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Reconnection in a weakly stochastic field
We examine the effect of weak, small-scale magnetic field structure on the rate of
reconnection in a strongly magnetized plasma. This affects the rate of reconnection by …
reconnection in a strongly magnetized plasma. This affects the rate of reconnection by …
Estudio de la inestabilidad tipo tearing en plasmas colisionales
LF Moreno Mosquera - 2024 - repository.eia.edu.co
Reconnection in photospheric-chromospheric current sheet and coronal heating
It has been observed by various ground and space based solar missions that magnetic
reconnection occurs frequently in the photosphere-chromosphere region as well as in the …
reconnection occurs frequently in the photosphere-chromosphere region as well as in the …
Reconnection via the tearing instability
We discuss the role of tearing instabilities in magnetic reconnection. In three dimensions this
instability leads to the formation of strong Alfvenic waves that remove plasma efficiently from …
instability leads to the formation of strong Alfvenic waves that remove plasma efficiently from …
Forced MHD turbulence simulations for coronal loop heating
Z Romeou, M Velli, G Einaudi - AIP Conference Proceedings, 2006 - pubs.aip.org
In this work we revisit the question of whether the assumption of a turbulent photosphere
provides an efficient mechanism for the disposition of energy in the solar corona. Through a …
provides an efficient mechanism for the disposition of energy in the solar corona. Through a …
[KIRJA][B] Equilibrium and stability of coronal helmet streamers
VS Glukhov - 1997 - search.proquest.com
from any type of computer printer. Page 1 INFORMATION TO USERS This manuscript has
been reproduced from the microfilm master. UMI films the text directly from the original or copy …
been reproduced from the microfilm master. UMI films the text directly from the original or copy …
[HTML][HTML] A Reduced MHD Turbulence Numerical Approach On Coronal Loop Heating: Deriving Scaling Laws
Z Romeou, M Velli, G Einaudi - Second Solar Orbiter Workshop, 2007 - adsabs.harvard.edu
We have carried out incompressible 2D Reduced MHD simulations to extensively
investigate the long time statistical behavior of a coronal loop subject to magnetic forcing …
investigate the long time statistical behavior of a coronal loop subject to magnetic forcing …