Reducing heliospheric magnetic flux from coronal mass ejections without disconnection
By N. Crooker, J. Gosling, S. Kahler. 2002
203 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/567c744d57da3b5c0528fc26f38dd21977ab01a8
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In Astronomy and Astrophysics
Citations in the corpus
- Observations of discrete, global magnetospheric oscillations directly driven by solar wind density variations (2003, background): “[35] A possible mechanism for the generation of the periodic solar wind density variations is interchange reconnection, which reconnects open flux tubes with closed flux tubes, leading to an influx of new plasma [Fisk, 1996; Fisk and Schwadron, 2001; Wang, 1998; Crooker et al., 2002].”
- Solar Wind Electrons Alphas and Protons (SWEAP) Investigation: Design of the Solar Wind and Coronal Plasma Instrument Suite for Solar Probe Plus (2015, background): “…of the importance of interchange reconnection, a model that aims to jointly explain coronal heating and solar wind formation by proposing that open magnetic field lines are present all over the Sun, including regions that are predominantly closed (Fisk and Schwadron 2001; Crooker et al. 2002).”
- Topological Evolution of a Fast Magnetic Breakout CME in Three Dimensions (2008, background): “The connectivity of the erupting sheared flux has been completely eaten away through interchange reconnection (e.g., Gosling et al. 1995; Crooker et al. 2002; Owens et al. 2006) from either side of the original AR PIL and now connects to the polar open field regions representing either coronal…”
- The Heliospheric Magnetic Field (2013, background): “…between the open HMF within coronal holes and closed coronal loops at the edges of coronal holes (referred to as “interchange reconnection,” e.g., Crooker et al., 2002) allows the HMF footpoints to saltate across the photosphere against differential rotation (Nash et al., 1988; Wang and…”
- CME interactions with coronal holes and their interplanetary consequences (2009, background): “Such a process known as the interchange reconnection [ Crooker et al., 2002 ] thought cause the erosion of flux ropes in the interplanetary medium [Reinard and Fisk, 2004].”
- Slow Solar Wind: Observations and Modeling (2016, unknown): “Therefore, any dynamics associated with the open-closed boundary—field line opening and closing and interchange reconnection (Crooker et al. 2002)—will affect a broad swath of the inner heliosphere, not just a narrow region about the HCS.”