Science, Volume 314, Issues 5796-5801John Michels (Journalist) American Association for the Advancement of Science, 2006 |
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Page 71
... magnetic loops form above the galactic plane , and the gas concentrated at the base of the magnetic loops may form molecular clouds . Unless the tops of the loops are weighed down by dense gas , they will keep expanding into the halo of ...
... magnetic loops form above the galactic plane , and the gas concentrated at the base of the magnetic loops may form molecular clouds . Unless the tops of the loops are weighed down by dense gas , they will keep expanding into the halo of ...
Page 108
... magnetic fields against a gravita- tional field . In this instability , the gas layer will begin to undulate when it is disturbed in space . Linear theory and nonlinear numerical simu- lations have been extensively developed on the ...
... magnetic fields against a gravita- tional field . In this instability , the gas layer will begin to undulate when it is disturbed in space . Linear theory and nonlinear numerical simu- lations have been extensively developed on the ...
Page 284
... magnetic moment by ~ μ ( / A ) . Because μ≫ μ , this greatly enhances the nuclear Larmor precession rate for nearby spins . Furthermore , the enhance- ment is anisotropic : It is strongest when the external field is oriented ...
... magnetic moment by ~ μ ( / A ) . Because μ≫ μ , this greatly enhances the nuclear Larmor precession rate for nearby spins . Furthermore , the enhance- ment is anisotropic : It is strongest when the external field is oriented ...
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