The Formation of a Prominence in Active Region NOAA 8668. I. SOHO/MDI Observations of Magnetic Field Evolution
By J. Chae, Haimin Wang, J. Qiu, P. Goode, L. Strous, H. Yun. 2001
191 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/66eab3b755a6801e3c85ee78677d7102dbb069e7
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In Astronomy and Astrophysics
- P. Démoulin
- Etienne Pariat
- G. Aulanier
- P. Schuck
- Brigitte Schmieder
- Mitchell A. Berger
- L. Green
- L. Driel-Gesztelyi
Citations in the corpus
- Interplanetary flux rope ejected from an X-ray bright point. The smallest magnetic cloud source-region ever observed (2005, result): “Third, it is a simple and isolated magnetic bipole, well separated from other ARs (by at least half solar radius) but it was still eruptive.”
- Tracking Vector Magnetograms with the Magnetic Induction Equation (2008, background): “Chae et al. (2001) conjecture that local correlation tracking (LCT) (Leese et al. 1970, 1971; November & Simon 1988) provides a direct estimate of the horizontal photospheric plasma velocity:J( LCT) ¼ Vh. Démoulin & Berger (2003) conjecture that line-of-sight tracking methods, and in particular…”
- Photospheric flux density of magnetic helicity (2005, methodology): “Initially, since only horizontal velocities were deduced from the temporal evolution of Bn, it was supposed that only the shear term could be derived (e.g. Chae et al. 2001; Nindos & Zhang 2002; Moon et al. 2002b).”
- Observational Determination of the Rate of Magnetic Helicity Transport through the Solar Surface via the Horizontal Motion of Field Line Footpoints (2001, methodology): “This kind of large-40 10.4# 10 amplitude fluctuation was also noticed in the study of Chae et al. (2001).”
- Physics of Solar Prominences: II—Magnetic Structure and Dynamics (2010, background): “…that filaments are supported by nearly force-free flux ropes that lie horizontally above the PIL (e.g., Kuperus and Raadu, 1974; Pneuman, 1983; 15 van Ballegooijen and Martens, 1989; Priest et al., 1989; Rust and Kumar, 1994; Aulanier and Démoulin, 1998; Chae et al., 2001; Gibson and Fan, 2006).”
- The Magnetic Helicity Budget of Solar Active Regions and Coronal Mass Ejections (2003, methodology): “Chae et al. (2001) have studied possible fake motions introduced by errors in vLCT due to projection effects.”
- Magnetic Energy and Helicity Fluxes at the Photospheric Level (2003, methodology): “The tracking velocity ~u has been used as a proxy for the tangential plasma velocity ~vt (Chae, 2001; Chae et al., 2001; Kusano et al., 2002; Moon et al., 2002a, 2002b; Nindos & Zhang, 2002).”