Inner magnetospheric modeling with the Rice Convection Model

By F. Toffoletto, S. Sazykin, R. Spiro, R. Wolf. 2003

385 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/736cb78b59cd94732490c06bf3e2e03cb016e9d3

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In Astronomy and Astrophysics

1. R. Thorne
2. R. Horne
3. W. Manchester IV
4. Vania Jordanova
5. Nigel P. Meredith
6. J. Fennell
7. Tamas I. Gombosi
8. Wen Li

In Molecular Biology

1. R. Thorne
2. Vania Jordanova
3. R. Horne
4. W. Manchester IV
5. H. Korth
6. Tamas I. Gombosi
7. Brian J. Anderson
8. J. Fennell

Citations in the corpus

• Adaptive numerical algorithms in space weather modeling (2012, background): “The RCM [45,46] solves for the bounce averaged and isotropic but energy resolved particle distribution of electrons and various ions.”
• Global simulation of EMIC wave excitation during the 21 April 2001 storm from coupled RCM‐RAM‐HOTRAY modeling (2010, methodology): “This objective can be achieved by combining three codes (see flowchart in Figure 1): RCM [Toffoletto et al., 2003, and references therein], RAM [Jordanova et al., 1996, 1997, and references therein] and the HOTRAY code [Horne, 1989].”
• Kinetic simulations of ring current evolution during the Geospace Environment Modeling challenge events (2006, methodology): “obtained with the ring current model of Fok et al. [2001] coupled with the Rice Convection Model (RCM) [Wolf et al. ,1 982; Toffoletto et al., 2003 ], reproduced well the postmidnight enhancements of the proton fluxes observed with the HENA instrument on the Imager for Magnetopause-to-Aurora Global ”
• Space Weather Modeling Framework: A new tool for the space science community (2005, background): “Since the RCM model is symmetric, the IM is either coupled with the Northern or the Southern Hemisphere (or possibly an average of these) of the IE component.”
• Global simulation of magnetosonic wave instability in the storm time magnetosphere (2010, methodology): “[5] A global simulation of energetic ring current ion and electron phase space density, and thermal electron plasma density distribution, has been performed by coupling of two well‐established codes: RCM [ Toffoletto et al., 2003, and reference within] and RAM [Jordanova et al., 1996, 1997, and ref”
• Entropy and plasma sheet transport (2007, methodology): “The same kind of result has been obtained from more elaborate calculations with the RCM-E code, which couples the Rice Convection Model to a friction-code equilibrium solver [Toffoletto et al., 2003].”
• Interaction between direct penetration and disturbance dynamo electric fields in the storm‐time equatorial ionosphere (2005, background): “…for re-establishing shielding, controlled by several factors such as ionospheric conductivity and the temperature and density of the plasmasheet [Wolf, 1983; Toffoletto et al., 2003], was found to be less than one hour [Spiro et al., 1988] if the magnetospheric magnetic field remains constant.”
• Development of large‐scale Birkeland currents determined from the Active Magnetosphere and Planetary Electrodynamics Response Experiment (2014, methodology): “…current simulations that use the R1 currents or the corresponding fully formed polar cap convection electric field as the outer/poleward boundary to drive the inner magnetospheric response [Toffoletto et al., 2003; Zheng et al., 2006; Pembroke et al., 2012; Chen et al., 2012; Liemohn et al., 2013].”