Magnetic field inclination and atmospheric oscillations above solar active regions
By H. Schunker, P. Cally. 2006
161 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/9067f115002fa1e132f4ad710e5ec3197d33c426
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In Astronomy and Astrophysics
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Citations in the corpus
- Solar Fine-Scale Structures. I. Spicules and Other Small-Scale, Jet-Like Events at the Chromospheric Level: Observations and Physical Parameters (2012, background): “Waves that propagate from the photosphere into the chromosphere, undergo mode conversion, refraction and reflection when they reach the canopy (see e.g. Rosenthal et al., 2002; Bogdan et al., 2003; Schunker and Cally, 2006; Cally, 2007; Khomenko et al., 2008b; Kuridze et al., 2009; Nutto et al., 201”
- Oscillations and Waves in Sunspots (2015, methodology): “Later on this theory was improved and extended to the case of inclined magnetic fields, by means of the ray theory and eikonal approximation (e.g., Cally, 2005, 2006; Schunker and Cally, 2006; Cally and Goossens, 2008).”
- Local Helioseismology: Three-Dimensional Imaging of the Solar Interior (2010, background): “The waves couple near the layer where the sound speed and the Alfvén speed, a = B/ √ 4πρ, are equal (e.g. Schunker & Cally 2006).”