Richard Horne

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British Antarctic Survey

United Kingdom

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Recent Grants

Grant: Close

Modelling the acceleration, transport and loss of radiation belt electrons to protect satellites from space weather (Rad-Sat)

Open Date: 2017-04-30

Close Date: 2021-04-29

Grant: Close

Electron Acceleration, Transport and Loss in Planetary Radiation Belts

Open Date: 2015-03-31

Close Date: 2019-03-31

Grant: Close

BAS Space Weather and Atmosphere

Open Date: 2015-03-31

Close Date:

Grant: Close

NOx and HOx production by energetic electrons and impacts on polar stratospheric ozone (NOHO)

Open Date: 2013-06-29

Close Date: 2016-12-31

Grant: Close

Origin of electron acceleration in the radiation belts of Earth, Jupiter and Saturn

Open Date: 2012-01-16

Close Date: 2016-01-15

Articles (25)

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2022

Collaborators (8)

Lunjin Chen

UNITED STATES

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Clare Watt

Northumbria University

UNITED KINGDOM

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AKIRA KADOKURA

National Institute of Polar Research

JAPAN

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Adam Kellerman

UNITED STATES

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Zhiyang Xia

UNITED STATES

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Harlan E. Spence

UNITED STATES

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K. R. Murphy

UNITED KINGDOM

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Iain Jonathan Rae

University College London

UNITED KINGDOM

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Richard Horne

Research Interests

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Recent Grants

Articles (25)

Modeling the Internal Redistribution of Earth's Proton Radiation Belt by Interplanetary Shocks

Satellite Internal Charging for a Reasonable Worst‐Case

Ray tracing of very low frequency waves produced by active experiments or lightning events at low Earth orbit

On the Wave‐Normal Distribution of Lightning‐Generated Whistlers and Their Propagation Modes

Modeling Field Line Curvature Scattering Loss of 1–10 MeV Protons During Geomagnetic Storms

Review of the August 1972 and March 1989 (Allen) Space Weather Events: Can We Learn Anything New From Them?

Measuring Low Plasma Density in the Earth's Equatorial Magnetosphere From Magnetosonic Waves

A New Model of Electron Pitch Angle Distributions and Loss Timescales in the Earth's Radiation Belts

Chorus wave power at the strong diffusion limit overcomes electron losses due to strong diffusion

Propagation of Very Oblique Chorus Waves Near a Plasmaspheric Plume Boundary

Characterizing Radiation‐Belt Energetic Electron Precipitation Spectra: A Comparison of Quasi‐Linear Diffusion Theory With In Situ Measurements

New Chorus Diffusion Coefficients for Radiation Belt Modeling

Reproducing Ultra‐Relativistic Electron Acceleration Using a Coupled Density and Radiation Belt Model

Strong Relativistic Electron Flux Events in GPS Orbit

The April 2023 SYM‐H = −233 nT Geomagnetic Storm: A Classical Event

A New Four‐Component L*‐Dependent Model for Radial Diffusion Based on Solar Wind and Magnetospheric Drivers of ULF Waves

Modeling the Propagation of Fast Magnetosonic Waves and Their Conversion to Electromagnetic Ion Cyclotron Waves at Low L Shells

Extreme Relativistic Electron Fluxes in GPS Orbit: Analysis of NS41 BDD‐IIR Data

Modeling the Effects of Drift Shell Splitting in Two Case Studies of Simultaneous Observations of Substorm‐Driven Pi1B and IPDP‐Type EMIC Waves

The Importance of Ion Composition for Radiation Belt Modeling

Variations in Observations of Geosynchronous Magnetopause and Last Closed Drift Shell Crossings With Magnetic Local Time

Whistler Waves Above the Lower Hybrid Frequency in the Ionosphere and Their Counterparts in the Magnetosphere

Electron Diffusion by Magnetosonic Waves in the Earth’s Radiation Belts

Ducted Chorus Waves Cause Sub‐Relativistic and Relativistic Electron Microbursts

Attention‐Based Machine Vision Models and Techniques for Solar Wind Speed Forecasting Using Solar EUV Images

Collaborators (8)

Lunjin Chen

Clare Watt

AKIRA KADOKURA

Adam Kellerman

Zhiyang Xia

Harlan E. Spence

K. R. Murphy

Iain Jonathan Rae

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