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Characteristics of auroral electron precipitation at 1 geomagnetic latitude 67° over Tromsø
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  • Habtamu W. Tesfaw,
  • Habtamu W Tesfaw,
  • Ilkka I Virtanen,
  • Anita T Aikio
Habtamu W. Tesfaw

Corresponding Author:[email protected]

Author Profile
Habtamu W Tesfaw
Space Physics and Astronomy Research Unit, University of Oulu
Ilkka I Virtanen
Space Physics and Astronomy Research Unit, University of Oulu
Anita T Aikio
Space Physics and Astronomy Research Unit, University of Oulu

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
19 May 2023Submitted to ESS Open Archive
25 May 2023Published in ESS Open Archive