Cavities of weak magnetic field strength in the wake of FTEs: Results from global magnetospheric MHD simulations

نویسندگان

  • M. M. Kuznetsova
  • D. G. Sibeck
  • M. Hesse
  • Y. Wang
  • L. Rastaetter
  • G. Toth
  • A. Ridley
چکیده

[1] We use the global magnetohydrodynamic (MHD) code BATS-R-US to model multipoint observations of Flux Transfer Event (FTE) signatures. Simulations with high spatial and temporal resolution predict that cavities of weak magnetic field strength protruding into the magnetosphere trail FTEs. These predictions are consistent with recently reported multi-point Cluster observations of traveling magnetopause erosion regions (TMERs). Citation: Kuznetsova, M. M., D. G. Sibeck, M. Hesse, Y. Wang, L. Rastaetter, G. Toth, and A. Ridley (2009), Cavities of weak magnetic field strength in the wake of FTEs: Results from global magnetospheric MHD simulations, Geophys. Res. Lett., 36, L10104, doi:10.1029/2009GL037489.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Pressure anisotropy in global magnetospheric simulations: Coupling with ring current models

[1] We have recently extended the global magnetohydrodynamic (MHD) model BATS-R-US to account for pressure anisotropy. Since the inner magnetosphere dynamics cannot be fully described even by anisotropic MHD, we coupled our anisotropic MHD model with two inner magnetospheric models: the Rice Convection Model (RCM) and the Comprehensive Ring Current Model (CRCM). The coupled models provide bette...

متن کامل

Dynamics of Ganymede’s magnetopause: Intermittent reconnection under steady external conditions

[1] Magnetic reconnection at the terrestrial magnetopause is frequently intermittent, leading to the formation of localized reconnected flux bundles referred to as flux transfer events (FTEs). It remains unclear whether the intermittency of the process is intrinsic or arises because of fluctuations of solar wind properties. Here we use Ganymede’s magnetosphere, which is embedded in a background...

متن کامل

Multiscale modeling of magnetospheric reconnection

[1] In our efforts to bridge the gap between small-scale kinetic modeling and global simulations, we introduced an approach that allows to quantify the interaction between large-scale global magnetospheric dynamics and microphysical processes in diffusion regions near reconnection sites. We use the global MHD code BATS-R-US and replace an ad hoc anomalous resistivity often employed by global MH...

متن کامل

Self-Consistent hot spot tracing particles by kinetic simulations: With the emphasis on Cusp particle entry

One of the most important advantages of particle simulation as compared to fluid simulation is the capacity for working with and tracing particles. In particle simulations, the test particle method is usually used to get some idea of the behavior of plasma or other substances. In this method, first, a small number of particles are injected into the frame of static electromagnetic fields. Then, ...

متن کامل

Coupling of a global MHD code and an inner magnetospheric model: Initial results

[1] This paper describes the coupling of BATS-R-US (Block Adaptive Tree Solar-wind Roe-type Upwind Scheme), a magnetohydrodynamics (MHD) code representing the Earth’s global magnetosphere and its coupling to the ionosphere and solar wind, and the Rice Convection Model (RCM), which represents the inner magnetosphere and its coupling to the ionosphere. The MHD code provides a time-evolving magnet...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2009