Storm‐time distortion of the inner magnetosphere: How severe can it get?

By N. Tsyganenko, H. Singer, Justin C. Kasper. 2003

246 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/665af74079ff64c532e836746fe4fe22995d2fc0

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. R. Thorne
2. Y. Shprits
3. Wen Li
4. Vania Jordanova
5. R. Horne
6. Nigel P. Meredith
7. Craig Kletzing
8. Jacob Bortnik

In Molecular Biology

1. R. Thorne
2. Vania Jordanova
3. M. Sitnov
4. Y. Shprits
5. Craig Kletzing
6. G. Reeves
7. S. Sazykin
8. N. Tsyganenko

Citations in the corpus

• Explaining sudden losses of outer radiation belt electrons during geomagnetic storms (2012, methodology): “Also shown are magnetic fields measured by GOES-13 (blue) and modeled (green) for the spacecraft location using the Tsyganenko-2001 Storm model [Tsyganenko et al., 2003] and the L for GOES-13 calculated using the same model.”
• The energization of relativistic electrons in the outer Van Allen radiation belt (2007, methodology): “16 , we used the Tsyganenko 2001 storm-time magnetic field mode”
• 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, background): “[2] In our earlier paper [Tsyganenko et al., 2003] (hereinafter referred to as TSK03), a model of the inner magnetospheric storm-time field was described, based on space”
• Interaction between direct penetration and disturbance dynamo electric fields in the storm‐time equatorial ionosphere (2005, methodology): “The RCM simulation of this event utilized a time-sequence of Tsyganenko et al. [2003] storm-time magnetic-field models, a plasma sheet model [Tsyganenko and Mukai, 2003] as the outer boundary condition, and a time-sequence of polar cap potential drop values [Boyle et al., 1997].”
• The Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) on RBSP (2013, background): “Large magnetic field depressions have been measured at distances as small as 3–4 Earth radii (RE) during major geomagnetic storms (Dst < 250 nT) and have been associated with the storm time ring current enhancement (e.g., Cahill 1966; Tsyganenko et al. 2003).”
• Space Weather: Terrestrial Perspective (2007, background): “There are a number of large-scale magnetospheric magnetic field models that give the field configuration as a function of either solar wind conditions or magnetospheric activity parameters (Tsyganenko, 1989, 1995; Tsyganenko et al., 2003).”