Acceleration of the solar wind as a result of the reconnection of open magnetic flux with coronal loops
By L. Fisk. 2003
167 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/8d3ce4fed66a3f2dfe81c2a0fa5e4dbc770aae88
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
- Pete Riley
- S. Gibson
- W. Manchester IV
- S. Cranmer
- Tamas I. Gombosi
- Roberto Lionello
- M. Owens
- Igor M. Sokolov
In Molecular Biology
- Pete Riley
- W. Manchester IV
- S. Cranmer
- S. Gibson
- Tamas I. Gombosi
- R. Marsden
- Igor M. Sokolov
- M. Owens
Citations in the corpus
- A Semiempirical Magnetohydrodynamical Model of the Solar Wind (2007, background): “…way to incorporate this empirical relationship to our MHD model—including neither the potential field expansion nor the potential field at all—is to relate the solar wind speed to the spatial distribution of the Bernoulli integral throughout the SC and IH (Parker 1963; Fisk 2003; Suzuki 2006).”
- Origins of the Ambient Solar Wind: Implications for Space Weather (2017, background): “…suggested that RLO-type energy interchange primarily occurs at the scale of the supergranular network (Axford and McKenzie 1992; Fisk et al. 1999; Fisk 2003; Schwadron et al. 2006; Yang et al. 2013; Karpen et al. 2017), and others favor larger-scale reconnection events near global null points…”
- Self-consistent Coronal Heating and Solar Wind Acceleration from Anisotropic Magnetohydrodynamic Turbulence (2007, background): “…Kovalenko 1978, 1981; Wang & Sheeley 1991, 2006; Wang 1993; Cranmer 2005a), some have treated it as a by-product of varying boundary conditions in the low corona (e.g., Fisk 2003; Schwadron & McComas 2003), and some have considered a combination of the two (Bravo & Stewart 1997; Suzuki 2006).”
- Solar Wind Helium Abundance as a Function of Speed and Heliographic Latitude: Variation through a Solar Cycle (2007, background): “Qualitatively, it is expected that the confinement time of plasma to a coronal loop is related to its physical size, and these factors in turn determine the temperature profile and the timescale for wave absorption, gravitational settling, radiation, and kinetic processes (Woo 2004; Fisk 2003).”
- Global distribution of the solar wind during solar cycle 23: ACE observations (2009, background): “The loop temperature determines the coronal electron temperature of the released material and thus the elevated solar wind charge states [Fisk et al., 1998; Fisk, 2003].”
- The Solar Orbiter mission (2020, background): “…active in the intermediate areas of the quiet Sun (Bellot Rubio & Orozco Suárez 2019), and is the underlying mechanism invoked by Fisk and coworkers (Fisk et al. (1998); Fisk (2003); Fisk & Zurbuchen (2006); Fisk & Zhao (2009); Zhao et al. (2017)) in their model for the heliospheric magnetic field.”
- A MODEL FOR THE SOURCES OF THE SLOW SOLAR WIND (2010, background): “This latter process is the underlying mechanism invoked by Fisk and co-workers (Fisk et al. 1998; Fisk 2003; Fisk & Zhao 2009) in their model for the heliospheric field.”
- The Heliospheric Magnetic Field (2013, background): “Indeed, a similar mechanism has been proposed as the source of the slow solar wind (Fisk, 2003).”
- Slow Solar Wind: Observations and Modeling (2016, unknown): “The interchange reconnection model (Fisk et al. 1998; Fisk and Schwadron 2001; Fisk 2003; Zurbuchen 2006; Fisk and Zhao 2009) discussed above as scenario SSW2 for the slow solar wind formations, in which the small-scale dynamics of the photospheric magnetic field, as in the so-called magnetic carpet”
- Solar Orbiter (2012, background): “This process should occur predominantly at the coronal hole boundary, but may also be active in the intermediate areas of quiet Sun, and is the underlying mechanism invoked by Fisk and coworkers (Fisk, Schwadron, and Zurbuchen, 1998; Fisk, 2003; Fisk and Zurbuchen, 2006; Fisk and Zhao, 2009) in thei”