COEXISTING FLUX ROPE AND DIPPED ARCADE SECTIONS ALONG ONE SOLAR FILAMENT

By Yang Guo, Brigitte Schmieder, P. Démoulin, T. Wiegelmann, G. Aulanier, Tibor Török, V. Bommier. 2010

137 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/9dc5e313fb6e244c81b0ac1c169e32dd0eed01ee

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In Astronomy and Astrophysics

1. G. Aulanier
2. Brigitte Schmieder
3. P. Démoulin
4. Xin Cheng
5. M. Ding
6. J. Zhang
7. Yang Liu
8. S. Saar

Citations in the corpus

• OBSERVING FLUX ROPE FORMATION DURING THE IMPULSIVE PHASE OF A SOLAR ERUPTION (2011, background): “Through nonlinear force-free field models, several authors were able to reconstruct a flux rope configuration in the corona from observed photospheric magnetic fields (e.g., Canou et al. 2009; Guo et al. 2010; Cheng et al. 2010b).”
• DIFFERENTIAL EMISSION MEASURE ANALYSIS OF MULTIPLE STRUCTURAL COMPONENTS OF CORONAL MASS EJECTIONS IN THE INNER CORONA (2012, methodology): “Such helical flux rope configuration has been reconstructed using nonlinear force-free field models based on photospheric vector magnetogram data (e.g., Canou et al. 2009; Cheng et al. 2010; Guo et al. 2010; Jing et al. 2010).”
• Solar filament eruptions and their physical role in triggering Coronal Mass Ejections (2012, methodology): “Further more, NLFFF magnetic extrapolations are able to reconstruct a flux rope even in a complex magnetic topology from observed vector magnetograms (see Figure 4, Canou et al., 2009; Canou and Amari, 2010; Guo et al., 2010a).”