Modeling of the halo CME propagation using ENLIL Heliospheric Cone Model

Details Modeling of the halo CME propagation using ENLIL Heliospheric Cone Model Modeling of the halo CME propagation using ENLIL Heliospheric Cone Model

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agusmsh41b..01t&link_type=abstract

American Geophysical Union, Spring Meeting 2007, abstract #SH41B-01

Computer Science

Performance

2101 Coronal Mass Ejections (7513), 2728 Magnetosheath, 2790 Substorms, 7513 Coronal Mass Ejections (2101), 7526 Magnetic Reconnection (2723, 7835)

Scientific paper

We will test the ability of the ENLIL heliospheric cone model, available at the Community Coordinated Modeling Center (CCMC) of the NASA/GSFC, to model the propagation of halo CMEs. We will use different approaches to derive CME parameters from the LASCO/C3 instrument images. We also will study the sensitivity of the model performance to parameters that can not be derived from the observations. We will simulate a number of geomagnetic storms and series of events selected by community campaigns, including the recent fall AGU storm on December 15, 2006, to study ENLIL cone model performance comparing it to the ACE satellite data. The development of such a tool at the CCMC will support the development of space weather event forecasting.

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