activity
20042023
most citedAn Observational Overview of Solar Flares

850 citations · 4.1k across the 83 of their papers we have counts for

collaborators

82 papers

astro-ph.SR2023★ 17 cited

Statistical analysis of the onset temperature of solar flares in 2010-2011

Douglas Félix da Silva, Li Hui, Paulo J. A. Simões +7

Understanding the physical processes that trigger solar flares is paramount to help with forecasting space weather and mitigating the effects on our technological infrastructure. A…

astro-ph.SR2023★ 40 cited

The F-CHROMA grid of 1D RADYN flare models

Mats Carlsson, Lyndsay Fletcher, Joel Allred +6

Context: Solar flares are the result of the sudden release of magnetic energy in the corona. Much of this energy goes into accelerating charged particles to high velocity. These pa…

astro-ph.SR2023

Specialist Discussion Meeting: 3D structure of the flare chromosphere

David Kuridze, Lyndsay Fletcher, Hugh Hudson

David Kuridze, Lyndsay Fletcher and Hugh Hudson report on the RAS Specialist Discussion Meeting '3D Structure of the Flare Chromosphere'.

astro-ph.SR2022★ 19 cited

Flare Kernels May be Smaller than You Think: Modelling the Radiative Response of Chromospheric Plasma Adjacent to a Solar Flare

Christopher M. J. Osborne, Lyndsay Fletcher

Numerical models of solar flares typically focus on the behaviour of directly-heated flare models, adopting magnetic field- aligned, plane-parallel methodologies. With high spatial…

astro-ph.IM2022

Development of Integral Field Spectrographs to Revolutionize Spectroscopic Observations of Solar Flares and other Energetic Solar Eruptions

Haosheng Lin, Tetsu Anan, Gianna Cauzzi +9

The Sun's proximity offers us a unique opportunity to study in detail the physical processes on a star's surface; however, the highly dynamic nature of the stellar surface -- in pa…

astro-ph.SR2022★ 8 cited

Fast Prograde Coronal Flows in Solar Active Regions

Hugh S. Hudson, Sargam M. Mulay, Lyndsay Fletcher +6

We report the discovery and characterization of high-speed (>100 km/s) horizontal flows in solar active regions, making use of the Sun-as-a-star spectroscopy in the range 5-105 nm…