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  • Presentation | SM51D: Revealing the Mysteries of High-Latitude Currents from Above and Below II Poster
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  • SM51D-1170: Investigating Ultra Low Frequency Pi1B waves as a proxy for substorm onset
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Author(s):
Michelle Salzano, Space Science Institute Boulder (First Author, Presenting Author)
Michael Hartinger, Space Science Institute Boulder
Kristina Collins, Space Science Institute Boulder
Marc Lessard, University of New Hampshire
Kazuo Shiokawa, Nagoya University
Zhonghua Xu, University of Texas at Arlington
Jesper Gjerloev, Johns Hopkins University, Applied Physics Laboratory
Atsuki Shinbori, Nagoya University
Shin-ichiro Oyama, National Institute of Polar Research
Martin Connors, Athabasca University


Space weather events have the ability to seriously impact satellites in orbit, power grids on earth, and many facets of modern life and society. While sometimes its effects on the public are limited to the Northern Lights and similar impressive displays, other times it can lead to massive and prolonged power outages, endangering the lives of those affected. In order to predict and account for space weather and its effects, it is necessary to understand the dynamics and processes involved. This research looks into a type of space weather event called a substorm. While we have many ways to study substorms in the Northern Hemisphere, there is not enough land coverage in the Southern Hemisphere to be able to use the same methods. Space weather can have different effects across the two hemispheres, and it is important to be able to study both areas at once. This research investigates if a different kind of space weather event can be used as a proxy to study substorms, and if so, if it can be used consistently and reliably to study substorms in both hemispheres.



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