Random Forest Model of Ultralow‐Frequency Magnetospheric Wave Power

Bentley, Sarah, Stout, J. R., Bloch, T. E. and Watt, Clare (2020) Random Forest Model of Ultralow‐Frequency Magnetospheric Wave Power. Earth and Space Science, 7 (10). e2020EA001274. ISSN 2333-5084

[img]
Preview
Text
2020EA001274.pdf - Published Version
Available under License Creative Commons Attribution 4.0.

Download (10MB) | Preview
Official URL: https://doi.org/10.1029/2020EA001274

Abstract

Models of magnetospheric ultralow-frequency (ULF) waves can be used to study wave phenomena and to calculate the effect of these waves on the energization and transport of radiation belt electrons. We present a decision tree ensemble (i.e., a random forest) model of ground-based ULF wave power spectral density driven by solar wind speed vsw, north-south component of the interplanetary magnetic field Bz, and variance of proton number density var(Np). This model corresponds to four radial locations in the magnetosphere (roughly L ∼ 4.21 to 7.94) and spans 1–15 mHz, with hourly magnetic local time resolution. The decision tree ensembles are easier to use than the previous model generation; they have better coverage, perform better at predicting power, and have reduced error due to intelligently chosen bins in parameter space. We outline the difficulties in extracting physics from parameterized models and demonstrate a hypothesis testing framework to iteratively explore finer driving processes. We confirm a regime change for ULF driving about Bz = 0. We posit that ULF wave power directly driven by magnetopause perturbations corresponds to a latitude-dependent dawn-dusk asymmetry, which we see with increasing speed. Model uncertainty identifies where the underlying physics is not fully captured; we find that power due to substorms is less well characterized by Bz > 0, with an effect that is seen globally and not just near midnight. The largest uncertainty is seen for the smallest amounts of solar wind driving, suggesting that internal magnetospheric properties may play a significant role in ULF wave occurrence.

Item Type: Article
Uncontrolled Keywords: ULF waves, radiation belt, machine learning, space weather, magnetosphere, ensemble
Subjects: F500 Astronomy
G900 Others in Mathematical and Computing Sciences
Department: Faculties > Engineering and Environment > Mathematics, Physics and Electrical Engineering
Depositing User: John Coen
Date Deposited: 30 Nov 2020 14:21
Last Modified: 31 Jul 2021 13:51
URI: http://nrl.northumbria.ac.uk/id/eprint/44867

Actions (login required)

View Item View Item

Downloads

Downloads per month over past year

View more statistics