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We investigate differential rotation in rapidly rotating solar-type stars by means of an axisymmetric mean field model that was previously applied to the sun. This allows us to calculate the latitudin...
Modeling eclipsing binaries in globular clusters。
The very complicated problem of the solar wind-interstellar medium interaction requires a very sophisticated numerical approach. To achieve such a goal first we need to understand very deeply the resu...
We give an overview of procedures to recover and simulate typical coronal static magnetic field topologies from given boundary data on the photo- sphere. Relatively simple analytical treatments allo...

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