Concepedia

A first step in reconstructing the solar corona self-consistently with a magnetohydrostatic model during solar activity minimum

Panpan Ruan, T. Wiegelmann, B. Inhester, T. Neukirch, S. K. Solanki, Li Feng

Astronomy and Astrophysics · 2008 · 45 citations · 62 references

DOIFull text

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Concepts

Abstract

Aims. We compute the distribution of the magnetic field and the plasma in the global corona with a self-consistent magnetohydrostatic (MHS) model.

References

62

Dynamics of the quiescent solar corona

R. Rosner, W. H. Tucker, G. S. Vaiana · The Astrophysical Journal · 1978 · 1.4K citations · Full text

, , +16

A Model for Solar Coronal Mass Ejections

The Astrophysical Journal · 1999 · 1.4K citations · Full text

, , +17

A Model for Solar Coronal Mass Ejections

Defense Technical Information Center (DTIC) · 1999 · 876 citations

, , +17

An Optimization Approach to Reconstructing Force‐free Fields

M. S. Wheatland, P. A. Sturrock, G. Roumeliotis · The Astrophysical Journal · 2000 · 496 citations

, , +13

Optimization code with weighting function for the reconstruction of coronal magnetic fields

Solar Physics · 2004 · 483 citations · Full text

, , +4