Andrew Wright - Observations & Simulations of 3D Field Lines Resonances in the Earth's Magnetosphere
Andrew Wright (University of St Andrews) - Observations and Simulations of 3D Field Lines Resonances in the Earth'sΒ ...
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Search every verified Andrew Wright interview, podcast appearance, and on-the-record quote β each transcript cross-checked by AI and human review to confirm speaker identity. Andrew Wright, a reader in the solar and magnetospheric MHD theory group at the University of St Andrews, presented a seminar on September 17, 2024, titled "Observations and Simulations of 3D Field Lines Resonances in the Earth's Magnetosphere." In the talk, Wright discussed the lowest frequency MHD waves, describing how fast modes propagate cross field lines and transport energy from the magnetopause into the magnetosphere. He noted that in a non-uniform medium, these waves are coupled, comparing the effect to nudging a jelly on a plate. Wright stated that his team has "figured out the way of getting the AlfvΓ©n frequency for an arbitrary polarization," moving beyond traditional toroidal and poloidal frequencies. He identified data from the Van Allen probes as "a good candidate for a 3D field line resonance," particularly in the afternoon region where strong variations of azimuthal polarization are expected. Wright emphasized that the research has highlighted "how important the cold plasma density is for controlling MHD wave dynamics," especially in structures like plumes. He argued that rotating away from traditional 2D azimuthal polarization is significant for how these waves interact with radiation belt particles, calling this "the subject of ongoing research." Wright also referenced a review paper written by his team members that outlines the current understanding of 3D field line resonance theory.
“The way the waves I'm going to be talking about are the lowest frequency MHD waves of the system β for example the fast modes which propagate cross field lines transport energy from the magnetopause into the magnetosphere.”
“When you have a non-uniform medium these two waves are coupled together β imagine having an impulsive solar wind nudge, it's a bit like if you nudge a jelly on a plate it'll reverberate with its natural frequencies.”
“If you're up here well things change quite dramatically as you cross the plume boundaries β if you want to study wave coupling in these sort of regions then you're really going to need 3D theory.”
“It's been realized you can have actually any intermediate polarization and you can work out the frequency β we've figured out the way of getting the AlfvΓ©n frequency for an arbitrary polarization.”
“The most reliable way we found was to look at hodograms β on a satellite of the perpendicular fields of the AlfvΓ©n wave you should see something like this.”
“When you cross the plume you should see a rotation at the plume boundaries either in this sense or this sense depending which boundary you're on.”
“Van Allen probes data β it's exactly the right place in the afternoon, that's where we expect these strong variations of azimuthal to occur β this is a good candidate for a 3D field line resonance.”
“It's really brought home how important the cold plasma density is for controlling MHD wave dynamics, particularly when you've got structures like plumes, and rotating away from the traditional 2D azimuthal polarization is important for how these waves will interact with radiation belt particles.”
Andrew Wright (University of St Andrews) - Observations and Simulations of 3D Field Lines Resonances in the Earth'sΒ ...
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