kw.\*:("Plasma interplanetario")
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A computerized complex for observation of scintillating sourcesISAEV, E. A; LAPAEV, K. A; TYUL'BASHEV, S. A et al.Radiophysics and quantum electronics. 1997, Vol 40, Num 5, pp 392-394, issn 0033-8443Article
A numerical study of the evolution of the solar wind from Ulysses to Voyager 2WANG, C; RICHARDSON, J. D; GOSLING, J. T et al.Journal of geophysical research. 2000, Vol 105, Num A2, pp 2337-2344, issn 0148-0227Article
Comment on «a new method fo forecasting geomagnetic activity and protons showers» by A. Hewish and P.J. Duffet-SmithTSURUTANI, B. T; GOLDSTEIN, B. E; GONZALEZ, W. D et al.Planetary and space science. 1988, Vol 36, Num 2, pp 205-206, issn 0032-0633Article
A density and current plasma wave antennaKELLOGG, P. J; GOETZ, K; MONSON, S. J et al.Journal of geophysical research. 1999, Vol 104, Num A6, pp 12627-12635, issn 0148-0227Article
Interstellar pickup protons at pressure-balanced structuresISENBERG, P. A.JGR. Journal of geophysical research. Part A, Space physics. 1991, Vol 96, Num 1, pp 155-159, 5 p.Article
Particle and field signatures of coronal mass ejections in the solar windNEUGEBAUER, M; GOLDSTEIN, R.Geophysical monograph. 1997, Vol 99, pp 245-251, issn 0065-8448Article
Some current challenges in space plasma physicsRYCROFT, M. J.Radiophysics and quantum electronics. 1996, Vol 39, Num 1, pp 3-17, issn 0033-8443Article
The inertial-range spectrum of fully developed magnetohydrodynamic turbulenceCARBONE, V.Annales geophysicae (1988). 1993, Vol 11, Num 9, pp 866-868, issn 0992-7689Article
Shock drift mechanism for forbush decreasesCHENG, A. F; SARRIS, E. T; DODOPOULOS, C et al.The Astrophysical journal. 1990, Vol 350, Num 1, pp 413-418, issn 0004-637X, 1Article
A revised shock time of arrival (STOA) model for interplanetary shock propagation: STOA-2MOON, Y.-J; DRYER, M; SMITH, Z et al.Geophysical research letters. 2002, Vol 29, Num 10, pp 28.1-28.4, issn 0094-8276Article
Dust-magnetosonic modes in planetary ringsVERHEEST, Frank; HELLBERG, Manfred A.IEEE transactions on plasma science. 2001, Vol 29, Num 2, pp 283-287, issn 0093-3813Article
Ion acoustic damping effects on parametric decays of Alfvén wavesGOMBEROFF, L.Journal of geophysical research. 2000, Vol 105, Num A5, pp 10509-10518, issn 0148-0227Article
Solar wind plasma correlations between IMP 8, INTERBALL-1, and WINDPAULARENA, K. I; ZASTENKER, G. N; LAZARUS, A. J et al.Journal of geophysical research. 1998, Vol 103, Num A7, pp 14601-14617, issn 0148-0227Article
Ulysses observations of a density hole in the high-speed solar windRILEY, P; GOSLING, J. T; MCCOMAS, D. J et al.Journal of geophysical research. 1998, Vol 103, Num A2, pp 1933-1940, issn 0148-0227Article
What causes the variations of the peak intensity of CIR accelerated energetic ion fluxes?KEPPLER, E.Annales geophysicae (1988). 1998, Vol 16, Num 12, pp 1552-1556, issn 0992-7689Conference Paper
Solar cycle changes in the level of compressive microturbulence near the SunCOLES, W. A; GRALL, R. R; KLINGLESMITH, M. T et al.Journal of geophysical research. 1995, Vol 100, Num A9, pp 17069-17079, issn 0148-0227Article
Evolution of the Alvénic correlation in the solar windBRUNO, R; BAVASSANO, B.Nuovo cimento della società italiana di fisica. C. 1992, Vol 15, Num 5, pp 599-605, issn 0390-5551Conference Paper
Helios spacecraft photometer observation of elongated corotating structures in the interplanetary mediumJACKSON, B. V.JGR. Journal of geophysical research. Part A, Space physics. 1991, Vol 96, Num 7, pp 11.307-11.318Article
Physical reasons and consequences of a three-dimensionally structured heliosphereFAHR, H.-J; FICHTNER, H.Space science reviews. 1991, Vol 58, Num 3-4, pp 193-258, issn 0038-6308Article
The interstellar wind as a cause for longitudinal solar wind asymmetriesFAHR, H. J; FICHTNER, H; NEUTSCH, W et al.Planetary and space science. 1990, Vol 38, Num 3, pp 383-394, issn 0032-0633Article
A user's guide to scintillationHEWISH, A.Journal of atmospheric and terrestrial physics. 1989, Vol 51, Num 9-10, pp 743-750, issn 0021-9169, 8 p.Article
Evolution on interplanetary slow shocksWHANG, Y. C.JGR. Journal of geophysical research. Part A, Space physics. 1988, Vol 93, Num 1, pp 251-255Article
The Structure and Dynamics of the Corona-Heliosphere ConnectionANTIOCHOS, Spiro K; LINKER, Jon A; LIONELLO, Roberto et al.Space science reviews. 2012, Vol 172, Num 1-4, pp 169-185, issn 0038-6308, 17 p.Article
Type II radio emission predictions : Sources of coronal and interplanetary spectral structureKNOCK, S. A; CAIRNS, Iver H.Journal of geophysical research. 2005, Vol 110, Num A1, pp A01101.1-A01101.13, issn 0148-0227Article
The Martian plasma environment: Electric field and Langmuir probe diagnosticsBLOMBERG, Lars G; CUMNOCK, Judy A; ERIKSSON, Anders I et al.IEEE transactions on plasma science. 2003, Vol 31, Num 6, pp 1232-1236, issn 0093-3813, 5 p., 1Article