International audienceThe global evolutions of foF2 anomalies were examined for three very intense geomagnetic storms, namely the Halloween events of October-November 2003 (Event X, 29?30 October 2003, Dst ?401 nT; Event Y, 20?21 November 2003, Dst ?472 nT), and the largest Dst storm (Event Z, 13?14 March 1989, Dst ?589 nT). For Event X, troughs (negative storms) were clearly seen for high northern and southern latitudes. For northern midlatitudes as well as for low latitudes, there were very strong positive effects on 29 October 2003, followed by negative effects the next day. For Event Y, there were no troughs in NH high latitudes for morning and evening hours but there were troughs for night. For midlatitudes and low latitudes, some long...
606-616A study of the intense geomagnetic storm on 2-6 April 2004 has been carried out using ionosp...
International audienceCurrent theories of F-layer storms are discussed using numerical simulations w...
International audienceWe have presented a comparison between the modeled NmF2 and hmF2, and NmF2 and...
The global evolutions of foF2 anomalies were examined for three very intense geomagnetic storms, na...
Ionospheric disturbances produced at the equatorial anomaly (EA) region during some geomagnetic stor...
Ionospheric disturbances at the crests of the equatorial anomaly during some geomagnetic storms were...
After more than 60 years of research, ionospheric disturbances are today a most challenging topic of...
International audienceIonospheric storms showing a strong depression in daytime foF2 values were sou...
An investigation of the response of the mid-high, mid and low latitude critical frequency foF2 to th...
International audienceThe ionospheric storm evolution process was monitored during the 22 September ...
International audienceUsing 8-year global ionosphere maps (GIMs) of TEC products from the Jet Propul...
The main purpose of this investigation is to study the ionospheric F region response induced by the ...
The main purpose of this investigation is to study the ionospheric F region response induced by the ...
A study is made of the intense storms of March 13–15, 1989 (Dst = –600nT), October 20–21, 1989 (Dst...
We investigate the variations in the ionosphere during a small geomagnetic storm on June 23, 2000, u...
606-616A study of the intense geomagnetic storm on 2-6 April 2004 has been carried out using ionosp...
International audienceCurrent theories of F-layer storms are discussed using numerical simulations w...
International audienceWe have presented a comparison between the modeled NmF2 and hmF2, and NmF2 and...
The global evolutions of foF2 anomalies were examined for three very intense geomagnetic storms, na...
Ionospheric disturbances produced at the equatorial anomaly (EA) region during some geomagnetic stor...
Ionospheric disturbances at the crests of the equatorial anomaly during some geomagnetic storms were...
After more than 60 years of research, ionospheric disturbances are today a most challenging topic of...
International audienceIonospheric storms showing a strong depression in daytime foF2 values were sou...
An investigation of the response of the mid-high, mid and low latitude critical frequency foF2 to th...
International audienceThe ionospheric storm evolution process was monitored during the 22 September ...
International audienceUsing 8-year global ionosphere maps (GIMs) of TEC products from the Jet Propul...
The main purpose of this investigation is to study the ionospheric F region response induced by the ...
The main purpose of this investigation is to study the ionospheric F region response induced by the ...
A study is made of the intense storms of March 13–15, 1989 (Dst = –600nT), October 20–21, 1989 (Dst...
We investigate the variations in the ionosphere during a small geomagnetic storm on June 23, 2000, u...
606-616A study of the intense geomagnetic storm on 2-6 April 2004 has been carried out using ionosp...
International audienceCurrent theories of F-layer storms are discussed using numerical simulations w...
International audienceWe have presented a comparison between the modeled NmF2 and hmF2, and NmF2 and...