International audienceUsing EISCAT radar data, we find that electrons are strongly heated in the magnetic field-line direction during high electric field events. The remote site data show that the electron temperature increases in almost the same way in the field-perpendicular direction; electron heating by E region plasma turbulence is isotropic. We discuss the implications of our observation for the "plasmon"-electron as well as the wave Joule heating models of the anomalous electron heating in the E region
International audienceWe analyzed 20 reconnection events observed by the Magnetosphere MultiScale mi...
International audienceShock waves are ubiquitous in space and astrophysics. They transform directed ...
International audienceTaking advantage of the string-of-pearls configuration of the five THEMIS spac...
Using EISCAT radar data, we find that electrons are strongly heated in the magnetic field-line dire...
It has been shown in previous studies that at 110 km altitude, the electron temperature can be quite...
International audienceUsing EISCAT data, we have studied the behavior of the E region electron tempe...
We present data from nighttime sounding rocket flights in the low latitude E region. The payloads ca...
International audienceThe electron component of intensive electric currents flowing along the geomag...
In recent years, large electron temperature increases of 300% (3000 K above background) caused by po...
An extensive series of spectral measurements has been made in the auroral E region with the Chatanik...
We have recently implemented a new module that includes both the anomalous electron heating and the ...
We present the first observations of large amplitude waves in a well-defined electron diffusion regi...
During periods of intense geomagnetic activity, strong electric fields and currents pen-etrate from ...
International audienceIt is argued that anisotropic electron pitch angle distributions in the closed...
The two major techniques for the E-region electron temperature measurements, namely, the Langmuir pr...
International audienceWe analyzed 20 reconnection events observed by the Magnetosphere MultiScale mi...
International audienceShock waves are ubiquitous in space and astrophysics. They transform directed ...
International audienceTaking advantage of the string-of-pearls configuration of the five THEMIS spac...
Using EISCAT radar data, we find that electrons are strongly heated in the magnetic field-line dire...
It has been shown in previous studies that at 110 km altitude, the electron temperature can be quite...
International audienceUsing EISCAT data, we have studied the behavior of the E region electron tempe...
We present data from nighttime sounding rocket flights in the low latitude E region. The payloads ca...
International audienceThe electron component of intensive electric currents flowing along the geomag...
In recent years, large electron temperature increases of 300% (3000 K above background) caused by po...
An extensive series of spectral measurements has been made in the auroral E region with the Chatanik...
We have recently implemented a new module that includes both the anomalous electron heating and the ...
We present the first observations of large amplitude waves in a well-defined electron diffusion regi...
During periods of intense geomagnetic activity, strong electric fields and currents pen-etrate from ...
International audienceIt is argued that anisotropic electron pitch angle distributions in the closed...
The two major techniques for the E-region electron temperature measurements, namely, the Langmuir pr...
International audienceWe analyzed 20 reconnection events observed by the Magnetosphere MultiScale mi...
International audienceShock waves are ubiquitous in space and astrophysics. They transform directed ...
International audienceTaking advantage of the string-of-pearls configuration of the five THEMIS spac...