Multipoint ICME encounters: Pre-STEREO and STEREO observations
暂无分享,去创建一个
C. Russell | J. Luhmann | E. Kilpua | L. Jian | Y. Li
[1] J. Gosling. Coronal Mass Ejections and Magnetic Flux Ropes in Interplanetary Space , 2013 .
[2] L. Burlaga,et al. Global Configuration of a Magnetic Cloud , 2013 .
[3] K. Marubashi. Interplanetary Magnetic Flux Ropes and Solar Filaments , 2013 .
[4] J. Gosling. Coronal Mass Ejections: An Overview , 2013 .
[5] R. Goldstein,et al. Particle and Field Signatures of Coronal Mass Ejections in the Solar Wind , 2013 .
[6] C. Russell,et al. Comparing Solar Minimum 23/24 with Historical Solar Wind Records at 1 AU , 2011 .
[7] B. Heber,et al. Multi‐point observations of CIR‐associated energetic particles during the 2008 solar minimum , 2010 .
[8] J. Luhmann,et al. STEREO observations of interplanetary coronal mass ejections and prominence deflection during solar minimum period , 2009 .
[9] T. Howard,et al. Interplanetary Coronal Mass Ejections Observed in the Heliosphere: 3. Physical Implications , 2009 .
[10] D. Odstrcil,et al. Numerical Heliospheric Simulations as Assisting Tool for Interpretation of Observations by STEREO Heliospheric Imagers , 2009 .
[11] J. Luhmann,et al. ROTATION OF CORONAL MASS EJECTIONS DURING ERUPTION , 2009 .
[12] A. Galvin,et al. Optimized Grad – Shafranov Reconstruction of a Magnetic Cloud Using STEREO-Wind Observations , 2009 .
[13] J. Luhmann,et al. Multispacecraft recovery of a magnetic cloud and its origin from magnetic reconnection on the Sun , 2009 .
[14] C. Russell,et al. Multispacecraft Observations of Magnetic Clouds and Their Solar Origins between 19 and 23 May 2007 , 2009 .
[15] C. Russell,et al. Stream Interactions and Interplanetary Coronal Mass Ejections at 5.3 AU near the Solar Ecliptic Plane , 2008 .
[16] Y. Lin,et al. A uniform-twist magnetic flux rope in the solar wind , 2008 .
[17] E. Christian,et al. The STEREO Mission: An Introduction , 2008 .
[18] C. Russell,et al. Stream Interactions and Interplanetary Coronal Mass Ejections at 0.72 AU , 2008 .
[19] C. Russell,et al. Reconstruction of the 2007 May 22 Magnetic Cloud: How Much Can We Trust the Flux-Rope Geometry of CMEs? , 2008 .
[20] M. Temmer,et al. Two-spacecraft reconstruction of a magnetic cloud and comparison to its solar source , 2007 .
[21] R. Lepping,et al. Long-duration magnetic clouds: a comparison of analyses using torus- and cylinder-shaped flux rope models , 2007 .
[22] W. Manchester,et al. Reply to comment by P. Riley and J. T. Gosling on “Are high‐latitude forward‐reverse shock pairs driven by overexpansion?” , 2007 .
[23] P. Démoulin,et al. Progressive Transformation of a Flux Rope to an ICME , 2007, 0706.2889.
[24] C. Owen,et al. Multi-Spacecraft Study of the 21 January 2005 ICME , 2007 .
[25] J. Krall,et al. Are All Coronal Mass Ejections Hollow Flux Ropes? , 2007 .
[26] Christopher T. Russell,et al. Properties of Interplanetary Coronal Mass Ejections at One AU During 1995 – 2004 , 2006 .
[27] T. Zurbuchen,et al. In-Situ Solar Wind and Magnetic Field Signatures of Interplanetary Coronal Mass Ejections , 2006 .
[28] N. Gopalswamy,et al. On the Rates of Coronal Mass Ejections: Remote Solar and In Situ Observations , 2006 .
[29] Nat Gopalswamy,et al. Coronal mass ejections of solar cycle 23 , 2006 .
[30] J. Richardson,et al. Constraints on the global structure of magnetic clouds: Transverse size and curvature , 2006, physics/0606003.
[31] A. Vourlidas,et al. The Proper Treatment of Coronal Mass Ejection Brightness: A New Methodology and Implications for Observations , 2006 .
[32] A. Szabo,et al. A summary of WIND magnetic clouds for years 1995-2003: model-fitted parameters, associated errors and classifications , 2006 .
[33] M. Owens,et al. A kinematically distorted flux rope model for magnetic clouds , 2006 .
[34] R. Wiens,et al. Suprathermal electrons in high‐speed streams from coronal holes: Counterstreaming on open field lines at 1 AU , 2005 .
[35] H. Koskinen,et al. Properties and geoeffectiveness of magnetic clouds in the rising, maximum and early declining phases of solar cycle 23 , 2005 .
[36] Q. Hu,et al. Fitting Flux Ropes to a Global MHD Solution: A Comparison of Techniques. Appendix 1 , 2004 .
[37] I. Richardson,et al. The fraction of interplanetary coronal mass ejections that are magnetic clouds: Evidence for a solar cycle variation , 2004 .
[38] I. Richardson,et al. Identification of interplanetary coronal mass ejections at 1 AU using multiple solar wind plasma composition anomalies , 2004 .
[39] V. Bothmer,et al. On the three-dimensional configuration of coronal mass ejections , 2004 .
[40] N. Gopalswamy,et al. A catalog of white light coronal mass ejections observed by the SOHO spacecraft , 2004 .
[41] J. Richardson,et al. Interplanetary coronal mass ejections observed by Voyager 2 between 1 and 30 AU , 2004 .
[42] R. Forsyth,et al. Two examples of magnetic clouds with double rotations observed by the Ulysses spacecraft , 2004 .
[43] D. D. Zeeuw,et al. Modeling a space weather event from the Sun to the Earth: CME generation and interplanetary propagation , 2004 .
[44] J. Luhmann,et al. Solar cycle control of the magnetic cloud polarity and the geoeffectiveness , 2004 .
[45] P. Riley,et al. Kinematic Treatment of Coronal Mass Ejection Evolution in the Solar Wind , 2004 .
[46] J. Gosling,et al. Properties of high‐latitude CME‐driven disturbances during Ulysses second northern polar passage , 2003 .
[47] M. Hidalgo. A study of the expansion and distortion of the cross section of magnetic clouds in the interplanetary medium , 2003 .
[48] J. Linker,et al. Using an MHD simulation to interpret the global context of a coronal mass ejection observed by two spacecraft , 2003 .
[49] G. Aulanier,et al. Interpretation of a complex CME event: Coupling of scales in multiple flux systems , 2003 .
[50] L. Burlaga,et al. Successive CMEs and complex ejecta , 2002 .
[51] Qiang Hu,et al. Reconstruction of magnetic clouds in the solar wind: Orientations and configurations , 2002 .
[52] C. Cid,et al. Plasma and Magnetic Field Inside Magnetic Clouds: a Global Study , 2002 .
[53] B. Heber,et al. An ICME observed by Voyager 2 at 58 AU and by Ulysses at 5 AU , 2001 .
[54] E. Cliver,et al. Sources of geomagnetic storms for solar minimum and maximum conditions during 1972–2000 , 2001 .
[55] C. Russell,et al. Multispacecraft modeling of the flux rope structure of interplanetary coronal mass ejections: Cylindrically symmetric versus nonsymmetric topologies , 2001 .
[56] J. Richardson,et al. Voyager 2 observations of helium abundance enhancements from 1–60 AU , 2001 .
[57] Russell A. Howard,et al. Properties of coronal mass ejections: SOHO LASCO observations from January 1996 to June 1998 , 2000 .
[58] Barbara June Thompson,et al. Relationship of halo coronal mass ejections, magnetic clouds, and magnetic storms , 2000 .
[59] C. Russell,et al. Intercomparison of NEAR and Wind interplanetary coronal mass ejection observations , 1999 .
[60] J. Luhmann,et al. Solar cycle evolution of the structure of magnetic clouds in the inner heliosphere , 1998 .
[61] J. Gosling,et al. Overexpanding coronal mass ejections at high heliographic latitudes: Observations and simulations , 1998 .
[62] V. Bothmer,et al. The structure and origin of magnetic clouds in the solar wind , 1997 .
[63] N. Crooker,et al. A magnetic cloud as a distended flux rope occlusion in the heliospheric current sheet , 1996 .
[64] L. Burlaga,et al. Magnetic flux rope versus the spheromak as models for interplanetary magnetic clouds , 1995 .
[65] J. Phillips,et al. A CME-driven solar wind disturbance observed at both low and high heliographic latitudes , 1995 .
[66] M. Vandas,et al. Evidence for a spheroidal structure of magnetic clouds , 1993 .
[67] M. Vandas,et al. Spheroidal models of magnetic clouds and their comparison with spacecraft measurements , 1993 .
[68] J. Phillips,et al. Counterstreaming solar wind halo electron events : solar cycle variations , 1992 .
[69] L. Burlaga,et al. Magnetic field structure of interplanetary magnetic clouds at 1 AU , 1990 .
[70] K. G. Ivanov,et al. Configuration, structure, and dynamics of magnetic clouds from solar flares in light of measurements on board Vega 1 and Vega 2 in January–February 1986 , 1989 .
[71] L. Burlaga,et al. Magnetic clouds and force‐free fields with constant alpha , 1988 .
[72] D. Baker,et al. Bidirectional solar wind electron heat flux events , 1987 .
[73] H. Goldstein. On the field configuration in magnetic clouds , 1983 .
[74] F. Mariani,et al. Magnetic loop behind an interplanetary shock: Voyager, Helios and IMP-8 observations , 1981 .
[75] P. Caloi. Interazioni Ira atmosfera ed idrosfera , 1963 .
[76] C. Russell,et al. Evolution of solar wind structures from 0.72 to 1 AU , 2008 .
[77] J. Richardson,et al. ICMES at very large distances , 2006 .
[78] P. Démoulin,et al. Large scale MHD properties of interplanetary magnetic clouds , 2005 .
[79] John W. Belcher,et al. A statistical study of the properties of interplanetary coronal mass ejections from 0.3 to 5.4 AU , 2005 .
[80] M. Vandas,et al. Magnetic clouds of oblate shapes , 2005 .
[81] C. Russell,et al. A new parameter to define interplanetary coronal mass ejections , 2005 .
[82] C. Russell,et al. The true dimensions of interplanetary coronal mass ejections , 2002 .
[83] C. Cid,et al. A non‐force‐free approach to the topology of magnetic clouds in the solar wind , 2002 .
[84] N. Sidiropoulos,et al. Study of CME structure and evolution deduced from ULYSSES/HI-SCALE energetic particle observations , 2000 .
[85] C. Russell,et al. Physics of magnetic flux ropes. Geophysical Monograph, No. 58 , 1990 .
[86] K. Marubashi. Structure of the interplanetary magnetic clouds and their solar origins , 1986 .