Lunar dust levitation
Journal of Aerospace Engineering, ISSN: 0893-1321, Vol: 22, Issue: 1, Page: 2-9
2009
- 78Citations
- 4Usage
- 46Captures
- 4Mentions
Metric Options: CountsSelecting the 1-year or 3-year option will change the metrics count to percentiles, illustrating how an article or review compares to other articles or reviews within the selected time period in the same journal. Selecting the 1-year option compares the metrics against other articles/reviews that were also published in the same calendar year. Selecting the 3-year option compares the metrics against other articles/reviews that were also published in the same calendar year plus the two years prior.
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Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
Citation Benchmarking is provided by Scopus and SciVal and is different from the metrics context provided by PlumX Metrics.
Metrics Details
- Citations78
- Citation Indexes78
- 78
- CrossRef49
- Usage4
- Abstract Views4
- Captures46
- Readers46
- 45
- Mentions4
- References4
- 4
Article Description
Observations of a lunar "horizon glow" by several Surveyor spacecraft on the lunar surface in the 1960s and detections of dust particle impacts by the Apollo 17 Lunar Ejecta and Meteoroid Experiment have been explained as the result of micron-sized charged particles lifting off the surface. The surface of the Moon is exposed to the solar wind and solar UV radiation causing photoemission, so it develops a surface charge and an electric field near the surface. Dust particles injected into this plasma from the lunar regolith, whether from human and mechanical activity or from meteoroid impacts or electrostatic forces, may be stably levitated above the surface and may undergo preferential deposition onto areas of the lunar surface (or equipment) with different electrical properties. This can lead to a net transport as well as contamination of sensitive equipment. This paper reports on new experimental measurements and numerical simulations of the plasma environment above the lunar surface and the related behavior of charged dust. © 2009 ASCE.
Bibliographic Details
https://stars.library.ucf.edu/facultybib2000/1433; https://stars.library.ucf.edu/scopus2000/12277; http://stars.library.ucf.edu/facultybib2000/1433
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=58149251812&origin=inward; http://dx.doi.org/10.1061/(asce)0893-1321(2009)22:1(2); https://ascelibrary.org/doi/10.1061/%28ASCE%290893-1321%282009%2922%3A1%282%29; http://ascelibrary.org/doi/10.1061/%28ASCE%290893-1321%282009%2922%3A1%282%29; http://ascelibrary.org/doi/pdf/10.1061/%28ASCE%290893-1321%282009%2922%3A1%282%29; https://stars.library.ucf.edu/facultybib2000/1433; https://stars.library.ucf.edu/cgi/viewcontent.cgi?article=2432&context=facultybib2000; https://stars.library.ucf.edu/scopus2000/12277; https://stars.library.ucf.edu/cgi/viewcontent.cgi?article=13276&context=scopus2000; http://stars.library.ucf.edu/facultybib2000/1433; http://stars.library.ucf.edu/cgi/viewcontent.cgi?article=2432&context=facultybib2000; http://dx.doi.org/10.1061/%28asce%290893-1321%282009%2922%3A1%282%29; https://dx.doi.org/10.1061/%28asce%290893-1321%282009%2922%3A1%282%29
American Society of Civil Engineers (ASCE)
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