Near-Earth Interplanetary Coronal Mass Ejections During Solar Cycle 23 (1996 – 2009): Catalog and Summary of Properties
暂无分享,去创建一个
[1] I. Richardson,et al. A study of solar energetic particle events of 1997–2006: Their composition and associations , 2010 .
[2] Alan J. Lazarus,et al. The solar wind helium abundance: Variation with wind speed and the solar cycle , 2001 .
[3] Menghua Wang,et al. Study of the Sea‐Viewing Wide Field‐of‐View Sensor (SeaWiFS) aerosol optical property data over ocean in combination with the ocean color products , 2005 .
[4] Ezequiel Echer,et al. Interplanetary conditions causing intense geomagnetic storms (Dst ≤ −100 nT) during solar cycle 23 (1996–2006) , 2008 .
[5] H. Rosenbauer,et al. Singly‐ionized helium in the driver gas of an interplanetary shock wave , 1980 .
[6] P. Démoulin,et al. Global and local expansion of magnetic clouds in the inner heliosphere , 2012, 1206.1112.
[7] S. Lepri,et al. Iron Charge Distribution as an Identifier of Interplanetary Coronal Mass Ejections , 2001 .
[8] C. Russell,et al. A new parameter to define interplanetary coronal mass ejections , 2005 .
[9] Hilary V. Cane,et al. An Introduction to CMEs and Energetic Particles , 2006 .
[10] J. Richardson,et al. Propagation of the October/November 2003 CMEs through the heliosphere , 2005 .
[11] N. Gopalswamy. Properties of Interplanetary Coronal Mass Ejections , 2007 .
[12] V. Bothmer,et al. The structure and origin of magnetic clouds in the solar wind , 1997 .
[13] G. Kanbach,et al. A 154-day periodicity in the occurrence of hard solar flares? , 1984, Nature.
[14] Bojan Vršnak,et al. Influence of the aerodynamic drag on the motion of interplanetary ejecta , 2002 .
[15] I. Richardson,et al. A 22-year dependence in the size of near-ecliptic corotating cosmic ray depressions during five solar minima , 1999 .
[16] R. Lepping,et al. Comparison of the Characteristics of Magnetic Clouds and Magnetic Cloud-Like Structures for the Events of 1995 – 2003 , 2007 .
[17] Andrew Wilson. Solar variability as an input to the Earth's environment , 2003 .
[18] J. T. Gosling,et al. Helium abundance enhancements in the solar wind , 1982 .
[19] Y. Lou. Rossby-Type Wave-Induced Periodicities in Flare Activities and Sunspot Areas or Groups during Solar Maxima , 2000 .
[20] Chang Liu,et al. The May 13, 2005 Eruption: Observations, Data Analysis and Interpretation , 2006 .
[21] W. Gonzalez,et al. The association of coronal mass ejections with their effects near the Earth , 2005 .
[22] David A. Benson,et al. Lagrangian simulation of multidimensional anomalous transport at the MADE site , 2008 .
[23] R. Goldstein,et al. Features observed in the trailing regions of interplanetary clouds from coronal mass ejections , 1997 .
[24] W. Feldman,et al. He+ and other unusual ions in the solar wind: A systematic search covering 1972–1980 , 1982 .
[25] I. Richardson,et al. Identification of interplanetary coronal mass ejections at 1 AU using multiple solar wind plasma composition anomalies , 2004 .
[26] N. Gopalswamy,et al. Predicting the 1‐AU arrival times of coronal mass ejections , 2001 .
[27] J. Geiss,et al. Unusual composition of the solar wind in the 2–3 May 1998 CME observed with SWICS on ACE , 1999 .
[28] C. Russell,et al. ON DEFINING INTERPLANETARY CORONAL MASS EJECTIONs FROM FLUID PARAMETERS , 2005 .
[29] A. Reinard. Analysis of Interplanetary Coronal Mass Ejection Parameters as a Function of Energetics, Source Location, and Magnetic Structure , 2008 .
[30] Jie Zhang,et al. Interplanetary origin of multiple‐dip geomagnetic storms , 2008 .
[31] S. Bame,et al. Solar flares and solar wind helium enrichments: July 1965–July 1967 , 1972 .
[32] W. Feldman,et al. Observations of large fluxes of He/+/ in the solar wind following an interplanetary shock , 1980 .
[33] H. Cane,et al. A survey of interplanetary coronal mass ejections in the near-Earth solar wind during 1996-2002 , 2003 .
[34] Victor J. Pizzo,et al. Anomalously low proton temperatures in the solar wind following interplanetary shock waves—evidence for magnetic bottles? , 1973 .
[35] I. Richardson. A Survey of Bidirectional >= 1 MeV Ion Flows during the HELIOS 1 and HELIOS 2 Missions: Observations from the Goddard Space Flight Center Instruments , 1994 .
[36] Ian G. Richardson,et al. Regions of abnormally low proton temperature in the solar wind (1965–1991) and their association with ejecta , 1995 .
[37] J. Zhang,et al. Multiple‐step geomagnetic storms and their interplanetary drivers , 2008 .
[38] I. Richardson,et al. Bidirectional about 1 MeV/amu ion intervals in 1973-1991 observed by the Goddard Space Flight Center instruments on IMP 8 and ISEE 3/ICE , 1993 .
[39] H. Koskinen,et al. Properties and geoeffectiveness of magnetic clouds in the rising, maximum and early declining phases of solar cycle 23 , 2005 .
[40] Christopher T. Russell,et al. Properties of Interplanetary Coronal Mass Ejections at One AU During 1995 – 2004 , 2006 .
[41] P. Démoulin,et al. Expected in Situ Velocities from a Hierarchical Model for Expanding Interplanetary Coronal Mass Ejections , 2008 .
[42] Nat Gopalswamy,et al. Arrival time of halo coronal mass ejections in the vicinity of the Earth , 2004 .
[43] I. Richardson,et al. A simple concept for modeling cosmic ray modulation in the inner heliosphere , 2002 .
[44] L. Burlaga,et al. Fast ejecta during the ascending phase of solar cycle 23: ACE observations, 1998-1999 , 2001 .
[45] S. Owocki,et al. The solar wind ionization state as a coronal temperature diagnostic , 1983 .
[46] Robert L. Tokar,et al. A prolonged He+ enhancement within a coronal mass ejection in the solar wind , 1999 .
[47] G. Siscoe,et al. Characteristic magnetic field and speed properties of interplanetary coronal mass ejections and their sheath regions , 2005 .
[48] S. Lepri,et al. Iron charge state distributions as an indicator of hot ICMEs: Possible sources and temporal and spatial variations during solar maximum , 2004 .
[49] L. Burlaga,et al. Interplanetary magnetic clouds at 1 AU , 1982 .
[50] I. Richardson,et al. Signatures of shock drivers in the solar wind and their dependence on the solar source location , 1993 .
[51] R. Mewaldt,et al. Role of flares and shocks in determining solar energetic particle abundances , 2006 .
[52] Enhanced Rieger-type periodicities' detection in X-ray solar flares and statistical validation of Rossby waves' existence , 2008 .
[53] F. Mcdonald,et al. Composition of Solar Energetic Particles , 1975 .
[54] H. Cane. The large-scale structure of flare-associated interplanetary shocks , 1988 .
[55] J. Gosling,et al. Counterstreaming electrons in magnetic clouds , 2000 .
[56] J. Ballester,et al. MAGNETIC ROSSBY WAVES IN THE SOLAR TACHOCLINE AND RIEGER-TYPE PERIODICITIES , 2009, 0911.4591.
[57] I. Richardson,et al. Particle flows observed in ejecta during solar event onsets and their implication for the magnetic field topology , 1996 .
[58] J. Lean. Evolution of the 155 Day Periodicity in Sunspot Areas during Solar Cycles 12 to 21 , 1990 .
[59] A. Hundhausen,et al. Ionization state of the interplanetary plasma , 1968 .
[60] H. Cane,et al. The ∼150 day quasi‐periodicity in interplanetary and solar phenomena during cycle 23 , 2005 .
[61] Ian G. Richardson,et al. Energetic Particles and Corotating Interaction Regions in the Solar Wind , 2004 .
[62] T. Zurbuchen,et al. In-Situ Solar Wind and Magnetic Field Signatures of Interplanetary Coronal Mass Ejections , 2006 .
[63] W. C. Erickson,et al. Solar flares, type III radio bursts, coronal mass ejections, and energetic particles , 2002 .
[64] O. S. St. Cyr,et al. Coronal mass ejections, interplanetary ejecta and geomagnetic storms , 2000 .
[65] A. N. Zhukov,et al. Major geomagnetic storms (Dst<=-100~nT) generated by corotating interaction regions in 1996--2004 , 2006 .
[66] Jie Zhang,et al. Solar and interplanetary sources of major geomagnetic storms (Dst ≤ −100 nT) during 1996–2005 , 2007 .
[67] J. Richardson,et al. Characteristics of the interplanetary coronal mass ejections in the heliosphere between 0.3 and 5.4 AU , 2005 .
[68] J. Gosling,et al. The eastward deflection of fast coronal mass ejecta in interplanetary space , 1987 .
[69] T. Horbury,et al. ICMEs in the Inner Heliosphere: Origin, Evolution and Propagation Effects , 2006 .
[70] R. H. Becker,et al. Elemental Abundances of the Bulk Solar Wind: Analyses from Genesis and ACE , 2007 .
[71] N. Gopalswamy,et al. Interplanetary acceleration of coronal mass ejections , 2000 .
[72] T. Sanderson,et al. Energetic Particle Observations , 2006 .
[73] Hui Wang,et al. A regional climate model study of how biomass burning aerosol impacts land-atmosphere interactions over the Amazon , 2008 .
[74] I. Richardson,et al. The fraction of interplanetary coronal mass ejections that are magnetic clouds: Evidence for a solar cycle variation , 2004 .
[75] Chang Liu,et al. The Eruption from a Sigmoidal Solar Active Region on 2005 May 13 , 2007, 0707.2240.
[76] John W. Belcher,et al. A statistical study of the properties of interplanetary coronal mass ejections from 0.3 to 5.4 AU , 2005 .
[77] C. Torrence,et al. A Practical Guide to Wavelet Analysis. , 1998 .
[78] L. Burlaga,et al. Successive CMEs and complex ejecta , 2002 .
[79] I. Richardson,et al. Cosmic ray decreases and shock structure: A multispacecraft study , 1994 .
[80] A. Galvin,et al. Consequences of the force-free model of magnetic clouds for their heliospheric evolution , 2007 .
[81] D. Baker,et al. Bidirectional solar wind electron heat flux events , 1987 .
[82] P. Bochsler. Abundances and charge states of particles in the solar wind , 2000 .
[83] C. Farrugia,et al. Solar‐cycle variation of low density solar wind during more than three solar cycles , 2000 .
[84] J. Zhang,et al. Sizes and relative geoeffectiveness of interplanetary coronal mass ejections and the preceding shock sheaths during intense storms in 1996–2005 , 2008, Geophysical Research Letters.
[85] A. Reinard. Comparison of Interplanetary CME Charge State Composition with CME-associated Flare Magnitude , 2005 .
[86] Yuming Wang,et al. A statistical study on the geoeffectiveness of Earth‐directed coronal mass ejections from March 1997 to December 2000 , 2002 .
[87] J. Steinberg,et al. Solar Wind Helium Abundance as a Function of Speed and Heliographic Latitude: Variation through a Solar Cycle , 2007 .
[88] H. Cane. Coronal Mass Ejections and Forbush Decreases , 2000 .
[89] G. Gloeckler,et al. Investigation of the composition of solar and interstellar matter using solar wind and pickup ion measurements with SWICS and SWIMS on the ACE spacecraft , 1998 .
[90] L. Lanzerotti,et al. October/November 2003 interplanetary coronal mass ejections: ACE/EPAM solar energetic particle observations , 2005 .
[91] T. T. von Rosenvinge,et al. The role of interplanetary shocks in the longitude distribution of solar energetic particles , 1988 .