Skip to main content

and
  1. No Access

    Article

    Theoretical plasma distributions consistent with Ulysses magnetic field observations in a solar wind tangential discontinuity

    The overall multi-layer structure of the magnetic field profile observed by Ulysses across a broad solar wind tangential discontinuity can be reproduced fairly well by means of a kinetic model. Such a simulation ...

    J. De Keyser, M. Roth, J. Lemaire, B. T. Tsurutani, C. M. Ho in Solar Physics (1996)