Mathew Owens

Professor of Space Physics

University of Reading

United Kingdom

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About

Mathew Owens is a Professor of Space Physics at the University of Reading in the United Kingdom. His research areas include solar wind forecasting, ionospheric irregularity, and the statistical analysis of solar and cometary interactions. Recent publications highlight his work on quantifying predictability in solar wind parameters and advancements in understanding auroral activity over extended timeframes.

Articles (29)

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Collaborators (23)

Benjamin Pope

Lecturer in Astrophysics

University of Queensland

AUSTRALIA

Mathew Owens

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About

Articles (29)

Advancing Ionospheric Irregularity Reconstruction With ICON/MIGHTI Wind‐Driven Insights

Quantifying Uncertainties in Solar Wind Forecasting due to Incomplete Solar Magnetic Field Information

Sub‐Auroral Heating at Jupiter Following a Solar Wind Compression

Analog Ensemble Forecasts of Solar Wind Parameters: Quantification of the Predictability and Time‐Domain Spectral Performance

The 2024 May event in the context of auroral activity over the past 375 yr

Implications of Using Spheroidal “Cone Model” CMEs in Solar‐Wind Models

Statistical Analysis of Comet Disconnection Events Using STEREO HI and a Data-assimilative Solar Wind Model

A Geomagnetic Estimate of Heliospheric Modulation Potential over the Last 175 Years

On the Origin of the Sudden Heliospheric Open Magnetic Flux Enhancement During the 2014 Pole Reversal

Solar Wind Interactions with Comet C/2021 A1 Using STEREO HI and a Data-assimilative Solar Wind Model

A Multi‐Model Ensemble System for the Outer Heliosphere (MMESH): Solar Wind Conditions Near Jupiter

Multi-source connectivity as the driver of solar wind variability in the heliosphere

Analyses for graphical records for a total solar eclipse in 1230 May: a possible reference for the ‘Medieval Grand Maximum’

Tracking solar radio bursts using Bayesian multilateration

Reconstruction of Carrington Rotation Means of Open Solar Flux over the Past 154 Years

Constraints on Solar Wind Density and Velocity Based on Coronal Tomography and Parker Solar Probe Measurements

Coronal Models and Detection of the Open Magnetic Field

Adapting Ensemble‐Calibration Techniques to Probabilistic Solar‐Wind Forecasting

Solar Wind Data Assimilation in an Operational Context: Use of Near‐Real‐Time Data and the Forecast Value of an L5 Monitor

SIR‐HUXt—A Particle Filter Data Assimilation Scheme for CME Time‐Elongation Profiles

Universal Time Variations in the Magnetosphere and the Effect of CME Arrival Time: Analysis of the February 2022 Event that Led to the Loss of Starlink Satellites

Sensitivity of Model Estimates of CME Propagation and Arrival Time to Inner Boundary Conditions

Causal Analysis of Influence of the Solar Cycle and Latitudinal Solar-Wind Structure on Co-Rotation Forecasts

Solar Energetic-Particle Ground-Level Enhancements and the Solar Cycle

Rate of Change of Large-Scale Solar-Wind Structure

Modelling cosmic radiation events in the tree-ring radiocarbon record

Quantifying the Effect of ICME Removal and Observation Age for in Situ Solar Wind Data Assimilation

Predictive Capabilities of Corotating Interaction Regions Using STEREO and Wind In‐Situ Observations

Evidence From Galactic Cosmic Rays That the Sun Has Likely Entered a Secular Minimum in Solar Activity

Collaborators (23)

Benjamin Pope

Mike Lockwood

Manuela Temmer

Deborah Baker

Christopher Scott

Konstantin Herbst

Tom Stallard

Yosuke Yamazaki

Andrea Scifo

Huw Morgan

David Long

Koji Murata

Andrew Smith

Harriet Turner

Luke Barnard

Eleanna Asvestari

James O'Donoghue

Nachiketa Chakraborty

jack connerney

Ilya Usoskin

Shannon R. Jones

Peter Gallagher

Lisa Upton

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