Conference proceeding
The Evolution of Chorus Emissions Over Time and Magnetic Latitude
2023 International Conference on Electromagnetics in Advanced Applications (ICEAA), pp.406-406
10/09/2023
DOI: 10.1109/ICEAA57318.2023.10297941
Abstract
Chorus wave emissions are pervasive electromagnetic waves observed throughout the inner magnetosphere, and can intensify significantly during enhanced geomagnetic activity. Chorus waves have been shown to drive a particular type of precipitation that is composed of ring current and radiation belt losses and results in the quasi-periodic optical ionospheric phenomenon called pulsating aurora. Understanding how chorus waves evolve over time following periods of generation and rapid growth (i.e. injection-driven) and how they evolve as they propagate from equatorial sources to higher magnetic latitudes will lead to insights about how they drive energetic electron precipitation.
Details
- Title: Subtitle
- The Evolution of Chorus Emissions Over Time and Magnetic Latitude
- Creators
- Allison N. Jaynes - University of IowaRiley N. Troyer - University of IowaKeith R. Vidal - University of Iowa
- Resource Type
- Conference proceeding
- Publication Details
- 2023 International Conference on Electromagnetics in Advanced Applications (ICEAA), pp.406-406
- Publisher
- IEEE
- DOI
- 10.1109/ICEAA57318.2023.10297941
- eISSN
- 2766-2284
- Language
- English
- Date published
- 10/09/2023
- Academic Unit
- University College Courses; Physics and Astronomy
- Record Identifier
- 9984507158802771
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