Ye. G. Yeroshenko

TL;DR: In this article, the magnetic fields of Mars have been measured from Phobos 2 with high temporal resolution in the tail and down to an 850 km altitude during four successive highly elliptical orbits, the position of the bow shock as well as that of a transition layer, the 'planetopause', were identified.

TL;DR: In this article, the magnetometer (MISCHA) aboard the Vega 1 spacecraft observed an increased level of magnetic field turbulence, resulting from an upstream bow wave, and measured a peak field strength of 70-80 nT and observed draping of magnetic fields around the cometary obstacle.

TL;DR: In this article, high-resolution Vega 1 and 2 magnetic measurements in the cometary magnetosphere and magnetosheath of Halley reveal the presence of fluctuations with the signature expected for the mirror instability.

TL;DR: The region upstream from the Mars subsolar bow shock is surveyed for the presence of MHD wave phenomena using the high-temporal resolution data from the Magma magnetometer as discussed by the authors, and strong turbulence is observed when the magnetic field is connected to the Mars bow shock in such a way as to allow diffuse ions to reach the spacecraft.

TL;DR: In this paper, a 2-lobed magnetic tail of the Phobos spacecraft was observed to have a peak solar-antisolar component of the magnetic field in these lobes.