z-logo
open-access-imgOpen Access
Experimental Demonstration of How Strapping Fields Can Inhibit Solar Prominence Eruptions
Author(s) -
J. F. Hansen,
Paul M. Bellan
Publication year - 2001
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/338736
Subject(s) - strapping , physics , magnetic field , field (mathematics) , solar prominence , scale (ratio) , mechanical engineering , engineering , mathematics , quantum mechanics , pure mathematics
It has been conjectured that the eruption of a solar prominence can be inhibited if a much larger scale, arched magnetic field straddles the prominence,and effectively straps it down. We have demonstrated,this effect in a laboratory experiment where,a vacuum,strapping field acts on a scaled simulation of a solar prominence. The required magnitude,of the strapping field is in good agreement,with a theoretical model that takes into account the full three-dimensional magnetic topology. Subject headings: methods: laboratory — MHD — plasmas — Sun: flares — Sun: magnetic fields — Sun: prominences 1. BACKGROUND Solar prominences are large, arched plasma structures pro-

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom