The differential rotation of solar magnetic field elements

Details The differential rotation of solar magnetic field elements The differential rotation of solar magnetic field elements

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988kfnt....4...23g&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 4, Nov.-Dec. 1988, p. 23-27. In Russian.

Astronomy and Astrophysics

Astrophysics

Gyromagnetism, Magnetic Field Configurations, Solar Magnetic Field, Solar Rotation, Angular Velocity, Solar Corona, Visible Spectrum

Scientific paper

The structure of solar magnetic field elements is studied using high spatial resolution observations of the longitudinal component in the Fe I 525.02 nm line. The observations were carried out at the solar tower telescope of the Crimean Astrophysical Observatory in September 1986. It is found that the east-west asymmetry of the magnetic field elements is different at different latitudes. The sidereal rotation rate of the magnetic elements is about 1.93 km/s at a latitude of 17 deg N and 1.47 km/s at a latitude of 40 deg N. It is found that the solar magnetic field elements as well as the K corona have more rigid-body differential rotation than does a photospheric plasma.

Affiliated with

Also associated with

No associations

Rating

The differential rotation of solar magnetic field elements 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 differential rotation of solar magnetic field elements, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The differential rotation of solar magnetic field elements will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1758841