S. Sazykin
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View article: Stability Analysis of Interchange-Stable Plasma Sheet to ExB Shear Flow at Substorm Onset
Stability Analysis of Interchange-Stable Plasma Sheet to ExB Shear Flow at Substorm Onset Open
Earth and Space Science Open Archive This is a preprint and has not been peer reviewed. ESSOAr is a venue for early communication or feedback before peer review. Data may be preliminary.Learn more about preprints preprintOpen AccessYou are…
View article: Theoretical Studies of Penetration of Magnetospheric Electric Fields to the Ionosphere
Theoretical Studies of Penetration of Magnetospheric Electric Fields to the Ionosphere Open
Ionospheric disturbance electric fields of magnetospheric origin play an important role in determining the global morphology and dynamics of the ionosphere of the Earth. In this work, we present a number of numerical simulations of the tra…
View article: Magnetospheric Source and Electric Current System Associated With Intense SAIDs
Magnetospheric Source and Electric Current System Associated With Intense SAIDs Open
The text files are RCM-I simulation output. The file names specify simulation time (format: hhmmss). The stored quantities are, "I","J","COLAT","ALOCT","MLT", "BNDLOC","XMIN","YMIN","FTV","BMIN", "V", "BIRK_fromV(NH)", "RCM_T_p","RCM_T_e",…
View article: Magnetospheric Source and Electric Current System Associated With Intense SAIDs
Magnetospheric Source and Electric Current System Associated With Intense SAIDs Open
The text files are RCM-I simulation output. The file names specify simulation time (format: hhmmss). The stored quantities are, "I","J","COLAT","ALOCT","MLT", "BNDLOC","XMIN","YMIN","FTV","BMIN", "V", "BIRK_fromV(NH)", "RCM_T_p","RCM_T_e",…
View article: Coupling the Rice Convection Model-Equilibrium to the Lyon– Fedder–Mobarry Global Magnetohydrodynamic Model
Coupling the Rice Convection Model-Equilibrium to the Lyon– Fedder–Mobarry Global Magnetohydrodynamic Model Open
Self-consistent inner-magnetosphere model is driven by inputs from the Lyon-Fedder- Mobarry global magnetohydrodynamic model. The expanded inner magnotospheric modeling region captures high-resolution bursty bulk flows in the plasma sheet.…
View article: Coupling the Rice Convection Model-Equilibrium to the Lyon– Fedder–Mobarry Global Magnetohydrodynamic Model
Coupling the Rice Convection Model-Equilibrium to the Lyon– Fedder–Mobarry Global Magnetohydrodynamic Model Open
Self-consistent inner-magnetosphere model is driven by inputs from the Lyon-Fedder- Mobarry global magnetohydrodynamic model. The expanded inner magnotospheric modeling region captures high-resolution bursty bulk flows in the plasma sheet.…
View article: Coupling the Rice Convection Model-Equilibrium to the Lyon– Fedder–Mobarry Global Magnetohydrodynamic Model
Coupling the Rice Convection Model-Equilibrium to the Lyon– Fedder–Mobarry Global Magnetohydrodynamic Model Open
Self-consistent inner-magnetosphere model is driven by inputs from the Lyon-Fedder- Mobarry global magnetohydrodynamic model. The expanded inner magnotospheric modeling region captures high-resolution bursty bulk flows in the plasma sheet.…
View article: The Inertialized Rice Convection Model
The Inertialized Rice Convection Model Open
The Rice Convection Model (RCM) is an established first‐principles physics model in which the field‐aligned current density is computed by the Vasyliunas equation. Its slow‐flow assumption neglects the inertial term in the MHD momentum equ…
View article: Diffuse Auroral Electron and Ion Precipitation Effects on RCM‐E Comparisons With Satellite Data During the 17 March 2013 Storm
Diffuse Auroral Electron and Ion Precipitation Effects on RCM‐E Comparisons With Satellite Data During the 17 March 2013 Storm Open
Effects of scattering of electrons from whistler chorus waves and of ions due to field line curvature on diffuse precipitating particle fluxes and ionospheric conductance during the large 17 March 2013 storm are examined using the self‐con…
View article: Recent Developments in Our Knowledge of Inner Magnetosphere‐Ionosphere Convection
Recent Developments in Our Knowledge of Inner Magnetosphere‐Ionosphere Convection Open
Plasma convection in the coupled inner magnetosphere‐ionosphere is influenced by different factors such as neutral winds, penetration electric fields, and polarization electric fields. Several crucial insights about the dynamics in the reg…
View article: Issue Information
Issue Information Open
No abstract is available for this article.
View article: Erosion of the plasmasphere during a storm
Erosion of the plasmasphere during a storm Open
The erosion of the plasmasphere during a storm is analyzed using the Naval Research Laboratory Sami3 is Also a Model of the Ionosphere ionosphere/plasmasphere code, coupled to the Rice Convection Model of the inner magnetosphere and ring c…
View article: SAMI3‐RCM simulation of the 17 March 2015 geomagnetic storm
SAMI3‐RCM simulation of the 17 March 2015 geomagnetic storm Open
We present a self‐consistent modeling study of the ionosphere‐plasmasphere system response to the 17 March 2015 geomagnetic storm using the coupled SAMI3‐RCM code. The novel feature of this work is that we capture the important storm time …
View article: Multispacecraft observations and modeling of the 22/23 June 2015 geomagnetic storm
Multispacecraft observations and modeling of the 22/23 June 2015 geomagnetic storm Open
The magnetic storm of 22–23 June 2015 was one of the largest in the current solar cycle. We present in situ observations from the Magnetospheric Multiscale Mission (MMS) and the Van Allen Probes (VAP) in the magnetotail, field‐aligned curr…
View article: On the contribution of plasma sheet bubbles to the storm time ring current
On the contribution of plasma sheet bubbles to the storm time ring current Open
Particle injections occur frequently inside 10 Re during geomagnetic storms. They are commonly associated with bursty bulk flows or plasma sheet bubbles transported from the tail to the inner magnetosphere. Although observations and theore…