The Cluster spacecraft have now amassed 3 years of data from crossings of the mid-altitude cleft/cusp.Comparison of particle data from the PEACE and CIS instruments shows that there is pronounceable difference in latitude between the equatorward edges of the electron and ion populations of the cleft region, and this difference increases in the dawn/dusk directions. We define the electron edge of the cleft by the first injection of the magnetosheath-like electrons and the disappearance of the trapped plasma-sheet particles.Correspondingly the ion boundary is identified by the first injection of magnetosheath-like ions. The region between these two boundaries, which we define as the 'electron-only' cleft region, contains parallel and/or antip...
International audienceThis paper reviews Cluster observations of the high altitude and exterior (out...
Abstract. We analyse two crossings of the polar cusp at mid-altitudes (≈4RE) by Cluster in order to ...
Abstract SM51A-06The polar cusps are two regions of the magnetosphere where the influence of the int...
The Cluster spacecraft have now amassed 3 years of data from crossings of the mid-altitude cleft/cus...
International audienceThe nature of particle precipitations at dayside mid-altitudes can be interpre...
We present examples of electron measurements from the PEACE instruments on the Cluster spacecraft ...
The Cluster spacecraft often cross the midaltitude cleft/cusp and observe a very well defined “elect...
During southward interplanetary magnetic field (IMF), the electron and ion boundary are separated ne...
We study the energetic electrons by the Cluster-II Rapid instrument on a dayside high-latitude pass ...
Abstract. Energetic electrons (e.g., 50 keV) travel along field lines with a high speed of around 20...
[1] We present a comparison of two events, monitored by the Double Star and Cluster spacecraft at se...
International audienceAbove the polar caps and during prolonged periods of Northward IMF, the Cluste...
Launched on an elliptical high inclination orbit (apogee: 19.6 RE) since January 2001 the Cluste...
International audienceThis paper reviews Cluster observations of the high altitude and exterior (out...
Abstract. We analyse two crossings of the polar cusp at mid-altitudes (≈4RE) by Cluster in order to ...
Abstract SM51A-06The polar cusps are two regions of the magnetosphere where the influence of the int...
The Cluster spacecraft have now amassed 3 years of data from crossings of the mid-altitude cleft/cus...
International audienceThe nature of particle precipitations at dayside mid-altitudes can be interpre...
We present examples of electron measurements from the PEACE instruments on the Cluster spacecraft ...
The Cluster spacecraft often cross the midaltitude cleft/cusp and observe a very well defined “elect...
During southward interplanetary magnetic field (IMF), the electron and ion boundary are separated ne...
We study the energetic electrons by the Cluster-II Rapid instrument on a dayside high-latitude pass ...
Abstract. Energetic electrons (e.g., 50 keV) travel along field lines with a high speed of around 20...
[1] We present a comparison of two events, monitored by the Double Star and Cluster spacecraft at se...
International audienceAbove the polar caps and during prolonged periods of Northward IMF, the Cluste...
Launched on an elliptical high inclination orbit (apogee: 19.6 RE) since January 2001 the Cluste...
International audienceThis paper reviews Cluster observations of the high altitude and exterior (out...
Abstract. We analyse two crossings of the polar cusp at mid-altitudes (≈4RE) by Cluster in order to ...
Abstract SM51A-06The polar cusps are two regions of the magnetosphere where the influence of the int...