The behavior of the Sun's magnetic field is strongly influenced by the combination of convective currents, which bring the charged plasma from deep within the Sun to the Sun's surface, and the differential rotation of the outer layers of the Sun. The complex, swirling motions that result make a tangled mess of...
www.windows.ucar.edu/tour/link=/sun/Solar_interior/Sun_... www.windows.ucar.edu/tour/link=/sun/Solar_interior/Sun_layers/differential_rotation.html
Solar rotation - Wikipedia, the free encyclopedia
Solar rotation is able to vary with latitude because the Sun is composed of a gaseous plasma. The rate of rotation is observed to be fastest at the equator (latitude φ=0 deg), and to decrease as lati...
en.wikipedia.org/wiki/Solar_rotation
Lesson: Differential Rotation of the Sun ... This is known as differential rotation. ... Independent Student Research: Students study images of the sun for a period of 2 - 3 months, track active regions at different latitudes, and calculate differential rotations.
sohowww.nascom.nasa.gov/explore/lessons/diffrot9_12.htm... sohowww.nascom.nasa.gov/explore/lessons/diffrot9_12.html
2.   Differential rotation of the sun a. causes the heating in the chromosphere and corona that makes them hotter than the photosphere. b. is caused by the magnetic dynamo inside the sun. c. implies that the equatorial regions of the sun rotate more rapidly than the polar regions.
hoth.ncat.edu/~michael/moonstruck/astrotrivia/sun-earth... hoth.ncat.edu/~michael/moonstruck/astrotrivia/sun-earth.html
This lesson has students use Solar and Heliospheric Observatory (SOHO) data from the EIT (Extreme-ultraviolet Imaging Telescope) instrument on the spacecraft to discover differential rotation of the Sun. They will realize that the Sun has a north and south pole, just as the Earth does, and rotates on its axis.
www.dlese.org/library/catalog_DLESE-000-000-008-572.htm
Earth has a radius of about 6,400 km, the sun has a radius of about 7.0 x 105 km, and a rubber ball has a radius of 6.4 cm. If you were to construct a scale model of the solar system using the rubber ball to represent Earth, ... Precession of the rotation axis of Earth is caused by ... Differential rotation of the sun...
www.shawneecc.edu/craigb/AST111/tests/studyguide1-11.ht... www.shawneecc.edu/craigb/AST111/tests/studyguide1-11.htm
Title:; Wavelet analysis of stellar differential rotation. II. The Sun in ultraviolet ... Among the several methods to study differential rotation on stellar surfaces the observation of a stellar butterfly diagram, i.e. monitoring the rotation period over a complete activity cycle, is the only method which can be applied...
adsabs.harvard.edu/abs/2002A&A...388..540H
Title : CONVECTION AND THE DIFFERENTIAL ROTATION OF THE SUN, ... It appears that, although the effect of rotation is negligible in the photosphere, it may double the superadiabatic gradient in the deep convective zone. Consequently, if convective heat transport is the same at the poles as at the equator of the Sun,
stinet.dtic.mil/oai/oai?verb=getRecord&metadataPrefix=h... stinet.dtic.mil/oai/oai?verb=getRecord&metadataPrefix=html&identifier=AD0618261
Turbulent Convection and Differential Rotation in the Sun ... Differential rotation and cycles of magnetic activity are intimately linked dynamical processes within the deep shell of highly turbulent convection occupying the outer 30 percent of the Sun just below its surface.
amath.colorado.edu/seminarsOLD/2000fall/toomre.html
Differential rotation in stars - Wikipedia, the free encyclopedia
Differential rotation is when a rotating body has different angular velocities at different latitudes and/or depths of the body and/or in time. Differential rotation can be applied to any type of flu...
en.wikipedia.org/wiki/Differential_rotation_in_stars