Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1043..291p&link_type=abstract
EXPLORING THE SOLAR SYSTEM AND THE UNIVERSE. AIP Conference Proceedings, Volume 1043, pp. 291-297 (2008).
Astronomy and Astrophysics
Astronomy
Chromosphere, Interstellar Medium And Nebulae In External Galaxies, Convection, Turbulence, And Diffusion, Artificial Earth Satellites, Astronomical Observations, Asteroids, Meteoroids
Scientific paper
We present recent developments in the mathematical modeling and numerical simulations of the initiation and interplanetary evolution of CMEs in the framework of ideal magneto-hydrodynamics (MHD). In earlier work, we reconstructed simple, axisymmetric (2.5D) solar wind models for the quiet Sun. Next, we mimicked fast CME events by superposing high-density plasma blobs on the background wind and launching them in a given direction at a certain speed, enabling the study of the evolution of the fast CME shocks, their effects on the coronal field and background solar wind. Here, more realistic CME onset models are presented to investigate the possible role of magnetic foot point shearing and magnetic flux emergence/disppearence as triggering mechanisms of the instability. In particular, the well-known breakout model has been superposed on a solar wind model and it is shown that both foot point shearing and magnetic flux emergence can be used as a triggering mechanism in this model.
Jacobs Carla
Poedts Stefaan
Soenen Alexander
van der Hoist B.
Zuccarello F. P.
No associations
LandOfFree
Magnetic flux emergence and shearing motions as CME trigger mechanisms does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Magnetic flux emergence and shearing motions as CME trigger mechanisms, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magnetic flux emergence and shearing motions as CME trigger mechanisms will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1292748