A period (08:10–14:40 MLT, 11 February 1997) of enhanced electron density in the D- and E-regions is investigated using EISCAT, IRIS and other complementary instruments. The precipitation is determined to be due to substorm processes occurring close to magnetic midnight. Energetic electrons drift eastward after substorm injection and precipitate in the morning sector. The precipitation is triggered by small pulses in the solar wind pressure, which drive wave particle interactions. The characteristic energy of precipitation is inferred from drift timing on different L-shells and apparently verified by EISCAT measurements. The IMF influence on the precipitation in the auroral zone is also briefly discussed. A large change ...
Patterns of the precipitation of low energy electrons observed by polar satellites were examined as ...
Cosmic radio noise absorption (CNA) events associated with equatorward drifting arcs during a subst...
Substorms are short-lived but significant reconfigurations of the geomagnetic field during which ene...
A period (08:10–14:40 MLT, 11 February 1997) of enhanced electron density in the D- and E-regions is...
A period (08:10–14:40 MLT, 11 February 1997) of enhanced electron density in the D- and E-regions is...
DMSP F7 spacecraft observations for the whole of 1986 were used to construct the empir...
Using magnetically conjugate data from DMSP and ground all-sky TV instruments, temporal change in la...
Abstract It is well known that auroral patterns at the substorm recovery phase are characterized by...
Simultaneous observations with the IRIS, DASI and EISCAT systems are employed in the study of the ...
International audienceDMSP F7 spacecraft observations for the whole of 1986 were used to construct t...
18th EISCAT symposiumSession E6: The ERG mission and magnetosphere-ionosphere couplingMay 26 (Fri), ...
Abstract. The effects of energetic electron precipitation into the auroral region at a time of enhan...
The effects of energetic electron precipitation into the auroral region at a time of enhanced solar...
Using the data from satellite CRRES and three geostationary LANL spacecraft, the propagation of an ...
The IMAGE spacecraft obtained the first global images of the proton aurora. One of the discoveries ...
Patterns of the precipitation of low energy electrons observed by polar satellites were examined as ...
Cosmic radio noise absorption (CNA) events associated with equatorward drifting arcs during a subst...
Substorms are short-lived but significant reconfigurations of the geomagnetic field during which ene...
A period (08:10–14:40 MLT, 11 February 1997) of enhanced electron density in the D- and E-regions is...
A period (08:10–14:40 MLT, 11 February 1997) of enhanced electron density in the D- and E-regions is...
DMSP F7 spacecraft observations for the whole of 1986 were used to construct the empir...
Using magnetically conjugate data from DMSP and ground all-sky TV instruments, temporal change in la...
Abstract It is well known that auroral patterns at the substorm recovery phase are characterized by...
Simultaneous observations with the IRIS, DASI and EISCAT systems are employed in the study of the ...
International audienceDMSP F7 spacecraft observations for the whole of 1986 were used to construct t...
18th EISCAT symposiumSession E6: The ERG mission and magnetosphere-ionosphere couplingMay 26 (Fri), ...
Abstract. The effects of energetic electron precipitation into the auroral region at a time of enhan...
The effects of energetic electron precipitation into the auroral region at a time of enhanced solar...
Using the data from satellite CRRES and three geostationary LANL spacecraft, the propagation of an ...
The IMAGE spacecraft obtained the first global images of the proton aurora. One of the discoveries ...
Patterns of the precipitation of low energy electrons observed by polar satellites were examined as ...
Cosmic radio noise absorption (CNA) events associated with equatorward drifting arcs during a subst...
Substorms are short-lived but significant reconfigurations of the geomagnetic field during which ene...