Cosmical Magnetic Fields: Their Origin and their Activity

By E. Parker. 2019

815 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/524bf523838204914de8bcff06eb9e3c17c76fe7

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Citations in the corpus

Stellar Flares from the First TESS Data Release: Exploring a New Sample of M Dwarfs (2019, background): “Flares on fast rotators Stellar rotation is suggested to be linked to the flaring of a star according to the dynamo theory of magnetic field generation (e.g. Moffatt 1978; Parker 1979).”
Relationship between Magnetic Power Spectrum and Flare Productivity in Solar Active Regions (2005, background): “Thus, Iroshnikov (1964) and Kraichnan (1965) found that the Alfvén effect may produce an energy spectrum k 3=2 when the correlation between velocity and magnetic fields is weak.”
Dynamo action by differential rotation in a stably stratified stellar interior (2001, background): “Several distinct instabilities are candidates for this key ingredient: Balbus-Hawley instability, buoyant (Parker-) instability, and the toroidal-field instability studied by Tayler. I have argued here and in Spruit (1999) that the latter is probably the most relevant, and have shown how a small-sca”
Magnetic Fields in the Solar Convection Zone (2004, methodology): “…implies that as a twisted flux tube rises through the solar interior, a tube that is initially stable to kinking may become unstable as it rises, and that the apex of the flux loop will become kink unstable first because of the expanded tube cross-section there (Parker, 1979; Linton et al., 1996).”
The magnetic field in the solar atmosphere (2014, background): “For further reading, we want to draw the reader’s attention to classical overviews of the theoretical aspects of solar magnetism by Parker (1979) and Priest (1982, 2014), as well as previous descriptions dedicated to aspects of the magnetic properties of the Sun’s magnetic field by Solanki et al.…”
Local Helioseismology: Three-Dimensional Imaging of the Solar Interior (2010, background): “Together, this gives rise to an ’anchoring problem’ (cf. Parker 1979).”
A Reconnection Switch to Trigger gamma-Ray Burst Jet Dissipation (2010, background): “…is an anomalous resistivity, which can be due to plasma microinstabilities (Parker 1963b; Hasegawa 1975; Coroniti & Eviatar 1977; Tsuda & Ugai 1977; Parker 1979; Syrovatskii 1981; Biskamp 1986b; Melrose 1986; Taylor 1986; Begelman & Chiueh 1988; Parker 1988b; Scholer 1989; Masuda et al. 1994;…”