Physics
Scientist
Geophysical Inst. University of Alaska, College
A Dynamical Model of Auroral Morphology
Dynamo action in the ionosphere and motions of the magnetospheric plasma. I. Symmetric dynamo action
Dynamo action in the ionosphere and motions of the magnetospheric plasma. II. Deformation of the radiation belts due to the electrostatic field produced by ionospheric winds
Dynamo action in the ionosphere and motions of the magnetospheric plasma. III. The Pedersen conductivity, generalized to take account of acceleration of the neutral gas
Radiation Information from 1958δ2
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