Science, Том 314,Выпуски 5796-5801John Michels (Journalist) American Association for the Advancement of Science, 2006 |
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Стр. 71
... field lines oriented parallel to the midplane of a disk - shaped galaxy . The real galactic magnetic field is subject to considerable distortion about the mean field shown . ( Middle ) Any vertical per- turbation to the field lines ...
... field lines oriented parallel to the midplane of a disk - shaped galaxy . The real galactic magnetic field is subject to considerable distortion about the mean field shown . ( Middle ) Any vertical per- turbation to the field lines ...
Стр. 108
... 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 instability ...
... 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 instability ...
Стр. 284
... field is oriented perpendicular to the NV axis , corresponding to the largest degree A 1 NV E Probability ( p ) 0.75 0.5 0.25 O 0.5 B 14 NV C 12 10 NV E 8 1.5 of mixing . For a properly oriented magnetic field , proximal nuclei can ...
... field is oriented perpendicular to the NV axis , corresponding to the largest degree A 1 NV E Probability ( p ) 0.75 0.5 0.25 O 0.5 B 14 NV C 12 10 NV E 8 1.5 of mixing . For a properly oriented magnetic field , proximal nuclei can ...
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