Cosmic Electrodynamics by Gregory D. Fleishman & Igor N. Toptygin

Author:Gregory D. Fleishman & Igor N. Toptygin
Language: eng
Format: epub
Publisher: Springer New York, New York, NY

(8.79)

where the velocity of large-scale motion is , with the angular velocity dependent on the coordinates. A possible rotation model includes a spherically symmetric component:

(8.80)

where Ω 0 and Ω 1 are some constants. The ratio quantifies the differential rotation. This parameter is positively or negatively defined depending on where the rotation is faster—at the center or surface of the star.

The turbulent parameters α and ν t , which are distinctly different in the two considered zones, can be modeled by smooth functions with a narrow transition region:

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