A model of the near magnetosphere with a dawn-dusk asymmetry 1. Mathematical structure
By N. Tsyganenko. 2002
601 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/09a3b09601221209ef4d90d3c7e047b4a5a9ead6
How researchers see this paper
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In Astronomy and Astrophysics
- R. Thorne
- V. Angelopoulos
- R. Horne
- Vania Jordanova
- Wen Li
- Nigel P. Meredith
- J. Fennell
- Yoshizumi Miyoshi
In Molecular Biology
- V. Angelopoulos
- M. Sitnov
- Vania Jordanova
- N. Tsyganenko
- G. Reeves
- J. Fennell
- R. Thorne
- Yoshizumi Miyoshi
Citations in the corpus
- Magnetospheric configurations from a high-resolution data-based magnetic field model (2007, methodology): “[5] In the recent models [Tsyganenko, 1995, 1996, 2002a, 2002b; Tsyganenko et al., 2003; Tsyganenko and Sitnov, 2005, referred henceforth as T96, T02a, b, TSK03, and TS05, respectively] the tail field was represented by a linear combination of two or three partial fields, or ‘‘modules’’ BT,i (i =…”
- Modeling the dynamics of the inner magnetosphere during strong geomagnetic storms (2005, result): “TSK03, as in an earlier work [Tsyganenko, 2002a, 2002b] (hereinafter referred to as T02a and T02b), attempted to empirically model the delayed reaction of the magnetosphere to changing solar wind and IMF conditions.”
- First Results from the THEMIS Mission (2008, methodology): “The yellow curve is an equatorial projection of an ionospheric trace on a constant (66deg) magnetic longitude line, at 5deg magnetic longitude increments from 285deg to 330deg using the Tsyganenko (1989) model.”
- Precipitation of radiation belt electrons by EMIC waves, observed from ground and space (2008, methodology): “The magnetic field intensity was calculated using an empirical model [ Tsyganenko, 2002a, 2002b ].”
- Entropy and plasma sheet transport (2007, methodology): “Kubyshkina et al.[2008] compared 25 several versions of this type of model, based on T89 [Tsyganenko, 1989], T01 [Tsyganenko, 2002a, b] and T96 [Tsyganenko, 1995] magnetic fields and slightly different adjustable parameters.”
- Kinetic simulations of ring current evolution during the Geospace Environment Modeling challenge events (2006, methodology): “In addition, the ring current buildup during the main phase of a storm induces a magnetic field in an opposite direction to the terrestrial magnetic field and thus significantly modifies the field [e.g., Tsyganenko, 2002; Zaharia et al., 2005] and the storm-time particle drifts.”