Differential solar rotation: below the convection zone.

Details Differential solar rotation: below the convection zone. Differential solar rotation: below the convection zone.

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996nawg.1996..223k&link_type=abstract

Nachr. Akad. Wiss. Göttingen II, Jahrg. 1996, Nr. 4, p. 223 - 229

Mathematics

Logic

Solar Interior: Differential Rotation, Solar Convective Zone: Solar Rotation

Scientific paper

The authors discuss the possibility of a sharp transition from differential to rigid rotation below the solar convection zone being produced by an internal magnetic field of the radiative core. The transition due to viscosity is smooth irrespectively of the viscosity value. The poloidal magnetic field locked in the radiative core makes a strong effect. Even a very weak field of 10-4 G reduces the thickness of the transition layer below the helioseismologically imposed upper limit of ≡0.1Rsun.

Affiliated with

Also associated with

No associations

Rating

Differential solar rotation: below the convection zone. 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 Differential solar rotation: below the convection zone., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Differential solar rotation: below the convection zone. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1150286