scholarly journals Rice Convection Model simulation of the substorm-associated injection of an observed bubble into the inner magnetosphere: 1. Magnetic field and other inputs

2009 ◽  
Vol 114 (A8) ◽  
pp. n/a-n/a ◽  
Author(s):  
J.-C. Zhang ◽  
R. A. Wolf ◽  
G. M. Erickson ◽  
R. W. Spiro ◽  
F. R. Toffoletto ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Model Simulation ◽  
Inner Magnetosphere ◽  
Rice Convection Model ◽  
Convection Model

Rice Convection Model simulation of the 18 April 2002 sawtooth event and evidence for interchange instability

2008 ◽  
Vol 113 (A11) ◽  
pp. n/a-n/a ◽  
Author(s):  
J. Yang ◽  
F. R. Toffoletto ◽  
R. A. Wolf ◽  
S. Sazykin ◽  
R. W. Spiro ◽  
...  
Keyword(s):  
Model Simulation ◽  
Rice Convection Model ◽  
Convection Model ◽  
Interchange Instability

Interplay of bubble injections in the plasma sheet dynamics as inferred from RCM-I simulations

2020 ◽  
Author(s):  
Sina Sadeghzadeh ◽  
Jian Yang
Keyword(s):  
Plasma Sheet ◽  
High Speed ◽  
Space Environment ◽  
Inner Magnetosphere ◽  
Near Earth Space ◽  
Hot Plasma ◽  
Plasma Distribution ◽  
Rice Convection Model ◽  
Convection Model ◽  
Interchange Instability

<p><span>Understanding the transport of hot plasma from tail towards the inner magnetosphere is of great importance to improve our perception of the near-Earth space environment. In accordance with the recent observations, the contribution of bursty bulk flows (BBFs)/bubbles in the inner plasma sheet especially in the storm-time ring current formation is nonnegligible. These high-speed plasma flows with depleted flux tube/entropy are likely formed in the mid tail due to magnetic reconnection and injected earthward as a result of interchange instability. In this presentation, we investigate the interplay of these meso-scale structures on the average magnetic field and plasma distribution in various regions of the plasma sheet, using the Inertialized Rice Convection Model (RCM-I). We will discuss the comparison of our simulation results with the observational statistics and data-based empirical models.</span></p>

Numerical simulation of plasma transport in Saturn's inner magnetosphere using the Rice Convection Model

2010 ◽  
Vol 115 (A12) ◽  
pp. n/a-n/a ◽  
Author(s):  
X. Liu ◽  
T. W. Hill ◽  
R. A. Wolf ◽  
S. Sazykin ◽  
R. W. Spiro ◽  
...  
Keyword(s):  
Numerical Simulation ◽  
Plasma Transport ◽  
Inner Magnetosphere ◽  
Rice Convection Model ◽  
Convection Model

scholarly journals Magnetic storm ring current injection modeled with the Rice Convection Model and a self-consistent magnetic field

2004 ◽  
Vol 31 (21) ◽  
pp. n/a-n/a ◽  
Author(s):  
C. Lemon ◽  
R. A. Wolf ◽  
T. W. Hill ◽  
S. Sazykin ◽  
R. W. Spiro ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Magnetic Storm ◽  
Ring Current ◽  
Current Injection ◽  
Rice Convection Model ◽  
Self Consistent ◽  
Convection Model
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