Energetic electron precipitation associated with pulsating aurora: EISCAT and Van Allen Probe observations
By Yoshizumi Miyoshi, S. Oyama, S. Saito, S. Kurita, Hitoshi Fujiwara, R. Kataoka, Yusuke Ebihara, Craig Kletzing, G. Reeves, O. Santolík and 4 more. 2015
170 citations recorded by the source corpus.
Pulsating auroras show quasi‐periodic intensity modulations caused by the precipitation of energetic electrons of the order of tens of keV. It is expected theoretically that not only these electrons but also subrelativistic/relativistic electrons precipitate simultaneously into the ionosphere owing to whistler mode wave‐particle interactions. The height‐resolved electron density profile was observed with the European Incoherent Scatter (EISCAT) Tromsø VHF radar on 17 November 2012. Electron density enhancements were clearly identified at altitudes >68 km in association with the pulsating aurora, suggesting precipitation of electrons with a broadband energy range from ~10 keV up to at least 200 keV. The riometer and network of subionospheric radio wave observations also showed the energetic electron precipitations during this period. During this period, the footprint of the Van Allen Probe‐A satellite was very close to Tromsø and the satellite observed rising tone emissions of the lower band chorus (LBC) waves near the equatorial plane. Considering the observed LBC waves and electrons, we conducted a computer simulation of the wave‐particle interactions. This showed simultaneous precipitation of electrons at both tens of keV and a few hundred keV, which is consistent with the energy spectrum estimated by the inversion method using the EISCAT observations. This result revealed that electrons with a wide energy range simultaneously precipitate into the ionosphere in association with the pulsating aurora, providing the evidence that pulsating auroras are caused by whistler chorus waves. We suggest that scattering by propagating whistler simultaneously causes both the precipitations of subrelativistic electrons and the pulsating aurora.
Subfields: Aerospace Engineering, Astronomy and Astrophysics, Geophysics
View Paper: https://www.semanticscholar.org/paper/af6a59a69f36e83618f65b2a7d9c5837c18f4df1
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In Astronomy and Astrophysics
- J. Fennell
- C. Crabtree
- Xinlin Li
- J. Ripoll
- Seth G. Claudepierre
- C. Colpitts
- A. Y. Ukhorskiy
- R. Thorne
In Geophysics
- J. Fennell
- C. Crabtree
- Xinlin Li
- J. Ripoll
- Seth G. Claudepierre
- C. Colpitts
- A. Y. Ukhorskiy
- R. Thorne
Citations in the corpus
- Particle Dynamics in the Earth's Radiation Belts: Review of Current Research and Open Questions (2020, background): “This is a dominant scattering process outside of the plasmasphere leading to diffuse auroral precipitation (e.g., Johnstone et al., 1993; Miyoshi et al., 2010, 2015; Ni et al., 2011; Nishimura et al., 2010; Oyama et al., 2017; Thorne et al., 2010).”