Abstract
We examine the nature of flows in the nightside auroral zone ionosphere and their relationship with concurrent geomagnetic activity by studying a three-hour interval of ground-based radar, magnetometer array and spacecraft data. We find that the flows are bursty in nature, a characteristic previously reported, and that the bursts are related to a series of substorm electrojet intensifications initiated in the pre-midnight sector.
Original language | English |
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Pages (from-to) | 135-138 |
Number of pages | 4 |
Journal | ADVANCES IN SPACE RESEARCH |
Volume | 13 |
Issue number | 4 |
Publication status | Published - Apr 1993 |
Keywords
- EISCAT