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Valeri Dikarev

Researcher at Max Planck Society

Publications -  31
Citations -  1369

Valeri Dikarev 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 15, co-authored 31 publications receiving 1274 citations. Previous affiliations of Valeri Dikarev include Saint Petersburg State University & Schiller International University.

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Cassini Dust Measurements at Enceladus and Implications for the Origin of the E Ring

TL;DR: During Cassini's close flyby of Enceladus on 14 July 2005, the High Rate Detector of the Cosmic Dust Analyzer registered micron-sized dust particles enveloping this satellite; this asymmetric signature is consistent with a locally enhanced dust production in the south polar region of Encesladus.
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The Cassini Cosmic Dust Analyzer

TL;DR: The Cassini-Huygens Cosmic Dust Analyzer (CDA) is intended to provide direct observations of dust grains with masses between 10-19 and 10-9 kg in interplanetary space and in the jovian and satumian systems, to investigate their physical, chemical and dynamical properties as functions of the distances to the Sun, to Jupiter and to Saturn and its satellites and rings as mentioned in this paper.
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Impact-generated dust clouds around planetary satellites: spherically symmetric case

TL;DR: In this article, an analytic model of an impact-generated, steady-state, spherically symmetric dust cloud around an atmosphereless planetary satellite (or planet) is constructed.
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Cassini between Venus and Earth: Detection of interstellar dust

TL;DR: In this paper, the authors reported the successful in situ measurement of interstellar dust particles inside the orbit of the Earth with the Cosmic Dust Analyzer (CDA) on the Cassini spacecraft.
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The Dust Halo of Saturn's Largest Icy Moon, Rhea

TL;DR: The Cassini spacecraft's in situ observations reveal that energetic electrons are depleted in the moon's vicinity, implying that Rhea's magnetospheric interaction region, rather than being exclusively induced by sputtered gas and its products, likely contains solid material that can absorb magnetosphere particles.