Average properties of the magnetic reconnection ion diffusion region in the Earth's magnetotail: The 2001–2005 Cluster observations and comparison with simulations

By J. Eastwood, T. Phan, M. Øieroset, M. Shay. 2009

187 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/a9dd78e50e310aac9c1553c36744371ed186c241

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. A. Runov
2. R. Ergun
3. S. Zaharia
4. Y. Khotyaintsev
5. Juhani Birn
6. R. Nakamura
7. A. Retinò
8. M. Sitnov

In Molecular Biology

1. A. Runov
2. S. Zaharia
3. Y. Khotyaintsev
4. Juhani Birn
5. M. Sitnov
6. V. Angelopoulos

Citations in the corpus

• Magnetospheric Multiscale Science Mission Profile and Operations (2016, background): “Since the reconnection line retreats tailward after its formation (e.g., Eastwood et al. 2010), the MMS spacecraft have a reasonable chance of encountering the reconnection line from these tailward flow events.”
• Dipolarization fronts as a consequence of transient reconnection: In situ evidence (2013, background): “In fact, this event has been identified by Eastwood et al. [2010] as a”
• Particle acceleration in dipolarization events (2013, background): “This is not consistent with direct acceleration at a neutral line, which is most typically inferred to be located at 20–30 RE distance [e.g., Nagai et al., 1998; Eastwood et al., 2010].”