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A Magnetofrictional model for the solar corona
Published online by Cambridge University Press: 27 November 2018
Abstract
Regular reconstruction of global solar corona constrained by observational data is required to monitor the space weather variations. We develop a model for simulating the global coronal magnetic field using magnetofrictional approach. Here we perform simulations to study the evolution of the magnetic field associated with a bipolar active region in response to photospheric flows.
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- Copyright © International Astronomical Union 2018