A probabilistic, empirical model of magnetospheric ultra-low frequency wave power

Description

The mean and standard deviation of a series of normal probability distributions, describing magnetospheric ultra-low frequency (ULF, 1-20mHz) plasma waves observed by ground based stations, binned by solar wind properties, station and azimuthal angle (i.e. magnetic local time, or MLT).

This model was constructed using fifteen years of solar wind OMNI data and a latitudinal magnetometer chain from the CANOPUS/CARISMA network.

Resource Type:	Dataset
Creators:	Bentley, Sarah ORCID: https://orcid.org/0000-0002-0095-1979
Rights-holders:	Sarah N Bentley
Data Publisher:	University of Reading
Publication Year:	2019
Data last accessed:	20 October 2024
DOI:	https://doi.org/10.17864/1947.190
Metadata Record URL:	https://researchdata.reading.ac.uk/id/eprint/190
Organisational units:	Science > School of Mathematical, Computational and Physical Sciences > Department of Meteorology
Participating Organisations:	University of Reading
Keywords:	ultra-low frequency (ULF), radiation belts, probabilistic, radial diffusion, magnetosphere, plasma waves, empirical model, space weather
Rights:	Creative Commons Attribution 4.0 International
Data Availability:	OPEN
Additional details Additional details Project Name: SCENARIO Funders: Natural Environment Research Council (NE/L002566/1) Resource Language: English Depositing User: Sarah Bentley Date Deposited: 22 Jan 2019 12:07 Last Modified: 10 May 2023 12:32