Magnetohydrodynamics of the Sun

By E. Priest. 2014

328 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/b5073640f6f7b2b2efe9f51d57ccdd1e1a143bd3

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Citations in the corpus

Solar Force-free Magnetic Fields (2012, background): “Typical approaches (see the books by Priest 1982, 2014) to investigate the stability of ideal MHD equilibria (which correspond to the assumption of infinite electrical conductivity) are normal mode analysis and an energy criterion.”
Modelling Quasi-Periodic Pulsations in Solar and Stellar Flares (2018, background): “Neutral current sheets can be formed in one of three possible ways: the interaction of topologically different regions (this may give rise to a solar flare), the loss of equilibrium of a force-free field, and X-point collapse (see Priest 2014).”
Multiwavelength Studies of MHD Waves in the Solar Chromosphere (2015, unknown): “For an unbounded, homogeneous and magnetised plasma, p0, ρ0 and B0 are constant, resulting in (1a)–(1d) being rewritten as (Priest 2014), ∂ ∂t δρ = −ρ0∇ · (δv), (2a) ρ0 ∂ ∂t δv = −∇ ( δp + B0 · δB μ0 ) + 1 μ0 ∇ · (B0δB) , (2b) ∇δp = vS2∇δρ, (2c) ∂ ∂t δB = (B0 · ∇)δv − B0(∇ · δv), (2d) where the two…”
The magnetic field in the solar atmosphere (2014, background): “e locations for changes of the magnetic topology to happen, i.e., where the magnetic ﬁeld may change direction and/or magnitude (see chapter 2 in Priest (1982), Priest and Forbes (2007), chapter 6 in Priest (2014), and also section 4.5.3). As pointed out by Parnell et al. (2008), knowledge about the”
The Polarimetric and Helioseismic Imager on Solar Orbiter (2019, background): “It structures the solar chromosphere and corona and is responsible for coronal heating, it leads to flares and CMEs besides playing an important role in driving the solar wind (Solanki et al. 2006; Priest 2014).”
Observations of Turbulent Magnetic Reconnection within a Solar Current Sheet (2018, background): “Theoretically, magnetic reconnection is believed to take place in a localised region, i.e., the so-called current sheet, that has enhanced resistivity (Priest 2014; Yamada et al. 2010).”