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Dusty plasma effects in near earth space and interplanetary medium

Authors :
Sonoyo Mukai
Jana Safrankova
Tadashi Mukai
Edmond Murad
Zdenek Nemecek
Andrzej Czechowski
Olga Popova
Nicole Meyer-Vernet
Asta Pellinen-Wannberg
Ingrid Mann
Marlene Rosenberg
Belgian Institute for Space Aeronomy
Umeå University and Swedish Institute of Space Physics
Institute for Dynamics of Geospheres, Russian Academy of Sciences
Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA)
Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Physique des plasmas
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Department of Electrical and Computer Engineering [Univ California San Diego] (ECE - UC San Diego)
University of California [San Diego] (UC San Diego)
University of California (UC)-University of California (UC)
Kobe University
Polish Space Research Institute
Kinki University
Charles University, Prague, Czech Republic
Source :
Space Science Reviews, Space Science Reviews, 2011, 161, pp.1-47. ⟨10.1007/s11214-011-9762-3⟩
Publication Year :
2011
Publisher :
Umeå universitet, Institutionen för fysik, 2011.

Abstract

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 nanodust trajectories in the solar wind. Moreover understanding of the complex dependencies that cause the variation of nanodust fluxes is still a challenge. 540010117 Gästprofessur Mann 540010110 Driftsmedel Pellinen-Wannberg

Details

Language :
English
ISSN :
00386308 and 15729672
Database :
OpenAIRE
Journal :
Space Science Reviews, Space Science Reviews, 2011, 161, pp.1-47. ⟨10.1007/s11214-011-9762-3⟩
Accession number :
edsair.doi.dedup.....7fd5fc66b130803780786c34f748f218
Full Text :
https://doi.org/10.1007/s11214-011-9762-3⟩