A Parametric Survey of the CME Triggering Process by Numerical Simulations

Details A Parametric Survey of the CME Triggering Process by Numerical Simulations A Parametric Survey of the CME Triggering Process by Numerical Simulations

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005chjaa...5..636x&link_type=abstract

Chinese Journal of Astronomy and Astrophysics, Volume 5, Issue 6, pp. 636-644 (2005).

Astronomy and Astrophysics

Astrophysics

5

Scientific paper

Observations indicate that solar coronal mass ejections (CMEs) are closely associated with reconnection-favored flux emergence, which was explained in the emerging flux trigger mechanism for CMEs by Chen & Shibata based on numerical simulations. We present a parametric survey of the triggering agent: its polarity orientation, position, and the amount of the unsigned flux. The results suggest that whether a CME can be triggered depends on both the amount and location of the emerging flux, in addition to its polarity orientation. A diagram is presented to show the eruption and non-eruption regimes in the parameter space. The work is aimed at providing useful information for the space weather forecast.

Affiliated with

Also associated with

No associations

Rating

A Parametric Survey of the CME Triggering Process by Numerical Simulations 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 A Parametric Survey of the CME Triggering Process by Numerical Simulations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Parametric Survey of the CME Triggering Process by Numerical Simulations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1037719