Dusty Plasma Effects in Near Earth Space and Interplanetary Medium

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F11%3A10108197" target="_blank" >RIV/00216208:11320/11:10108197 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1007/s11214-011-9762-3" target="_blank" >http://dx.doi.org/10.1007/s11214-011-9762-3</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1007/s11214-011-9762-3" target="_blank" >10.1007/s11214-011-9762-3</a>

Result language
angličtina
Original language name
Dusty Plasma Effects in Near Earth Space and Interplanetary Medium
Original language description
We review dust and meteoroid fluxes and their dusty plasma effects in the interplanetary medium near Earth orbit and in the Earth's ionosphere. Aside from in-situ measurements from sounding rockets and spacecraft, experimental data cover radar and optical observations of meteors. Dust plasma interactions in the interplanetary medium are observed by the detection of charged dust particles, by the detection of dust that is accelerated in the solar wind and by the detection of ions and neutrals that are released from the dust. These interactions are not well understood and lack quantitative description. There is still a huge discrepancy in the estimates of meteoroid mass deposition into the atmosphere. The radar meteor observations are of particular interest for determining this number. Dust measurements from spacecraft require a better understanding of the dust impact ionization process, as well as of the dust charging processes. The latter are also important for further studying nanodus
Czech name
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Czech description
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Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BL - Plasma physics and discharge through gases
OECD FORD branch
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Publication year
2011
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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