cc.\*:("001E03B50C")
Results 1 to 25 of 710
Selection :
Electrostatic Solitary Waves in the Solar Wind: Evidence for Instability at Solar Wind Current SheetsMALASPINA, David M; NEWMAN, David L; WILLSON, Lynn B et al.Journal of geophysical research. Space physics. 2013, Vol 118, Num 2, pp 591-599, 9 p.Article
Ion temperature anisotropy instabilities in planetary magnetosheathsREMYA, B; REDDY, R. V; TSURUTANI, B. T et al.Journal of geophysical research. Space physics. 2013, Vol 118, Num 2, pp 785-793, 9 p.Article
Solar wind alpha particles and heavy ions in the inner heliosphere observed with MESSENGER : MESSENGER Views Mercury From OrbitGERSHMAN, Daniel J; ZURBUCHEN, Thomas H; FISK, Lennard A et al.Journal of geophysical research. 2012, Vol 117, Num A12, issn 0148-0227, A00M02.1-A00M02.14Article
Investigating the viscous interaction and its role in generating the ionospheric potential during the Whole Heliosphere IntervalBRUNTZ, R; LOPEZ, R. E; BHATTARAI, S. K et al.Journal of atmospheric and solar-terrestrial physics. 2012, Vol 83, pp 70-78, issn 1364-6826, 9 p.Article
Domination of heliosheath pressure by shock-accelerated pickup ions from observations of neutral atomsLINGHUA WANG; LIN, Robert P; LARSON, Davin E et al.Nature (London). 2008, Vol 454, Num 7200, pp 81-83, issn 0028-0836, 3 p.Article
A magnetic reconnection X-line extending more than 390 Earth radii in the solar windPHAN, T. D; GOSLING, J. T; BALOGH, A et al.Nature (London). 2006, Vol 439, Num 7073, pp 175-178, issn 0028-0836, 4 p.Article
Electron plasma oscillations upstream of the solar wind termination shock : Voyager 1GURNETT, D. A; KURTH, W. S.Science (Washington, D.C.). 2005, Vol 309, Num 5743, pp 2025-2027, issn 0036-8075, 3 p.Article
Voyager 1 explores the termination shock region and the heliosheath beyond : Voyager 1STONE, E. C; CUMMINGT, A. C; MCDONALD, F. B et al.Science (Washington, D.C.). 2005, Vol 309, Num 5743, pp 2017-2020, issn 0036-8075, 4 p.Article
Voyager 1 in the foreshock, termination shock, and heliosheath : Voyager 1DECKER, R. B; KRIMIGIS, S. M; ROELOF, E. C et al.Science (Washington, D.C.). 2005, Vol 309, Num 5743, pp 2020-2024, issn 0036-8075, 5 p.Article
Anisotropic wave turbulence in electron MHDGALTIER, Sébastien; BHATTACHARJEE, Amitava.Plasma physics and controlled fusion. 2005, Vol 47, Num 12B, pp B691-B701, issn 0741-3335Conference Paper
Determination of the solar wind slowdown near solar maximumWANG, C; RICHARDSON, J. D.Journal of geophysical research. 2003, Vol 108, Num A2, pp SSH1.1-SSH1.7, issn 0148-0227Article
Evidence for electrostatic decay in the solar wind at 5.2 AUTHEJAPPA, G; MACDOWALL, R. J; SCIME, E. E et al.Journal of geophysical research. 2003, Vol 108, Num A3, issn 0148-0227, SSH 9.1-SSH 9.10Article
Implications of the observed anticorrelation between solar wind speed and coronal electron temperatureGLOECKLER, George; ZURBUCHEN, Thomas H; GEISS, Johannes et al.Journal of geophysical research. 2003, Vol 108, Num A4, pp SSH8.1-SSH8.11, issn 0148-0227Article
Ulysses and beyondMARSDEN, R; SCHERER, K; HEBER, B et al.Annales geophysicae (1988). 2003, Vol 21, Num 6, issn 0992-7689, 177 p.Serial Issue
A non-force-free approach to the topology of magnetic clouds in the solar windHIDALGO, M. A; CID, C; VINAS, A. F et al.Journal of geophysical research. 2002, Vol 107, Num A1, issn 0148-0227, SSH 1.1-SSH 1.7Article
Symmetric suprathermal electron depletions on closed field lines in the solar windGOSLING, J. T; SKOUG, R. M; FELDMAN, W. C et al.Geophysical research letters. 2002, Vol 29, Num 12, pp 14.1-14.4, issn 0094-8276Article
Alfvénic turbulence in high-latitude solar wind: Radial versus latitudinal variationsBAVASSANO, B; PIETROPAOLO, E; BRUNO, R et al.Journal of geophysical research. 2002, Vol 107, Num A12, pp SSH7.1-SSH7.6, issn 0148-0227Article
Deceleration of streaming alpha particles interacting with waves and imbedded rotational discontinuitiesKAGHASHVILI, Edisher K; VASQUEZ, Bernard J; HOLLWEG, Joseph V et al.Journal of geophysical research. 2002, Vol 108, Num A1, pp SSH8.1-SSH8.17, issn 0148-0227Article
Electron heat flux instabilities in coronal holes: Implications for ion heatingMARKOVSKII, S. A; HOLLWEG, Joseph V.Geophysical research letters. 2002, Vol 29, Num 17, pp 24.1-24.4, issn 0094-8276Article
Hydrogen wall and heliosheath Ly α absorption toward nearby stars: Possible constraints on the heliospheric interface plasma flowIZMODENOV, Vlad; WOOD, Brian E; LALLEMENT, Rosine et al.Journal of geophysical research. 2002, Vol 107, Num A10, issn 0148-0227, SSH 13.1-SSH 13.15Article
The solar wind at solar maximum: comparisons of EISCAT IPS and in situ observationsBREEN, A. R; RILEY, P; LAZARUS, A. J et al.Annales geophysicae (1988). 2002, Vol 20, Num 9, pp 1291-1309, issn 0992-7689Conference Paper
Evidence for pitch angle diffusion of solar wind protons in resonance with cyclotron wavesMARSCH, E; TU, C.-Y.Journal of geophysical research. 2001, Vol 106, Num A5, pp 8357-8361, issn 0148-0227Article
Solar wind plasma parameters on Ulysses: Detailed comparison between the URAP and SWOOPS experimentsISSAUTIER, Karine; SKOUG, R. M; GOSLING, J. T et al.Journal of geophysical research. 2001, Vol 106, Num A8, pp 15665-15675, issn 0148-0227Article
Solar wind signatures associated with magnetic cloudsBLANCO-CANO, X; BRAVO, S.Journal of geophysical research. 2001, Vol 106, Num A3, pp 3691-3702, issn 0148-0227Article
Three spacecraft observations of solar wind discontinuitiesHORBURY, Timothy S; BURGESS, David; FRÄNZ, Markus et al.Geophysical research letters. 2001, Vol 28, Num 4, pp 677-680, issn 0094-8276Article