Turbulence and convection are phenomena that haunt astrophysicists because they pose problems that are both difficult and interesting, such as mixing and burning in stars; plumes in convection zones: two-phase shear instabilities and others. Representatives of four viewpoints approach these and other deep astronomy phenomena: the computational physicist's numerical three-dimensional large-eddy simulations; theorists, who wish to simplify the equations into approximate one-dimensional recipes; astrophysicists, who see ...
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Turbulence and convection are phenomena that haunt astrophysicists because they pose problems that are both difficult and interesting, such as mixing and burning in stars; plumes in convection zones: two-phase shear instabilities and others. Representatives of four viewpoints approach these and other deep astronomy phenomena: the computational physicist's numerical three-dimensional large-eddy simulations; theorists, who wish to simplify the equations into approximate one-dimensional recipes; astrophysicists, who see turbulence and convection as a subroutine; and experimentalists, who provide valuable insights into what really happens.
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Seller's Description:
Good-Bumped and creased book with tears to the extremities, but not affecting the text block, may have remainder mark or previous owner's name-GOOD PAPERBACK Standard-sized.