The Current Sheet Associated with the 2003 November 4 Coronal Mass Ejection: Density, Temperature, Thickness, and Line Width
By A. Ciaravella, J. C. Raymond. 2008
156 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/303b1bc5ef11a4cf67c2ed4b0265cdb3fd3b6af5
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In Astronomy and Astrophysics
- A. Lazarian
- Grzegorz Kowal
- Ethan Vishniac
- Gregory L. Eyink
- Xin Cheng
- M. Ding
- K. Otmianowska-Mazur
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Citations in the corpus
- FAST MAGNETIC RECONNECTION AND SPONTANEOUS STOCHASTICITY (2011, background): “Recent observations of a greatly thickened current sheet associated with coronal mass ejections give broad support to LV99 (Ciaravella & Raymond 2008; Bemporad et al. 2008).”
- Observations of Turbulent Magnetic Reconnection within a Solar Current Sheet (2018, background): “…sheet are mostly limited by the wavelength window that only responds to relatively narrow and low temperatures and/or the field of view that is not large enough (Lin et al. 2005, 2009; Ciaravella et al. 2003; Ciaravella & Raymond 2008; Savage et al. 2010; Ling et al. 2014; Seaton et al. 2017).”
- Magnetic Reconnection in Astrophysical and (2009, background): “Ciaravella & Raymond (2008) found evidence for a postflare vertical current sheet tens of thousands of kilometers wide that persisted for many hours.”
- RECONNECTION OUTFLOWS AND CURRENT SHEET OBSERVED WITH HINODE/XRT IN THE 2008 APRIL 9 “CARTWHEEL CME” FLARE (2010, methodology): “Thus the proposed current sheet is not observed directly edge-on, but with some projection (as in Ko et al. 2002 and Ciaravella & Raymond 2008).”
- NUMERICAL TESTS OF FAST RECONNECTION IN WEAKLY STOCHASTIC MAGNETIC FIELDS (2009, background): “Straus’ idea is closely related to recent attempts to explain the existence of the observed thick reconnection region in the context of numerical models of collisionless reconnection (Ciaravella & Raymond 2008) and predictions of particle acceleration within these regions (Drake et al. 2006a).”
- Acceleration of primary and secondary particles in galaxy clusters by compressible MHD turbulence: from radio haloes to gamma-rays (2010, unknown): “In addition, observational data does not support the X-point reconnection predicted in the Petscheck model either (see Ciaravella & Raymond 2008).”