Coronal prominence structure and dynamics: A magnetic flux rope interpretation

By S. Gibson, Yuhong Fan. 2006

147 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/e9b5b5be790d989a983f23d2a26172c054c9f942

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. G. Aulanier
2. Brigitte Schmieder
3. Yuhong Fan
4. S. Gibson
5. T. Okamoto
6. C. Schrijver
7. T. Magara
8. A. Title

In Molecular Biology

1. S. Gibson
2. G. Aulanier
3. Yuhong Fan
4. Brigitte Schmieder
5. T. Magara
6. Y. Suematsu
7. J. Karpen
8. D. Mackay

Citations in the corpus

• Physics of Solar Prominences: II—Magnetic Structure and Dynamics (2010, background): “Such a feature has been considered in the numerical simulations of Gibson and Fan (2006) and Magara et al. (2008).”
• Onset of Coronal Mass Ejections Due to Loss of Confinement of Coronal Flux Ropes (2007, methodology): “As was found in Gibson & Fan (2006a, 2006b), in case K, a flux rope containing dipped helical field lines is left behind in the posteruption state (see the left panels of Fig.”
• QUIESCENT PROMINENCE DYNAMICS OBSERVED WITH THE HINODE SOLAR OPTICAL TELESCOPE. I. TURBULENT UPFLOW PLUMES (2010, background): “Recent MHD models have made progress in understanding the large-scale dynamics of prominences modeled as twisted flux ropes (Gibson & Fan 2006; Fan 2005; Gibson & Low 1998) showing that eruption can be understood as a threshold event following quasi-static evolution of the system through states of…”