E
Eberhard Grün
Researcher at Max Planck Society
Publications - 414
Citations - 17010
Eberhard Grün is an academic researcher from Max Planck Society. The author has contributed to research in topics: Cosmic dust & Interplanetary dust cloud. The author has an hindex of 68, co-authored 414 publications receiving 15918 citations. Previous affiliations of Eberhard Grün include University of Hawaii & University of Colorado Boulder.
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Modeling the Galileo dust measurements at Jupiter
TL;DR: In this paper, the authors use a detailed fields and particles model of the magnetosphere and simultaneously follow the dynamics and the charging history of small dust particles to reproduce the observed dust impact rates during the first two Ganymede encounters of Galileo.
The interplanetary dust complex and comets
TL;DR: In this paper, the origin and evolution of interplanetary dust clouds are traced to their roots, and these particles are used to provide insights into the origins of their precursor bodies and look at dust production in the disks about other stars.
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Sixteen years of ulysses interstellar dust measurements in the solar system. i. mass distribution and gas-to-dust mass ratio
TL;DR: In this article, the authors analyzed the entire data set from 16 yr of Ulysses interstellar dust measurements in interplanetary space and found a gas-to-dust mass ratio in the local interstellar cloud of and a dust density of (2.1 ± 0.6) × 10−24 kg m−3.
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Dust in jupiter's magnetosphere: Origin of the ring
TL;DR: In this article, a model for the production of the Jovian ring is proposed, where the visible ring particles are micron-sized and produced by erosive collisions between an assumed population of km-sized parent bodies and sub-micron sized magnetospheric dust particles.
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Rosetta begins its Comet Tale
Matthew Taylor,C. Alexander,Nicolas Altobelli,Marco Fulle,Marcello Fulchignoni,Eberhard Grün,Paul R. Weissman +6 more
TL;DR: The first published results from Rosetta at comet 67P were reported in this article, where the authors reported the detection of several molecules, including H2 17O, H2 18O, CO, and CO2 and assessed their time variability and heterogeneous distribution.