Vladimir A. Osherovich

TL;DR: In this paper, high-resolution magnetic field and plasma measurements of an interplanetary magnetic cloud and its interaction with the earth's magnetosphere on January 14/15, 1988 are interpreted and discussed.

TL;DR: In this article, a dimensional analysis of two characteristic time scales in the boundary layer where the disk adjusts to the rotating neutron star (NS) is presented, where boundary layer is treated as a transition region between the NS surface and the first Keplerian orbit, where the radial transport of the angular momentum in this layer is controlled by a viscous force defined by the Reynolds number, which is related to the mass accretion rate.

TL;DR: In this article, the authors compare and contrast two models for the global magnetic field line topology of magnetic clouds: a magnetic flux tube geometry, on the one hand, and a spheromak geometry (including possible higher multiples), on the other.

TL;DR: In this paper, the dynamics of radially expanding magnetic clouds is rigorously analyzed within the framework of ideal MHD, where the cloud is modelled as a cylindrically symmetric magnetic flux rope.

TL;DR: The Unified Radio and Plasma Wave (URAP) experiment has produced new observations of the Jupiter environment, owing to the unique capabilities of the instrument and the traversal of high Jovian latitudes.