The Magnetic Connection between the Convection Zone and Corona in the Quiet Sun
By W. Abbett. 2007
134 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/9b7e5b8b484f6085e2ca9b59a66b23e9d5091893
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In Astronomy and Astrophysics
- W. Manchester IV
- Matthias Rempel
- Tibor Török
- Mark C. M. Cheung
- A. Title
- Tamas I. Gombosi
- Ilia I. Roussev
- Igor M. Sokolov
Citations in the corpus
- MAGNETOHYDRODYNAMIC WAVES AND CORONAL HEATING: UNIFYING EMPIRICAL AND MHD TURBULENCE MODELS (2012, methodology): “…to be competitive with ad hoc coronal heating models, the turbulence-driven model should quantitatively reproduce some successful heating function, that is the realistic wave dissipation should provide the same heating rate, as, for example, the unsigned-flux-based heating model Abbett (2007).”
- EXTENSION OF THE MURAM RADIATIVE MHD CODE FOR CORONAL SIMULATIONS (2016, background): “Comprehensive numerical simulations of the solar corona have been developed by a few teams in the past decade (Gudiksen & Nordlund 2002, 2005b,a; Abbett 2007; Gudiksen et al. 2011; Bingert & Peter 2011, 2013; Bourdin et al. 2013; Chen et al. 2014).”
- The Origin, Early Evolution and Predictability of Solar Eruptions (2018, background): “Work in this vein began with quiet sun magneto-convection (e.g. Stein and Nordlund, 2006; Abbett, 2007; Rempel, 2014), which shows the development of a near-surface dynamo and formation of kiloGauss flux tubes in convective downdrafts.”
- Solar Surface Emerging Flux Regions: A Comparative Study of Radiative MHD Modeling and Hinode SOT Observations (2008, background): “Although the magneto-convection simulations of Abbett (2007) and Isobe, Proctor, & Weiss (2008) were not initialized with buoyant magnetic flux tubes, both studies show that convective flows interacting with an ambient field naturally lead to the creation of small-scale magnetic loops (see also…”
- SIMULATION OF THE FORMATION OF A SOLAR ACTIVE REGION (2010, background): “…have shown these two effects to be very important to the properties of flux emergence (Stein & Nordlund 2006; Cheung et al. 2007, 2008; Isobe et al. 2008; Abbett 2007; Mart́ınez-Sykora et al. 2008, 2009; Tortosa-Andreu & Moreno-Insertis 2009; Yelles Chaouche et al. 2009; Fang et al. 2010).”