Session - The role of Interplanetary Coronal Mass Ejections in Space Weather

Luciano Rodriguez, Sergio Dasso

The study of Interplanetary Coronal Mass Ejections (ICMEs) has advanced greatly in the last few years thanks to multispacecraft observations and high performance numerical MHD simulations. The comparisons between models and observations are clarifying several problems, such as the effects of the ambient solar wind on their propagation and internal configuration, the link between ICMEs and non-thermal energetic particles in the heliosphere (solar, interplanetary, and galactic origin), etc. In this session we invite contributions based on models and/or observations of ICMEs, which can cover the ICME propagation in the heliosphere, the interaction of ICMEs with Earth and/or with other planets, the effects of ICMEs on energetic particles, as well as on other general topics linked with ICMEs in the heliosphere.

Tuesday November 24, 11:00 - 13:00, Permeke

Poster Viewing
Tuesday November 24, 10:00 - 11:00, Poster area

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Talks : Time schedule

Tuesday November 24, 11:00 - 13:00, Permeke
11:00Interplanetary shocks and space weatherDal lago, A et al.Invited Oral
11:30Solar radio observations as a tool to forecast the arrival of coronal mass ejections near Earth ? Klein, K et al.Oral
11:45Propagation of the 7 January 2014 CME and Resulting Geomagnetic Non-EventMays, M et al.Oral
12:00Analysis of CMEs-ICMEs on the ascending phase of SC24Mierla, M et al.Oral
12:15Analysis of CME arrival times at 1 AU with neural networkSudar, D et al.Oral
12:30Lagrangian MHD Particle-in-Cell simulations of coronal interplanetary shocks driven by observationsBacchini, F et al.Oral
12:45Automatic detection of CMEs in STEREO-HI dataRodriguez, L et al.Oral


Tuesday November 24, 10:00 - 11:00, Poster area
1Study of energy input into the magnetosphere during SC23 intense geomagnetic stormsBesliu-ionescu, D et al.e-Poster
2IMF disturbances and ICMEs over 5 solar cyclesVennerstrom, S et al.e-Poster
3Geoeffective ICMEs Propagation Properties Ontiveros, V et al.p-Poster
4Predicting in-situ transits of plasma sheaths and shock arrivals associated to fast halo CMEsCorona-romero, P et al.p-Poster
5Geoeffectiveness of Disk Centre Full Halo Coronal Mass Ejections During 1996-2014Ameri, D et al.p-Poster
6Geo-efficiency of solar wind flows during 24th solar cycleShugay, Y et al.p-Poster
9False alarms of geomagnetic storms triggered by halo coronal mass ejections.Leer, K et al.p-Poster