G. Erdos

TL;DR: In this article, the Ulysses spacecraft from the south polar regions of the heliosphere to the north polar regions has been used to obtain a unique perspective on the configuration and properties of heliospheric magnetic field at a time of solar minimum activity.

TL;DR: A map of the current sheet in heliographic latitude and Carrington longitude reveals two folds corresponding to four magnetic sectors, associated with a pair of asymmetrically placed polar coronal holes whereas the other two sectors coincided with a near-equatorial coronal hole on opposite sides of the equator as mentioned in this paper.

TL;DR: The ion measurements of the Cassini Plasma Spectrometer are presented which were acquired on 26 December 2005, during the T9 flyby at Titan, and the plasma flow and magnetic field directions in the distant plasma environment of the moon were distinctly different from the other flybys as mentioned in this paper.

TL;DR: Magnetometer data recorded by the Cassini spacecraft during the spacecraft's Earth swing-by maneuver in August 1999 are discussed in this paper, showing the instrument's performance in detection of magnetic phenomena in a planetary environment.

TL;DR: In this paper, the authors examined the onset of high-energy ions observed during the March 1991 series of solar events, and observed a region with a drop in the magnetic field strength, suggesting that they were being convected outward by the CME.