Svalgaard, and independently Mansurov, discovered a correspondence between the geomagnetic variations at the geomagnetic poles and the sector polarity of the interplanetary magnetic field (IMF). Heppner noted an asymmetry in the magnetospheric electric convection field observed within the polar caps at ionospheric altitudes which is also related to the sector polarity of the IMF. It is shown that both effects can be consistently explained by differential rotation of the magnetospheric plasma with respect to the earth. If the azimuthal component of the IMF is directed toward dusk, the magnetospheric plasma is slowed down in the northern polar cap and is accelerated in the southern polar cap. If the azimuthal com-ponent of the IMF is directed...
The solar-wind magnetosphere interaction primarily occurs at altitudes where the dipole component of...
Sondrestrom radar observations reveal that the dawn‐dusk (By) component of the interplanetary magnet...
The solar-wind magnetosphere interaction primarily occurs at altitudes where the dipole component of...
We assumed that the ionospheric plasma at high latitudes has a tendency to corotate about the geogra...
International audienceWe use the am, an, as and the aσ geomagnetic indices to the explore a previous...
The recently discovered relation between the azimuthal component of the interplanetary magnetic fiel...
An observed influence is studied of the interplanetary magnetic sector structure on the geomagnetic ...
It is believed that a southward interplanetary magnetic field (IMF) is mainly responsible for the en...
The solar-wind magnetosphere interaction primarily occurs at altitudes where the dipole component of...
We investigate with the help of a magnetohydrodynamic (MHD) model how the large-scale topology of ...
The solar-wind magnetosphere interaction primarily occurs at altitudes where the dipole component of...
Abstract. We used the dataset obtained from the EISCAT Svalbard Radar during 2000–2008 to study stat...
In this paper, we propose a modified procedure to infer the interplanetary magnetic field (IMF) pola...
In this paper we consider the interactions of coronal mass ejections (CMEs) with the Earth's magnet...
Preliminary observations of dayside high latitude ionospheric plasma convection with the Sondrestrom...
The solar-wind magnetosphere interaction primarily occurs at altitudes where the dipole component of...
Sondrestrom radar observations reveal that the dawn‐dusk (By) component of the interplanetary magnet...
The solar-wind magnetosphere interaction primarily occurs at altitudes where the dipole component of...
We assumed that the ionospheric plasma at high latitudes has a tendency to corotate about the geogra...
International audienceWe use the am, an, as and the aσ geomagnetic indices to the explore a previous...
The recently discovered relation between the azimuthal component of the interplanetary magnetic fiel...
An observed influence is studied of the interplanetary magnetic sector structure on the geomagnetic ...
It is believed that a southward interplanetary magnetic field (IMF) is mainly responsible for the en...
The solar-wind magnetosphere interaction primarily occurs at altitudes where the dipole component of...
We investigate with the help of a magnetohydrodynamic (MHD) model how the large-scale topology of ...
The solar-wind magnetosphere interaction primarily occurs at altitudes where the dipole component of...
Abstract. We used the dataset obtained from the EISCAT Svalbard Radar during 2000–2008 to study stat...
In this paper, we propose a modified procedure to infer the interplanetary magnetic field (IMF) pola...
In this paper we consider the interactions of coronal mass ejections (CMEs) with the Earth's magnet...
Preliminary observations of dayside high latitude ionospheric plasma convection with the Sondrestrom...
The solar-wind magnetosphere interaction primarily occurs at altitudes where the dipole component of...
Sondrestrom radar observations reveal that the dawn‐dusk (By) component of the interplanetary magnet...
The solar-wind magnetosphere interaction primarily occurs at altitudes where the dipole component of...