Three‐dimensional particle simulations of collisionless magnetic reconnection

By A. Zeiler, D. Biskamp, J. Drake, B. Rogers, M. Shay, M. Scholer. 2001

237 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/a5bc28309d64f3f2802d9aab6d030af817c751ce

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

1. M. Swisdak
2. M. Shay
3. E. Quataert
4. T. Phan
5. James Drake
6. J. Drake
7. Merav Opher
8. P. Cassak

In Nuclear and High Energy Physics

1. M. Swisdak
2. M. Shay
3. E. Quataert
4. J. Drake
5. James Drake
6. P. Cassak
7. T. Phan
8. Merav Opher

Citations in the corpus

• Cluster observations of electron holes in association with magnetotail reconnection and comparison to simulations (2005, methodology): “[13] Results from particle simulations are presented for comparison to the Cluster data (see Zeiler et al. [2002] for discussion of the p3d simulation code).”
• Ion heating resulting from pickup in magnetic reconnection exhausts (2009, methodology): “[5] Our simulations are performed with the particle-incell code p3d [Zeiler et al., 2002].”
• Recent Advances in Understanding Particle Acceleration Processes in Solar Flares (2011, methodology): “D kinetic PIC approach (Zeiler et al. 2002; Pritchett & Coroniti 2004; Karimabadi et al. 2007; Shay et al. 2007; Daughton et al. 2009; Drake et al. 2010).”
• THE VECTOR DIRECTION OF THE INTERSTELLAR MAGNETIC FIELD OUTSIDE THE HELIOSPHERE (2010, methodology): “For our kinetic simulations we use p3d, a massively parallel PIC code (Zeiler et al. 2002).”
• Average properties of the magnetic reconnection ion diffusion region in the Earth's magnetotail: The 2001–2005 Cluster observations and comparison with simulations (2009, methodology): “10 of 13 However, to ensure similar renormalization of the simulation data and enable accurate comparison with the observational data, a simulation of magnetic reconnection was performed using the particle in cell code P3D [Zeiler et al., 2002].”
• Formation of secondary islands during magnetic reconnection (2006, methodology): “[5] Our simulations are performed with the particle-incell code p3d [Zeiler et al., 2002].”
• Cluster observations of an intense normal component of the electric field at a thin reconnecting current sheet in the tail and its role in the shock-like acceleration of the ion fluid into the separatrix region (2005, methodology): “We do note that the width of this current sheet is comparable to the widths (0.1 ion inertial lengths) of the very thin current sheet studied in recent PIC simulations [ Zeiler et al., 2002; Ricci et al., 2002].”
• Diamagnetic suppression of component magnetic reconnection at the magnetopause (2003, methodology): “[10] The simulations are done with p3d, a massively parallel kinetic code that can evolve up to 10(9) particles on current Cray T3E and IBM SP systems [Zeiler et al., 2002].”
• A MAGNETIC RECONNECTION MECHANISM FOR ION ACCELERATION AND ABUNDANCE ENHANCEMENTS IN IMPULSIVE FLARES (2009, methodology): “Our simulations are performed with the PIC code p3d (Zeiler et al. 2002) and the Hall MHD code f3d (Shay et al. 2004).”