Flux Emergence (Theory)

By Mark C. M. Cheung, H. Isobe. 2014

190 citations recorded by the source corpus.

Magnetic flux emergence from the solar convection zone into the overlying atmosphere is the driver of a diverse range of phenomena associated with solar activity. In this article, we introduce theoretical concepts central to the study of flux emergence and discuss how the inclusion of different physical effects (e.g., magnetic buoyancy, magnetoconvection, reconnection, magnetic twist, interaction with ambient field) in models impact the evolution of the emerging field and plasma.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/8ca0dd1a6a1ce77e6a39dd8360a5e09856ca0ecf

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. J. Thalmann
2. T. Wiegelmann
3. C. Schrijver
4. S. Solanki
5. H. Hudson
6. S. Toriumi
7. L. Harra
8. K. Nagashima

In Molecular Biology

1. J. Thalmann
2. C. Schrijver
3. T. Wiegelmann
4. S. Solanki
5. S. Toriumi
6. H. Hudson
7. L. Harra
8. T. Sakurai

Citations in the corpus

• MAGNETIC PROPERTIES OF SOLAR ACTIVE REGIONS THAT GOVERN LARGE SOLAR FLARES AND ERUPTIONS (2016, background): “…by flux emergence, the transportation of dynamo-generated magnetic flux in the deeper interior to the solar surface (Parker 1955), it is of necessity to conduct numerical simulations and model the flux emergence (Fan 2009; Cheung & Isobe 2014), which is, however, beyond the scope of this paper.”
• The magnetic field in the solar atmosphere (2014, methodology): “Outside the scope of the present review are methods of the interaction of the convection zone with the solar atmosphere by flux emergence (the interested reader can find a recent review on the theory of flux emergence in Cheung and Isobe, 2014). Methods to analyse the 3D coronal magnetic field topol”