loading page

No statistical link between proton aurora and Pc1 pulsations in the high-latitude dayside using ground-based measurements
  • +2
  • Rowan Alethea Dayton-Oxland,
  • Rowan Dayton-Oxland,
  • Daniel K Whiter,
  • Hyomin Kim,
  • Betty Lanchester
Rowan Alethea Dayton-Oxland

Corresponding Author:[email protected]

Author Profile
Rowan Dayton-Oxland
School of Physics and Astronomy, University of Southampton
Daniel K Whiter
School of Physics and Astronomy, University of Southampton
Hyomin Kim
New Jersey Institute of Technology
Betty Lanchester
School of Physics and Astronomy, University of Southampton

Abstract

In order to test the hypothesis that EMIC waves are responsible for the acceleration of auroral protons, we have used spectrograph measurements of proton aurora over Svalbard alongside co-located magnetometer measurements of Pc1 pulsations. No evidence of a link between proton aurora and Pc1 waves was found by three different methods. Firstly, accelerated protons and Pc1 pulsations have no coincident occurrence. Secondly, the proton energy spectrum does not change between Pc1 activity and quiet times. Finally, no imprint of the EMIC wave is found in periodicity of the intensity and blue-shift of the proton H-α line, unlike in flickering electron aurora where intensity fluctuations are caused by EMIC waves. We find no evidence that EMIC waves are the mechanism responsible for accelerating auroral protons in the high-latitude dayside, at least based on the considered ground-based data of proton aurora and magnetic Pc1 pulsations.
13 Sep 2024Submitted to ESS Open Archive
15 Sep 2024Published in ESS Open Archive