collaborators

5 papers

astro-ph.SR2025

Investigating the Efficacy of Topologically Derived Time Series for Flare Forecasting. II. XGBoost Model

Thomas Williams, Christopher B. Prior, David MacTaggart +1

Solar flares are a primary driver of space weather, and forecasting their occurrence remains a significant challenge. This paper presents a novel flare prediction model based on to…

astro-ph.SR2025

On field line slippage rates in the solar corona

David MacTaggart

Magnetic reconnection is one of the fundamental dynamical processes in the solar corona. The method of studying reconnection in active region-scale magnetic fields generally depend…

physics.plasm-ph2024

On turbulent magnetic reconnection: fast and slow mean steady-states

Sage Stanish, David MacTaggart

We investigate a model of turbulent magnetic reconnection introduced by Higashimori, Yokoi and Hoshino (Phys. Rev. Lett. 110, 255001) and show that the classic two-dimensional, ste…

astro-ph.SR2024

Investigating the Efficacy of Topologically Derived Time-Series for Flare Forecasting. I. Dataset Preparation

Thomas Williams, Christopher B. Prior, David MacTaggart

The accurate forecasting of solar flares is considered a key goal within the solar physics and space weather communities. There is significant potential for flare prediction to be…

astro-ph.SR2024

The magnetic topology of AR13664 leading to its first halo CME

David MacTaggart, Tom Williams, OPM Aslam

In the first half of May 2024, the solar active region (AR)13664 was responsible for generating the strongest geomagnetic storm in over 20 years, through an enhanced production of…