In this paper, the mechanisms of field-aligned current (FAC) and westward electrojet generation are considered on the base of space measurements and laboratory simulation. Upward and downward FAC are generated in the Earth magnetotail current sheet (CS) due to the tail earthward electric field. They are connected in the ionosphere by the Pedersen current. The FAC enhancement takes place during magnetic reconnection and explosive energy release at a substorm. Electron acceleration in upward FAC produces fast electron precipitation and aurora appearance. The westward electrojet (Hall current) is located between two opposite directed sheets of FAC. The current in the jet is determined by the Hall conductivity in the ionosphere. The similar cur...
We present a simple (stationary) mechanism capable of generating the auroral downward field-aligned ...
The aurora shows explosive activities a few times in 24 h on a moderately active day. This specific ...
Energetic O⁺ ions are rapidly enhanced in the inner magnetosphere because of abrupt intensification ...
Special issue featuring the invited talks from the 44th EPS Conference on Plasma Physics, Belfast, 2...
Although the particle carriers of field-aligned currents (FACs) in the Earth's magnetotail play an i...
The Ninth Symposium on Polar Science/Ordinary sessions: [OS] Space and upper-atmosphere sciences, We...
Our studies elucidated the relationship between the auroral arcs and magnetotail phenomena. One pape...
International audienceWe investigate variations in the location and intensity of the auroral electro...
Dissertation (Ph.D.) University of Alaska Fairbanks, 1990This dissertation reports a study of the ge...
There are shortly described results of the analysis of variations in the location and intensity of t...
In this paper we present observations of a substorm field-aligned current (FAC) system that DMSP F7 ...
International audienceBased on 1829 well-defined substorm onsets in the Northern Hemisphere, observe...
Following a brief review of the processes which have been suggested for explaining the occurrence of...
The substorm current wedge (SCW), a core element of substorm dynamics coupling the magnetotail to th...
Precipitation from the inner edge of the electron plasma sheet creates a density maximum in the auro...
We present a simple (stationary) mechanism capable of generating the auroral downward field-aligned ...
The aurora shows explosive activities a few times in 24 h on a moderately active day. This specific ...
Energetic O⁺ ions are rapidly enhanced in the inner magnetosphere because of abrupt intensification ...
Special issue featuring the invited talks from the 44th EPS Conference on Plasma Physics, Belfast, 2...
Although the particle carriers of field-aligned currents (FACs) in the Earth's magnetotail play an i...
The Ninth Symposium on Polar Science/Ordinary sessions: [OS] Space and upper-atmosphere sciences, We...
Our studies elucidated the relationship between the auroral arcs and magnetotail phenomena. One pape...
International audienceWe investigate variations in the location and intensity of the auroral electro...
Dissertation (Ph.D.) University of Alaska Fairbanks, 1990This dissertation reports a study of the ge...
There are shortly described results of the analysis of variations in the location and intensity of t...
In this paper we present observations of a substorm field-aligned current (FAC) system that DMSP F7 ...
International audienceBased on 1829 well-defined substorm onsets in the Northern Hemisphere, observe...
Following a brief review of the processes which have been suggested for explaining the occurrence of...
The substorm current wedge (SCW), a core element of substorm dynamics coupling the magnetotail to th...
Precipitation from the inner edge of the electron plasma sheet creates a density maximum in the auro...
We present a simple (stationary) mechanism capable of generating the auroral downward field-aligned ...
The aurora shows explosive activities a few times in 24 h on a moderately active day. This specific ...
Energetic O⁺ ions are rapidly enhanced in the inner magnetosphere because of abrupt intensification ...