A turbulent model of the solar granulation

Details A turbulent model of the solar granulation A turbulent model of the solar granulation

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994stin...9529475k&link_type=abstract

Presented at the XV NSO/Sac Peak Solar Workshop, Sunspot, NM, 19-23 Sep. 1994

Astronomy and Astrophysics

Astronomy

Astronomical Models, Mathematical Models, Rotation, Solar Cycles, Solar Energy, Solar Granulation, Sun, Turbulence Models, Bernoulli Theorem, Dynamo Theory, Flow Distribution, Magnetic Fields, Solar Corona, Spatial Distribution, Velocity Distribution

Scientific paper

The paper dealt with a new model for the development of convective velocity fields at various spatial scales in order to understand the differential rotation of the sun which affects the solar dynamo responsible for the magnetic activity as seen in its myriad forms. The new model is based on inverse cascading of energy to take into account the granulation phenomenon in its entirety.

Affiliated with

Also associated with

No associations

Rating

A turbulent model of the solar granulation 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 A turbulent model of the solar granulation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A turbulent model of the solar granulation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1415704