Arrival time of solar eruptive CMEs associated with ICMEs of magnetic cloud and ejecta
暂无分享,去创建一个
[1] M. Dryer,et al. Current status of CME/shock arrival time prediction , 2014 .
[2] B. Vršnak,et al. Transit Time of Coronal Mass Ejections under Different Ambient Solar Wind Conditions , 2014 .
[3] N. Gopalswamy,et al. Testing the empirical shock arrival model using quadrature observations , 2013, 1310.8510.
[4] P. Hess,et al. A Comparative Study of Coronal Mass Ejections with and Without Magnetic Cloud Structure near the Earth: Are All Interplanetary CMEs Flux Ropes? , 2013 .
[5] N. Gopalswamy,et al. Near-Sun Flux-Rope Structure of CMEs , 2012, 1212.1409.
[6] Y. Moon,et al. Propagation Characteristics of CMEs Associated with Magnetic Clouds and Ejecta , 2012 .
[7] G. Michałek. Dynamics of CMEs in the LASCO Field of View – Statistical Analysis , 2012 .
[8] P. K. Manoharan,et al. Coronal Mass Ejections - Propagation Time and Associated Internal Energy , 2010, 1011.3687.
[9] C. Möstl,et al. The role of aerodynamic drag in propagation of interplanetary coronal mass ejections , 2010 .
[10] N. Gopalswamy,et al. INTERPLANETARY SHOCKS LACKING TYPE II RADIO BURSTS , 2009, 0912.4719.
[11] G. Michałek. Is the Asymmetric Cone Model for Halo Coronal Mass Ejections Correct? , 2010 .
[12] Haimin Wang,et al. CME Earthward Direction as an Important Geoeffectiveness Indicator , 2008 .
[13] Y. Moon,et al. Prediction of the 1-AU arrival times of CME-associated interplanetary shocks: Evaluation of an empirical interplanetary shock propagation model , 2007 .
[14] P. K. Manoharan,et al. Evolution of Coronal Mass Ejections in the Inner Heliosphere: A Study Using White-Light and Scintillation Images , 2006 .
[15] W. Gonzalez,et al. The association of coronal mass ejections with their effects near the Earth , 2005 .
[16] N. Gopalswamy,et al. A catalog of white light coronal mass ejections observed by the SOHO spacecraft , 2004 .
[17] Kenneth G. Powell,et al. Three‐dimensional MHD simulation of a flux rope driven CME , 2004 .
[18] Mathew J. Owens,et al. Predictions of the arrival time of Coronal Mass Ejections at 1AU: an analysis of the causes of errors , 2004 .
[19] Bojan Vršnak,et al. Influence of the aerodynamic drag on the motion of interplanetary ejecta , 2002 .
[20] Nat Gopalswamy,et al. An empirical model to predict the 1-AU arrival of interplanetary shocks , 2002 .
[21] N. Gopalswamy,et al. Predicting the 1‐AU arrival times of coronal mass ejections , 2001 .
[22] L. Burlaga,et al. Fast ejecta during the ascending phase of solar cycle 23: ACE observations, 1998-1999 , 2001 .
[23] P. Lamy,et al. The Large Angle Spectroscopic Coronagraph (LASCO) , 1995 .
[24] A. Hundhausen,et al. Sizes and locations of coronal mass ejections - SMM observations from 1980 and 1984-1989 , 1993 .
[25] F. Mariani,et al. Magnetic loop behind an interplanetary shock: Voyager, Helios and IMP-8 observations , 1981 .