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A model of the near magnetosphere with a dawn-dusk asymmetry 1. Mathematical structure
[1] A new empirical magnetic field model has been developed, representing the variable configuration of the inner and near magnetosphere for different interplanetary conditions and the groundExpand
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Storm‐time distortion of the inner magnetosphere: How severe can it get?
[1] First results are presented of an effort to model the storm-time distortion of the magnetic field in the inner magnetosphere using space magnetometer data. Strong geomagnetic storms areExpand
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Tail plasma sheet models derived from Geotail particle data
[1] Simple analytical models have been derived for the first time, describing the 2-D distribution (along and across the Earth's magnetotail) of the central plasma sheet (CPS) ion temperature,Expand
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Disturbances in Mercury's magnetosphere: Are the Mariner 10 “substorms” simply driven?
In addition to providing the first in situ evidence of a magnetosphere at Mercury, the first flyby by Mariner 10 inspired reports of Earth-like substorms. While the small scales at Mercury shouldExpand
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GLOBAL QUANTITATIVE MODELS OF THE GEOMAGNETIC-FIELD IN THE CISLUNAR MAGNETOSPHERE FOR DIFFERENT DISTURBANCE LEVELS
Abstract A previously proposed model (Tsyganenko and Usmanov, 1982, Planet. Space Sci . 30 , 985) is further developed, using IMP -A, C, D, E, F, G, H, I, J and HEOS -1, -2 spacecraft measurementsExpand
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Modeling of twisted/warped magnetospheric configurations using the general deformation method
A new method is developed for modeling the effects of the planetary dipole tilt and of the interplanetary magnetic field (IMF) related twisting of the cross-tail current sheet. The method extends theExpand
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Magnetospheric configurations from a high-resolution data-based magnetic field model
[1] We present first results of the magnetospheric magnetic field modeling, based on large sets of spacecraft data and a high-resolution expansion for the field of equatorial currents. In thisExpand
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Observations and model predictions of substorm auroral asymmetries in the conjugate hemispheres
[1] Based on imaging data from the Polar VIS Earth camera and the IMAGE-FUV instruments we have documented how the IMF orientation and the dipole tilt angle act as the main and the secondaryExpand
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An empirical model of the substorm current wedge
A wedge-shaped current linking the nightside ionosphere and the plasma sheet is believed to be the principal cause of a major reconfiguration of the magnetospheric field on the nightside, observed atExpand
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Storm time evolution of the outer radiation belt: Transport and losses
[1] During geomagnetic storms the magnetic field of the inner magnetosphere exhibits large-scale variations over timescales from minutes to days. Being mainly controlled by the magnetic field theExpand
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