Ion outflow from the high-latitude ionosphere is a well-known phenomenon and an important source of plasma for the magnetosphere. It is also well known that pumping the ionosphere with high-power high-frequency radio waves causes electron heating. On a few occasions, this has been accompanied by artificially induced ion upwelling. We analyze such a controlled experiment at EISCAT up to 600 km altitude. The pump-enhanced electron temperatures reached up to ∼4000 K above 350 km, and ion upwelling reached up to ∼300 m/s above 500 km altitude. The pump-induced electron pressure gradient can explain the ion velocity below 450 km. Between 450 and 600 km the electron pressure gradient correlates equally with ion acceleration and ion velocity, whic...
There are recent observations of artificial plasmas created during ionospheric modification experime...
We present a multi-scale dynamic model for the creation and propagation of artificial plasma layers ...
Data acquired by the Fast Auroral Snapshot (FAST) Small Explorer during the September 24th – 25th, 1...
On 12 November 2001, artificial optical annuli were produced using the EISCAT high-frequency (HF) io...
We have developed an active ground-based technique to estimate the steady state field-aligned anomal...
Ion flow along geomagnetic field lines is an important mechanism in the coupling of the magnetospher...
The ultrahigh-frequency observation during an ionospheric heating experiment on 11 March 2014 at the...
The observation of ultra high frequency radar during an ionospheric experiment carrying out at the E...
18th EISCAT symposiumSession E3: Ionoshere/thermosphere/mesosphereMay 27 (Sat), Poster Sessio
International audienceWe report on observations of a diverging ion flow along the geomagnetic field ...
At auroral latitudes, large electric fields drive the F-region plasma of the ionosphere through the ...
We investigate the origin of low-energy (Ek 500 m s−1) ion upflows within the cusp at altitudes betw...
Strong ion upflows with field-aligned velocity above 1000ms were observed by the European Incohere...
This thesis deals with heating of outowing oxygen ions at high altitude above the polar cap using da...
We present a case study of significant heating (up to 8 keV) perpendicular to the geomagnetic field...
There are recent observations of artificial plasmas created during ionospheric modification experime...
We present a multi-scale dynamic model for the creation and propagation of artificial plasma layers ...
Data acquired by the Fast Auroral Snapshot (FAST) Small Explorer during the September 24th – 25th, 1...
On 12 November 2001, artificial optical annuli were produced using the EISCAT high-frequency (HF) io...
We have developed an active ground-based technique to estimate the steady state field-aligned anomal...
Ion flow along geomagnetic field lines is an important mechanism in the coupling of the magnetospher...
The ultrahigh-frequency observation during an ionospheric heating experiment on 11 March 2014 at the...
The observation of ultra high frequency radar during an ionospheric experiment carrying out at the E...
18th EISCAT symposiumSession E3: Ionoshere/thermosphere/mesosphereMay 27 (Sat), Poster Sessio
International audienceWe report on observations of a diverging ion flow along the geomagnetic field ...
At auroral latitudes, large electric fields drive the F-region plasma of the ionosphere through the ...
We investigate the origin of low-energy (Ek 500 m s−1) ion upflows within the cusp at altitudes betw...
Strong ion upflows with field-aligned velocity above 1000ms were observed by the European Incohere...
This thesis deals with heating of outowing oxygen ions at high altitude above the polar cap using da...
We present a case study of significant heating (up to 8 keV) perpendicular to the geomagnetic field...
There are recent observations of artificial plasmas created during ionospheric modification experime...
We present a multi-scale dynamic model for the creation and propagation of artificial plasma layers ...
Data acquired by the Fast Auroral Snapshot (FAST) Small Explorer during the September 24th – 25th, 1...