Relationships of models of the inner magnetosphere to the Rice Convection Model

2001 ◽  
Vol 106 (A8) ◽  
pp. 15545-15554 ◽  
Author(s):  
M. Heinemann ◽  
R. A. Wolf

2020 ◽  
Author(s):  
Sina Sadeghzadeh ◽  
Jian Yang

<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>



2010 ◽  
Vol 115 (A12) ◽  
pp. n/a-n/a ◽  
Author(s):  
X. Liu ◽  
T. W. Hill ◽  
R. A. Wolf ◽  
S. Sazykin ◽  
R. W. Spiro ◽  
...  


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 ◽  
...  


2011 ◽  
Vol 116 (A11) ◽  
pp. n/a-n/a ◽  
Author(s):  
Chih-Ping Wang ◽  
Matina Gkioulidou ◽  
Larry R. Lyons ◽  
Richard A. Wolf ◽  
Vassilis Angelopoulos ◽  
...  


2009 ◽  
Vol 114 (A8) ◽  
pp. n/a-n/a ◽  
Author(s):  
J.-C. Zhang ◽  
R. A. Wolf ◽  
R. W. Spiro ◽  
G. M. Erickson ◽  
S. Sazykin ◽  
...  


2008 ◽  
Vol 113 (A11) ◽  
pp. n/a-n/a ◽  
Author(s):  
J. Yang ◽  
F. R. Toffoletto ◽  
R. A. Wolf ◽  
S. Sazykin ◽  
R. W. Spiro ◽  
...  


Author(s):  
Shanshan Bao ◽  
Frank Toffoletto ◽  
Jian Yang ◽  
Stanislav Sazykin ◽  
Michael Wiltberger


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