We report on observations of a diverging ion flow along the geomagnetic field that is often seen at the EISCAT Svalbard radar. The flow is upward above the peak of the electron density in the F-region and downward below the peak. We estimate that in such events mass transport along the field line is important for the ionization balance, and that the shape of the F-layer and its ion composition should be strongly influenced by it. Diverging flow typically occurs when there are signatures of direct entry of sheath plasma to the ionosphere in the form of intense soft particle precipitation, and we suggest that it is caused by the ionization and ionospheric electron heating associated with this precipitation. On average, 30% of all ...
International audienceWe report high-resolution observations of the southward-IMF cusp/cleft ionosph...
On 5 January 2003, the footprint of the Cluster spacecraft, then orbiting in the dayside magnetosph...
We report high-resolution observations of the southward-IMF cusp/cleft ionosphere made on December 1...
International audienceWe report on observations of a diverging ion flow along the geomagnetic field ...
Observations by the EISCAT Svalbard radar in summer have revealed electron density enhancements in ...
Observations by the EISCAT Svalbard radar are presented that show the response of the spatial st...
The archipelago of Svalbard is at daytime located underneath the polar cusp, the window towards the ...
International audienceWe report observations of the cusp/cleft ionosphere made on December 16th 1998...
Strong ion upflows with field-aligned velocity above 1000ms were observed by the European Incohere...
Ion flow along geomagnetic field lines is an important mechanism in the coupling of the magnetospher...
We report simultaneous global monitoring of a patch of ionization and in situ observation of ion upf...
Simultaneous Common Program Two experiments by the EISCAT UHF radar at Tromsø and the EISCAT Sva...
We have determined the MLT distribution and KP dependence of the ion upflow and downflow of the the...
18th EISCAT symposiumSession E3: Ionoshere/thermosphere/mesosphereMay 27 (Sat), Poster Sessio
We report simultaneous global monitoring of a patch of ionization and in situ observation of ion upf...
International audienceWe report high-resolution observations of the southward-IMF cusp/cleft ionosph...
On 5 January 2003, the footprint of the Cluster spacecraft, then orbiting in the dayside magnetosph...
We report high-resolution observations of the southward-IMF cusp/cleft ionosphere made on December 1...
International audienceWe report on observations of a diverging ion flow along the geomagnetic field ...
Observations by the EISCAT Svalbard radar in summer have revealed electron density enhancements in ...
Observations by the EISCAT Svalbard radar are presented that show the response of the spatial st...
The archipelago of Svalbard is at daytime located underneath the polar cusp, the window towards the ...
International audienceWe report observations of the cusp/cleft ionosphere made on December 16th 1998...
Strong ion upflows with field-aligned velocity above 1000ms were observed by the European Incohere...
Ion flow along geomagnetic field lines is an important mechanism in the coupling of the magnetospher...
We report simultaneous global monitoring of a patch of ionization and in situ observation of ion upf...
Simultaneous Common Program Two experiments by the EISCAT UHF radar at Tromsø and the EISCAT Sva...
We have determined the MLT distribution and KP dependence of the ion upflow and downflow of the the...
18th EISCAT symposiumSession E3: Ionoshere/thermosphere/mesosphereMay 27 (Sat), Poster Sessio
We report simultaneous global monitoring of a patch of ionization and in situ observation of ion upf...
International audienceWe report high-resolution observations of the southward-IMF cusp/cleft ionosph...
On 5 January 2003, the footprint of the Cluster spacecraft, then orbiting in the dayside magnetosph...
We report high-resolution observations of the southward-IMF cusp/cleft ionosphere made on December 1...