Initial condition influence on coronal mass ejection propagation

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

1

Interplanetary Physics: Coronal Mass Ejections (7513), Interplanetary Physics: Discontinuities (7811), Interplanetary Physics: Ejecta, Driver Gases, And Magnetic Clouds, Interplanetary Physics: Solar Wind Plasma, Solar Physics, Astrophysics, And Astronomy: Magnetic Reconnection (2723, 7835)

Scientific paper

In the melon-seed-overpressure-expansion (MSOE) model described by Siscoe et al. (2006) for the acceleration of coronal mass ejections (CMEs), magnetic repulsion force plays a central role. MSOE is a combination of Pneuman's (1984) melon seed concept with an overpressure expansion analytically formulated by Siscoe et al. (2006). The MSOE model creates a reduced formalism to describe CME acceleration and is highly advantageous for comparative studies. As originally presented, the MSOE model has the drawback of being able to produce only fast CMEs. For the work presented in this paper, we compare the acceleration of a 2.5-D magnetohydrodynamics (MHD)-modeled CME with that of a version of the MSOE model. On the basis of the results of the MHD simulations, we divide the acceleration of a CME into two phases: (1) a tethered phase before detachment (when the CME is tethered by external closed loops) and (2) a repulsion phase after detachment (when the tethering force that binds the CME is much smaller than outward magnetic repulsion force). We find that during the repulsion phase, the acceleration can be described well by the standard MSOE model. However, during the tethered phase, the CME acceleration is much slower than MSOE predictions. We therefore refine the MSOE model to include tethering and can account for both fast and slow CMEs with the final CME speed controlled by the CME detachment height.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Initial condition influence on coronal mass ejection propagation 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 Initial condition influence on coronal mass ejection propagation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Initial condition influence on coronal mass ejection propagation will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1861284

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.