The Trigger Mechanism of Solar Flares in a Coronal Arcade with Reversed Magnetic Shear

By K. Kusano, T. Maeshiro, T. Yokoyama, T. Sakurai. 2004

160 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/10b9c5dd52378f7a30b4094dffc518d454eacbeb

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. M. Temmer
2. P. Démoulin
3. T. Wiegelmann
4. S. Gibson
5. J. Thalmann
6. Etienne Pariat
7. Yuhong Fan
8. C. Schrijver

In Molecular Biology

1. P. Démoulin
2. S. Gibson
3. Yuhong Fan
4. T. Wiegelmann
5. J. Thalmann
6. Etienne Pariat
7. Mitchell A. Berger
8. M. Temmer

Citations in the corpus

• The Interaction of Successive Coronal Mass Ejections: A Review (2016, background): “…energy as well as helicity can be accumulated gradually via various ways, e.g., flux emergence (see, e.g. Heyvaerts, Priest, and Rust, 1977, Chen and Shibata, 2000), shearing/rotational motion (see, e.g., Manchester, 2003, Brown et al., 2003, Kusano et al., 2004, Zhang, Liu, and Zhang, 2008), etc.”
• The magnetic field in the solar atmosphere (2014, background): “ly a very accurate analysis of the helicity injection revealed that a strong, local injection of positive helicity served as the source for the observed positive helicity of the MC. Note that already Kusano et al. (2004) outlined the importance of neighbouring flux systems of helicity with opposite s”
• Photospheric flux density of magnetic helicity (2005, background): “It will also permit us to track the emergence of truly opposite magnetic polarity to the dominant one in an AR, a case which could be important for flaring (Kusano et al. 2004).”
• Coronal prominence structure and dynamics: A magnetic flux rope interpretation (2006, background): “Loss of equilibrium and eruptive behavior of both 2-D and 3-D twisted flux rope configurations have also been shown in numerical simulations [Linker et al., 2001; Amari et al., 2000, 2003a, 2004a, 2004b; Toeroek and Kliem, 2003; Kusano et al., 2004; Roussev et al., 2004; Kusano, 2005; Fan, 2005; T”
• MAGNETIC FIELD STRUCTURES TRIGGERING SOLAR FLARES AND CORONAL MASS EJECTIONS (2012, methodology): “…e.g. strong magnetic shear (Low 1977; Hagyard, et al. 1984; Mikic & Linker 1994; Kusano et al. 1995; Zhang 2001), reversed magnetic shear (Kusano et al. 2004; Wang et al. 2004; Chandra et al. 2010; Romano & Zuccarello 2011; Vemareddy et al. 2012), sigmoidal structure of the coronal…”