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
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.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
Dusty plasmas in the solar system
Goertz, C. K. (1989) · Reviews of Geophysics · doi:10.1029/rg027i002p00271 · Cited by 1,694
Encounter with Saturn: Voyager 1 imaging science results
Smith, B. A., Soderblom, L., Beebe, R., Boyce, J., Briggs, G., Bunker, A., Collins, S. A., Hansen, C. J., Johnson, T. V., Mitchell, J. L., et al. (1981) · Science · doi:10.1126/science.212.4491.163 · Cited by 795
Charging of Dust Grains in Plasma with Energetic Electrons
Walch, B., Horányi, M., & Robertson, S. (1995) · Physical Review Letters · doi:10.1103/physrevlett.75.838 · Cited by 208
Self-citation
Cited by
The beneficiation of lunar regolith for space resource utilisation: A review
Rasera, J. N., Cilliers, J. J., Lamamy, J. A., & Hadler, K. (2020) · Planetary and Space Science · doi:10.1016/j.pss.2020.104879 · Cited by 122
Lunar dust charging by photoelectric emissions
Abbas, M. M., Tankosic, D., Craven, P. D., Spann, J. F., LeClair, A., & West, E. A. (2007) · Planetary and Space Science · doi:10.1016/j.pss.2006.12.007 · Cited by 105
Review of dust transport and mitigation technologies in lunar and Martian atmospheres
Afshar-Mohajer, N., Wu, C.-Y., Curtis, J. S., & Gaier, J. R. (2015) · Advances in Space Research · doi:10.1016/j.asr.2015.06.007 · Cited by 96
Kennedy, G. M., & Wyatt, M. C. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.18041.x · Cited by 81
Efficiency determination of an electrostatic lunar dust collector by discrete element method
Afshar-Mohajer, N., Wu, C.-Y., & Sorloaica-Hickman, N. (2012) · Journal of Applied Physics · doi:10.1063/1.4739734 · Cited by 22
Metadata
- Authors
- Horányi, M.
- Venue
- Annual Review of Astronomy and Astrophysics
- Publisher
- Annual Reviews
- 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
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: CHARGED DUST DYNAMICS IN THE SOLAR SYSTEM. https://app.cochat.ai/papers/10.1146/annurev.astro.34.1.383
- The paper
- 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
Data sources
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.