interferometry

Scientific paper

A newly developed technique of speckle interferometry has been used to obtain simultaneous direct observations of the white light and magnetic field signatures of solar flux tubes. Individual flux tubes are seen with resolved diameters of about 200 km and continuum brightness contrasts of at least +30 percent. Magnetic features larger than 300 km in size tend, however, to be darker than their surroundings.

Affiliated with

Also associated with

No associations

Rating

Resolution of magnetic flux tubes on the sun 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 Resolution of magnetic flux tubes on the sun, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Resolution of magnetic flux tubes on the sun will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1091873