Mathematics – Logic
Scientific paper
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.
Kitchatinov Leonid L.
Rudiger Günther
No associations
LandOfFree
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.
Profile ID: LFWR-SCP-O-1150286