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            <gco:CharacterString>We present here further results concerning geostrophic baroclinic flow with a zonal magnetic field, in a Î²-plane channel, as extensions of earlier work by the writer. We find a necessary condition for instability that proves the existence of a short wave cutoff of unstable baroclinic waves for finite magnetic field. We also place bounds on the phase velocities of neutral waves in the system. For zero basic baroclinic and a uniform magnetic field, the neutral oscillations are zonally propagating geostrophic AlfvÃ©n waves. The lowest mode is purely horizontal and travels at the ordinary AlfvÃ©n speed, but all higher modes, which contain vertical as well as horizontal motion, move more slowly. With Î² â  0, we get, in general, combined AlfvÃ©n-Rossby waves, which, in the limit of large rotation, yield a class of waves very similar to those found by Hide. Finally, we solve the Eady problem (stability of baroclinic flow with constant shear) in a uniform magnetic field, without and with the Î² effect. We find, for Î² = 0, that the field stabilizes the baroclinic wave. Neutral AlfvÃ©n-like waves are found for large field and/or short wavelengths. We also find a pair of "edge waves." For Î² = 0, the longest baroclinic waves are stabilized for small field strengths, as in the nonmagnetic problem, but very weakly unstable waves occur for larger fields. A set of neutral Rossby waves also is present for long wavelengths and the short AlfvÃ©n-like waves are modified, but only slightly.</gco:CharacterString>
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