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Cited by 631

The DOI matches its Crossref record; 3 of the 3 references it cites were found in a registry or an index.

CHARGED DUST DYNAMICS IN THE SOLAR SYSTEM

Horányi, Mihály·1996·Annual Review of Astronomy and Astrophysics

Abstract

▪ Abstract In most space environments, dust particles are exposed to plasmas and UV radiation and, consequently, carry electrostatic charges. Their motion is influenced by electric and magnetic fields in addition to gravity, drag, and radiation pressure. On the surface of the Moon, in planetary rings, or at comets, for example, electromagnetic forces can shape the spatial and size distribution of micron-sized charged dust particles. The dynamics of small charged dust particles can be surprisingly complex, leading to levitation, rapid transport, energization and ejection, capture, and the formation of new planetary rings. This review briefly discusses the most important processes that determine the charge state of dust particles immersed in plasmas and the resulting dynamics on exposed dusty surfaces and in planetary magnetospheres.

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Metadata

Authors
Horányi, M.
Venue
Annual Review of Astronomy and Astrophysics
Published
1996-09
Volume
34
Issue
1
Pages
383-418
ISSN
  • 0066-4146 (ISSN-L)
  • 1545-4282
OpenAlex
W2145578438
Cited by
631
References
3
FWCI
1.52
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: CHARGED DUST DYNAMICS IN THE SOLAR SYSTEM. https://app.cochat.ai/papers/10.1146/annurev.astro.34.1.383
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Horányi, M. (1996). CHARGED DUST DYNAMICS IN THE SOLAR SYSTEM. Annual Review of Astronomy and Astrophysics. https://doi.org/10.1146/annurev.astro.34.1.383

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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.

Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.