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Ralf Srama

Researcher at University of Stuttgart

Publications -  269
Citations -  8158

Ralf Srama is an academic researcher from University of Stuttgart. The author has contributed to research in topics: Cosmic dust & Interplanetary dust cloud. The author has an hindex of 43, co-authored 264 publications receiving 7101 citations. Previous affiliations of Ralf Srama include Baylor University & Max Planck Society.

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High-velocity streams of dust originating from Saturn

TL;DR: All bursts of dust impacts detected within 150 Saturn radii are characterized by impact directions markedly different from those measured between the bursts, and they clearly coincide with the spacecraft's traversals through streams of compressed solar wind.

South-North and radial traverses through the interplanetary dust cloud

TL;DR: In this paper, a new model was developed based on Divine's (1993) "Five populations of interplanetary meteoroids" model to define four populations of meteoroids on elliptical orbits plus one population on hyperbolic orbits that all can fit the micrometeoroid flux observed by Galileo and Ulysses.
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The composition of Saturn's E ring

TL;DR: The first in situ direct measurement of the composition of particles in Saturn's rings is presented in this paper. But this measurement was performed by the Cassini cosmic dust analyser (CDA) which measured the mass spectra of nearly 300 impacting dust particles during the 2004 October E ring crossing.
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The electrostatic potential of E ring particles

TL;DR: In this article, the electrostatic potential of E ring particles was measured using the charge-sensitive grid system of the cosmic dust analyser (CDA) on the Cassini spacecraft, which allows an in situ determination of the charge of grains bigger than 2.
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Low-mass nitrogen-, oxygen-bearing, and aromatic compounds in Enceladean ice grains

TL;DR: In this article, a compositional analysis of CDA mass spectra from organic-bearing ice grains was performed on the Enceladus seafloor and the results indicated that low-mass amines, carbonyls, and aromatic compounds were the best candidates for the N- and O-bearing compounds.