Numerical Magnetohydrodynamic Model of Dark Filament Eruption and Arcade Flaring

Details Numerical Magnetohydrodynamic Model of Dark Filament Eruption and Arcade Flaring Numerical Magnetohydrodynamic Model of Dark Filament Eruption and Arcade Flaring

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999spro.proc..403h&link_type=abstract

Solar Physics with Radio Observations, Proceedings of the Nobeyama Symposium, held in Kiyosato, Japan, Oct. 27-30, 1998, Edited

Physics

Scientific paper

We performed 2.5 dimensional magnetohydrodynamics numerical simulation
based on the quadruple magnetic source model(Uchida 1980) to explain the
dark filament eruption and the following arcade flaring consistently.

Affiliated with

Also associated with

No associations

Rating

Numerical Magnetohydrodynamic Model of Dark Filament Eruption and Arcade Flaring 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 Numerical Magnetohydrodynamic Model of Dark Filament Eruption and Arcade Flaring, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Numerical Magnetohydrodynamic Model of Dark Filament Eruption and Arcade Flaring will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1062357