Add to ORKGUsing the Tsyganenko magnetic field model (TSYGANENKO, Planet. Space Sci., 37, 5, 1989) we make an attempt to determine the outer boundary of the closed region when the interplanetary magnetic field (IMF) is southward. As a simple magnetic field model including the effect of IMF B_z<0, the B_z component of a constant value of minus a few nanoTeslas is added to the magnetic field in the Tsyganenko model with low K_p values. In this paper, if the magnetic field strength, B, is not less than 2 nT in the whole range of a field line (namely the minimum B along a field line is greater than 2 nT), this field line is judged to be "firmly" closed. The firmly closed field lines are thought to be definitely closed as long as the fluctuation amplitude ...
This thesis investigates the effect that northward IMF (Interplanetary Magnetic Field) has on the Ea...
We model an interval of remarkable interplanetary magnetic field (IMF), for which we have a comprehe...
In this paper we consider the interactions of coronal mass ejections (CMEs) with the Earth's magnet...
Using the Tsyganenko magnetic field model (TSYGANENKO, Planet. Space Sci., 37, 5, 1989) we make an a...
This paper proposes that the outer boundary of the "firmly-closed" region should be represented by f...
[1] In this paper we investigate the effect of changes in the interplanetary magnetic field (IMF), s...
[1] The development of global magnetospheric models, such as Space Weather Modeling Framework (SWMF)...
Abstract. Observed properties of the magnetic field in the outer heliosphere are generally well desc...
International audienceWe study the topological structure of the magnetosphere for northward IMF. Usi...
All-sky auroral images acquired at Ny-Ålesund were used in conjunction with observations of a Polar ...
The Polar satellite with its high apogee and high latitude orbit offers a unique opportunity to char...
In the open magnetosphere model magnetic field lines from the polar caps connect to the interplaneta...
We investigate with the help of a magnetohydrodynamic (MHD) model how the large-scale topology of ...
The Mead-Fairfield geomagnetic field models have been used to trace field lines between the outer ma...
We model an interval of remarkable interplanetary magnetic field (IMF), for which we have a comprehe...
This thesis investigates the effect that northward IMF (Interplanetary Magnetic Field) has on the Ea...
We model an interval of remarkable interplanetary magnetic field (IMF), for which we have a comprehe...
In this paper we consider the interactions of coronal mass ejections (CMEs) with the Earth's magnet...
Using the Tsyganenko magnetic field model (TSYGANENKO, Planet. Space Sci., 37, 5, 1989) we make an a...
This paper proposes that the outer boundary of the "firmly-closed" region should be represented by f...
[1] In this paper we investigate the effect of changes in the interplanetary magnetic field (IMF), s...
[1] The development of global magnetospheric models, such as Space Weather Modeling Framework (SWMF)...
Abstract. Observed properties of the magnetic field in the outer heliosphere are generally well desc...
International audienceWe study the topological structure of the magnetosphere for northward IMF. Usi...
All-sky auroral images acquired at Ny-Ålesund were used in conjunction with observations of a Polar ...
The Polar satellite with its high apogee and high latitude orbit offers a unique opportunity to char...
In the open magnetosphere model magnetic field lines from the polar caps connect to the interplaneta...
We investigate with the help of a magnetohydrodynamic (MHD) model how the large-scale topology of ...
The Mead-Fairfield geomagnetic field models have been used to trace field lines between the outer ma...
We model an interval of remarkable interplanetary magnetic field (IMF), for which we have a comprehe...
This thesis investigates the effect that northward IMF (Interplanetary Magnetic Field) has on the Ea...
We model an interval of remarkable interplanetary magnetic field (IMF), for which we have a comprehe...
In this paper we consider the interactions of coronal mass ejections (CMEs) with the Earth's magnet...