Three‐dimensional collisionless magnetic reconnection in the presence of a guide field

By P. Pritchett, F. Coroniti. 2004

260 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/9022e41b7222fe65e0897ff0548fa01af2f1c019

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. P. Pritchett
4. E. Quataert
5. J. Drake
6. James Drake
7. A. Balogh
8. P. Cassak

In Atomic and Molecular Physics, and Optics

1. L. Fletcher
2. M. Swisdak
3. V. Petrosian
4. E. Quataert
5. P. Pritchett

In Nuclear and High Energy Physics

1. M. Swisdak
2. M. Shay
3. P. Pritchett
4. J. Drake
5. E. Quataert
6. James Drake
7. P. Cassak
8. A. Balogh

Citations in the corpus

• Collisionless magnetic reconnection in an asymmetric current sheet (2008, methodology): “[9] The PIC simulation model is similar to that employed in our previous studies of collisionless magnetic reconnection [ Pritchett and Coroniti, 2004; Pritchett, 2005a, 2005b].”
• Formation of secondary islands during magnetic reconnection (2006, background): “Further, the current layer develops a pronounced tilt as electrons accelerated parallel to the magnetic field stream preferentially outward along two of the four separatrices connected to the x-line [Tanaka, 1996; Pritchett and Coroniti, 2004; Drake et al., 2005].”
• Recent Advances in Understanding Particle Acceleration Processes in Solar Flares (2011, methodology): “Pritchett & Coroniti (2004) have further shown that in 3-”
• A MAGNETIC RECONNECTION MECHANISM FOR ION ACCELERATION AND ABUNDANCE ENHANCEMENTS IN IMPULSIVE FLARES (2009, background): “Evident are the low-density cavities, on two of the four separatrices (Pritchett & Coroniti 2004; Drake et al. 2005), which are evidence for the role of the kinetic Alfvén wave in driving the outflow from the x-line.”
• Cluster observations of electron holes in association with magnetotail reconnection and comparison to simulations (2005, background): “The pale yellow regions in Figure 6b are density cavities [Kleva et al., 1995; Tanaka, 1996; Pritchett and Coroniti, 2004 ] that result as the electrons, accelerated by the parallel electric field, move with high velocity toward the x line, effectively draining the separatrix region of electrons.”