Dominant role of the asymmetric ring current in producing the stormtime

By M. Liemohn, J. Kozyra, M. Thomsen, J. Roeder, G. Lu, J. Borovsky, T. Cayton. 2001

324 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/8e0ee3d623a1480986bedacd6016e3483f563160

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

In Molecular Biology

Citations in the corpus

The Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) on RBSP (2013, result): “Kinetic model simulations (Jordanova et al. 2001a, 2003; Liemohn et al. 2001; Zaharia et al. 2010) of ring current development during storms have shown reasonable agreement with the Dst index, indicating the dominant role of magnetospheric convection in ring current energization and trapping.”
Modeling the dynamics of the inner magnetosphere during strong geomagnetic storms (2005, result): “... from its parameters in Table 2. During quiet times (i.e., before a storm, when Wp =0 ) the partial ring current magnitude is very small, defined by the free term p (0) in the coefficient p. Upon the arrival of the disturbed solar wind with a strong southward IMF, the second term quickly grows, s”
Morphology of the ring current derived from magnetic field observations (2004, methodology): “…and the lack of significant partial ring current in the dayside afternoon sector argues against the details in most drift trajectory models that predict a morning-afternoon asymmetry due to a partial ring current in the afternoon sectors (Ejiri, 1978; Chen et al., 1993; Liemohn et al., 2001).”
Properties and geoeffectiveness of magnetic clouds in the rising, maximum and early declining phases of solar cycle 23 (2005, background): “However, the contribution of the magnetopause currents toDst was larger during the sheath than during the MC, and the pressure correctedDst reached its minimum already during the sheath (Liemohn et al, 2001).”
Differences between CME‐driven storms and CIR‐driven storms (2006, background): “the ring current and partial ring current in the magnetosphere [Liemohn et al., 2001; Jordanova et al., 2003].”
Role of solar wind turbulence in the coupling of the solar wind to the Earth's magnetosphere (2003, background): “The Dst index is a measure of the amount of plasma pressure in the inner magnetosphere [Rostoker, 1972; Liemohn et al., 2001], whereas the other indices are measures of convective activity in the outer magnetosphere.”
Magnetospheric configurations from a high-resolution data-based magnetic field model (2007, background): “A commonly accepted paradigm is that the stormtime duskside depression of the geomagnetic field at low latitudes is due to a PRC that develops owing to an increased convection of freshly injected particles in the evening sector [e.g., Liemohn et al., 2001 ].”
Space Weather: Terrestrial Perspective (2007, methodology): “The drift approximation has been quite successfully applied to model inner magnetosphere plasma transport and energization during magnetic storms (Liemohn et al., 2001; Jordanova et al., 2001).”
Magnetic Pulsations: Their Sources and Relation to Solar Wind and Geomagnetic Activity (2005, background): “There is growing evidence that most of these ions simply drift through the magnetosphere and exit through the dayside boundary (Liemohn et al., 2001).”
Storm‐time distortion of the inner magnetosphere: How severe can it get? (2003, background): “The idea behind replacing Dst with a function of G 3 stemmed from the fact that the rapid buildup of the partial ring current is a result of the strongly enhanced, directly driven convection from the tail, and it should also quickly recede during the recovery phase [Liemohn et al., 2001].”