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Dusty plasma processes in Earth's environments containing nano- and microscale grains

Published online by Cambridge University Press:  13 January 2010

SERGEY I. POPEL*
Affiliation:
Institute for Dynamics of Geospheres RAS, Leninsky prospect 38, building 1, 119334 Moscow, Russia ([email protected])

Abstract

Review of plasma processes in the Earth's environments containing nano- and microscale grains is presented. Possible observational manifestations of dusty ionospheric plasmas during high-speed meteor showers are described. A unified explanation of ionization properties of the polar mesosphere under summer conditions is given. Dusty plasma processes are also considered in application to active geophysical rocket experiments which involve release of some gaseous substance in near-Earth space, the origin of the primary Earth's crust, hydrosphere and atmosphere, and global electromagnetic Schumann resonances.

Type
Papers
Copyright
Copyright © Cambridge University Press 2010

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References

[1]Fortov, V. E., Ivlev, A. V., Khrapak, S. A., Khrapak, A. G. and Morfill, G. E. 2005 Phys. Rep. 421, 1103.CrossRefGoogle Scholar
[2]Ostrikov, K. 2005 Rev. Mod. Phys. 77, 489511.CrossRefGoogle Scholar
[3]Vladimirov, S. V., Ostrikov, K. and Samarian, A. A. 2005 Physics and Applications of Complex Plasmas. London: Imperial College Press.CrossRefGoogle Scholar
[4]Verheest, F. 1994 Space Sci. Rev. 68, 109114.CrossRefGoogle Scholar
[5]Klumov, B. A., Morfill, G. E. and Popel, S. I. 2005 JETP 100, 152164.CrossRefGoogle Scholar
[6]Popel, S. I. and Gisko, A. A. 2006 Nonlinear Proc. Geophys. 13, 223229.CrossRefGoogle Scholar
[7]Holton, J. R., Haynes, P. H., McIntyre, M. E., Douglass, A. R., Rood, R. B. and Pfister, L. 1995 Rev. Geophys. 33, 403439.CrossRefGoogle Scholar
[8]Fromm, M. D. and Servranckx, R. 2003 Geophys. Res. Lett. 30, 1542, doi: 10.1029/2002GL016820.CrossRefGoogle Scholar
[9]Besedina, Yu. N. and Popel, S. I. 2008 Doklady Earth Sciences 423A, 14751478.CrossRefGoogle Scholar
[10]Gadsen, M. and Schröder, W. 1989 Noctilucent Clouds. Berlin: Springer.CrossRefGoogle Scholar
[11]Klumov, B. A., Popel, S. I. and Bingham, R. 2000 JETP Lett. 72, 364368.CrossRefGoogle Scholar
[12]Kopnin, S. I., Kosarev, I. N., Popel, S. I. and Yu, M. Y. 2004 Planet. Space Sci. 52, 11871194.CrossRefGoogle Scholar
[13]McNeil, W., Lai, S. and Murad, E. 1998 J. Geophys. Res. 103, 10 89910 911.CrossRefGoogle Scholar
[14]Popel, S. I. and Tsytovich, V. N. 1999 Astrophys. Space Sci. 264, 219226.CrossRefGoogle Scholar
[15]Gavrilov, B. G., Podgorny, A. I., Podgorny, I. M., Sobyanin, D. B., Zetzer, J. I., Erlandson, R. E., Meng, C.-I. and Stoyanov, B. J. 1999 Geophys. Res. Letters 26, 15491552.CrossRefGoogle Scholar
[16]Besedina, Y. N. and Popel, S. I. 2007 Plasma Phys. Reports 33, 138145.CrossRefGoogle Scholar
[17]Musatenko, S. I., Musatenko, Y. S., Kurochka, E. V., Lastochkin, A. V., Cholij, V. Y., Maksimenko, O. I. and Slipchenko, A. S. 2006 Geomagn. Aeronomy 46, 173182.CrossRefGoogle Scholar
[18]Rao, N. N., Shukla, P. K. and Yu, M. Y. 1990 Planet. Space Sci. 38, 543546.CrossRefGoogle Scholar
[19]Kopnin, S. I., Popel, S. I. and Yu, M. Y. 2009 Phys. Plasmas 16, 063705.CrossRefGoogle Scholar
[20]Popel, S. I., Vladimirov, S. V. and Tsytovich, V. N. 1995 Phys. Rep. 259, 327405.CrossRefGoogle Scholar
[21]Shukla, P. K. and Vladimirov, S. V. 1995 Phys. Plasmas 2, 31793183.CrossRefGoogle Scholar
[22]Shukla, P. K. and Stenflo, L. 2001 IEEE Trans. Plasma Sci. 29, 267270.CrossRefGoogle Scholar
[23]Landau, L. D. and Lifshitz, E. M. 1987 Fluid Mechanics. Oxford: Pergamon.Google Scholar
[24]Hunten, D. M., Turco, R. P. and Toon, O. B. 1980 J. Atmos. Sci. 37, 13421357.2.0.CO;2>CrossRefGoogle Scholar
[25]Havnes, O., Aslaksen, T. and Brattli, A. 2001 Phys. Scripta T89, 133137.CrossRefGoogle Scholar
[26]Aburdzhaniya, G. D. 2006 Self-Organization of Vortex Structures and Vortex Turbulence in Dispersive Media [in Russian]. Moscow: KomKniga.Google Scholar
[27]Brasseur, G. and Solomon, S. 1984 Aeronomy of the Middle Atmosphere. Dordrecht, Netherland: Reidel.CrossRefGoogle Scholar
[28]Cho, J. Y. N. and Röttger, J. 1997 J. Geophys. Res. 102, 20012020.CrossRefGoogle Scholar
[29]Popel, S. I., Gisko, A. A., Golub', A. P., Losseva, T. V., Bingham, R. and Shukla, P. K. 2000 Phys. Plasmas 7, 24102416.CrossRefGoogle Scholar
[30]Nemtchinov, I. V., Shuvalov, V. V., Artemieva, N. A., Kosarev, I. B. and Popel, S. I. 2002 Intern. J. Impact Engineering 27, 521534.CrossRefGoogle Scholar
[31]Vitjazev, A. V., Pechernikova, G. V. and Safronov, V. S. 1990 Terrestrial Planets: Origin and Early Evolution[in Russian]. Moscow: Nauka.Google Scholar