Characteristics of auroral electron precipitation at 1 geomagnetic latitude 67° over Tromsø
Habtamu Wubie Tesfaw, Habtamu Wubie Tesfaw, Ilkka Virtanen, Anita T Aikio
Abstract
Habtamu Wubie Tesfaw, Habtamu Wubie Tesfaw, Ilkka Virtanen, Anita T Aikio
Abstract
Key Points: 5 • We use EISCAT UHF ISR data to study the 1-100 keV electron precipitation at 6 66.7° MLAT observed during 21 years 7 • Large auroral powers (≥60 mWm −2) are observed in the 18-02 MLT sector, and 8 mainly in the main auroral oval 9 • Peak energies higher than 50 keV are observed only after 22 MLT and preferen-10
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Key Points: 5 • We use EISCAT UHF ISR data to study the 1-100 keV electron precipitation at 6 66.7° MLAT observed during 21 years 7 • Large auroral powers (≥60 mWm −2) are observed in the 18-02 MLT sector, and 8 mainly in the main auroral oval 9 • Peak energies higher than 50 keV are observed only after 22 MLT and preferen-10
Key concepts: Electron precipitation, Precipitation, Geomagnetic latitude, Radar, Earth's magnetic field, Physics, Atmospheric sciences, Ionosphere