The radio-loud plasma in pulsars
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The pulsar magnetosphere contains a strongly magnetized, relativistic plasma. We need to understand the physics of that plasma if we want to connect the data to the models. Our group in Socorro is mixing theory and observations in order to study the radio-loud pulsar plasma. In this paper we report on several aspects of our current work.
16 pages, 20 figures. Invited review to appear in "Neutron Stars, Pulsars and Supernova Remnants" (proceedings of Bad Honnef meeting, Jan 2002), eds. w. Becker etal, to be published by MPI
16 pages, 20 figures. Invited review to appear in "Neutron Stars, Pulsars and Supernova Remnants" (proceedings of Bad Honnef meeting, Jan 2002), eds. w. Becker etal, to be published by MPI