Magnetic Field and Plasma Scaling Laws: Their Implications for Coronal Heating Models

By C. H. Mandrini, P. Démoulin, J. Klimchuk. 2000

197 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/bd1d11310f48f3a6b21786e6f0c9d267980b75a4

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

In Molecular Biology

Citations in the corpus

On Solving the Coronal Heating Problem (2005, methodology): “For such information, the reader is referred to Gómez (1990), Zirker (1993), Narain and Ulmschneider (1996), Mandrini, Démoulin, and Klimchuk (2000), Walsh and Ireland (2003), and Aschwanden (2004).”
Current sheet formation in quasi-separatrix layers and hyperbolic flux tubes (2005, background): “Many models exist for heating the corona by the dissipation of thin current layers, as extensively reviewed in Mandrini et al. (2000).”
Highly Efficient Modeling of Dynamic Coronal Loops (2005, background): “By determining which parameters best reproduce the observations, we can place important constraints on the heating and thereby gain insight into the physical mechanism (e.g., Mandrini et al. 2000; Schrijver et al. 2004;Warren&Winebarger 2006).”
HEATING OF THE SOLAR CHROMOSPHERE AND CORONA BY ALFVÉN WAVE TURBULENCE (2011, result): “This result may be compared with other models of coronal heating (see Mandrini et al. 2000; Schrijver et al. 2004).”
An Ab Initio Approach to the Solar Coronal Heating Problem (2004, background): “Further studies of heating models and observations have all supported these heating function characteristics (Mandrini et al. 2000; Foley et al. 2002; Schrijver & Aschwanden 2002; Démoulin et al. 2003; Schmieder et al. 2003).”
Coronal Loops: Observations and Modeling of Confined Plasma (2010, methodology): “Based on a previous study of the plasma parameters and the magnetic flux density (Mandrini et al., 2000), Démoulin et al.”
MULTISPECTRAL EMISSION OF THE SUN DURING THE FIRST WHOLE SUN MONTH: MAGNETOHYDRODYNAMIC SIMULATIONS (2008, background): “Mandrini et al. (2000), Priest et al. (2000), and Aschwanden (2001) have summarized the characteristics and physical implications of a number of models that are currently believed to be viable.”
The Relationship Between X-Ray Radiance and Magnetic Flux (2003, background): “…of coronal heating were limited to a particular solar/stellar object, e.g., dwarf stars (Saar & Schrijver 1987; Schrijver et al. 1989), active regions and dwarf stars (Fisher et al. 1998), solar active regions (Mandrini et al. 2000; Yashiro & Shibata 2001), and the quiet Sun (Wolfson et al. 2000).”