Physics of the Solar Corona. An Introduction

By Markus J. Aschwanden. 2004

614 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/133dc15a6fa8840143f97ab9bade3d7aa47c68b7

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

Citations in the corpus

Space Weather: The Solar Perspective (2006, background): “, the textbook Physics of the Solar Corona by Aschwanden (2004) or the upcoming article “Flare Models” in Living Reviews in Solar Physics).”
Advances in Observing Various Coronal EUV Waves in the SDO Era and Their Seismological Applications (Invited Review) (2014, unknown): “Interested readers are referred to relevant reviews (Aschwanden, 2004; Nakariakov and Verwichte, 2005; Banerjee et al., 2007; Roberts, 2008; Ofman, 2009) and recent AIA observations (e.g. Aschwanden and Schrijver, 2011; McIntosh et al., 2011; Wang et al., 2012; Gosain and Foullon, 2012; White and…”
Standing Slow-Mode Waves in Hot Coronal Loops: Observations, Modeling, and Coronal Seismology (2010, background): “Various periodic and quasi-periodic oscillations in radio, visible, EUV, and soft X-rays have been observed for decades (e.g. reviews by Aschwanden 2003, 2004a; Wang 2004; Banerjee et al. 2007).”
Coronal Heating by MHD Waves (2020, methodology): “An extensive body of literature on both resonant absorption and phase mixing exist, for which we refer the interested reader to reviews by e.g. Aschwanden (2004), Goedbloed and Poedts (2004), Goossens et al. (2011).”
Elementary Loop Structures in the Solar Corona Analyzed from TRACE Triple-Filter Images (2005, background): “This question is of fundamental importance for hydrodynamic modeling of the solar corona (Warren et al. 2002, 2003; Winebarger et al. 2003a, 2003b; Winebarger & Warren 2004; Aschwanden 2004, pp. 67–282).”
On Solving the Coronal Heating Problem (2005, methodology): “of coronal heating. 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). We deal explicitly with the magnetically-closed corona, where field lines are roo”
THREE-DIMENSIONAL SOLAR WIND MODELING FROM THE SUN TO EARTH BY A SIP-CESE MHD MODEL WITH A SIX-COMPONENT GRID (2010, background): “Solar wind heating/acceleration has long been debated by scientists for long (Aschwanden 2004; Aschwanden et al. 2008).”
CORONAL LOOP OSCILLATIONS OBSERVED WITH ATMOSPHERIC IMAGING ASSEMBLY—KINK MODE WITH CROSS-SECTIONAL AND DENSITY OSCILLATIONS (2011, background): “…reviews on the theory and observations of coronal seismology can be found in Roberts & Nakariakov (2003), Erdelyi et al. (2003), Roberts (2004), Aschwanden (2004, 2006), Wang (2004), Nakariakov & Verwichte (2005), Banerjee et al. (2007), Andries et al. (2009), Ruderman & Erdelyi (2009), and…”
A Semiempirical Magnetohydrodynamical Model of the Solar Wind (2007, background): “10 T ≈ T ≈ 10e i narrow transition region (Aschwanden 2004).”
A multiwavelength study of the M dwarf binary YY Geminorum (2015, background): “We conclude, therefore, that the Lyα light curve reflects the scale of the stellar outer atmosphere, i.e. optically thick conditions at Lyα out to heights of the order of twice the photospheric radii (cf. Aschwanden, 2004).”
Implications of X-ray Observations for Electron Acceleration and Propagation in Solar Flares (2011, background): “Observations of the radiation from hot flare plasma have shown this plasma to primarily be confined to magnetic loops or arcades of magnetic loops (cf. Aschwanden 2004).”
Kinetic Physics of the Solar Corona and Solar Wind (2006, background): “We cannot address the related physics issues here, but must refer the reader to the books of Benz (1993) and Aschwanden (2002), or the modern textbook of Aschwanden (2004) and the many references therein.”