Ralf Srama

TL;DR: In this article, the authors found that the detection patterns of the stream particles are well correlated with the interplanetary magnetic field structures, and that as the spacecraft crosses the compression regions of the Co-rotation interaction regions, not only the directionality of the impacts changes with the field direction, but also the impact signal and rate vary with an increase of field strength.

TL;DR: In this paper, the authors developed a meteoroid stream model that consists of a large database of cometary streams from all known comets in the inner solar system, which can be used to predict meteor showers from most known comet, that can be observed anytime from 1980 to 2080.

TL;DR: SARIM-PLUS as discussed by the authors employs latest in-situ techniques for a full characterisation of individual micrometeoroids (flux, mass, charge, trajectory, composition).

TL;DR: Max-Planck-Institut fur Kernphysik, Heidelberg, Germany LASP, University of Colorado, Boulder, CO, USA Institut fuer Planetologie, Westfalische Wilhelms-Universitat, Munster, Germany IGEP, Universitat Braunschweig, Braunschelm, Braunsching, Germany Maxplanck Institute for Sonnensystemforschung, Katlenburg-Lindau, Germany Institut fur Raumfahrtsysteme, Stutt

TL;DR: In this article, the results of studies of cratermorphology generated by impacts using micron-sized polypyrrole (PPy)-coated olivineparticles were presented.