Screen Shot 2015-01-23 at 3.13.53 PM.png
Earth directed ICME List  
1994
1995 Wind mission, operating during the last two decades, monitors in-situ observations critical to identify large scale solar transient events at 1 AU. ICMEs (Interplanetary Coronal Mass Ejections) have been grouped and published in different papers during this period of time at the same time the ICME features are most precisely defined.
1996
1997
1998
1999
2000 The catalogue provides the compiled list of ICME events. Information catalogued:
2001 * By year, ICME in-situ parameters: 
2002 Start/end ICME time: Start ICME time is defined by the IP forward shock or sheath signatures; End ICME time is defined by IP reverse shock, or end of magnetic obstacle.
2003
2004 Magnetic obstacle (MO) start/end time. The MO is characterized as: Flux-Rope (rotation in a magnetic field component), Flux-Rope-Like (partial rotation in a magnetic field component),Ejecta (magnetic field signatures without well defined rotation).
2005
2006
2007
2008
2009 *In-situ data plot (for e s from the Sun to the magnetosphere. ach ICME event): Magnetic field (MFI), plasma parameters (SWE).
2010
2011
2012
2013
2014
Solar Cycle 22 Solar Cycle 23 Solar Cycle 24
HSDlogo.png
Contact: Teresa Nieves-Chinchilla. Teresa.Nieves@nasa.gov. Telf. +1 301 286 8681
Collaborators:  Leila Mays  Last Update:2015/11/03
Neel Savani
Screen Shot 2015-01-23 at 3.21.04 PM.png