Tail Reconnection Triggering Substorm Onset

By V. Angelopoulos, J. Mcfadden, D. Larson, C. Carlson, S. Mende, H. Frey, T. Phan, D. Sibeck, Karl-Heinz Glassmeier, Uli Auster and 7 more. Science, 2008

657 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/31ed626e4b30d2ca0ea50b9265bea6fec5b99d5b

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. V. Angelopoulos
3. Xuzhi Zhou
4. Jiang Liu
5. V. Sergeev
6. R. Nakamura
7. Wolfgang Baumjohann
8. R. McPherron

In Geophysics

1. R. McPherron
2. A. Runov
3. V. Angelopoulos
4. Tuija I. Pulkkinen

Citations in the corpus

• Substorm Current Wedge Revisited (2015, background): “In addition, the Cluster, Geotail and THEMIS missions have shown the critical role fast flows play in substorm development (e.g., Angelopoulos et al. 2008; Baker et al. 2002).”
• Magnetic flux transport by dipolarizing flux bundles (2013, methodology): “During substorms, ground magnetic perturbations usually commence after the DFB appears in the tail [Angelopoulos et al., 2008; Liu et al., 2011a; Nishimura et al., 2012], so we compute each DFB’s corresponding AE value as the average over t0 + 1.5min to t0 + 4.5min.”
• On the current sheets surrounding dipolarizing flux bundles in the magnetotail: The case for wedgelets (2013, methodology): “The solid-state telescope (SST) [Angelopoulos, 2008] detects high-energy (25 keV to 1MeV) ion and electron fluxes also with 3-s time resolution during fast survey.”