activity
20062026
most citedThe optical depth of white-light flare continuum

18 citations · 71 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.EP2026

Plasma chemistry and electron-moderated pathways in substellar atmospheres: a new perspective on the L/T transition

Matthew I. Swayne, Declan A. Diver, Craig R. Stark

The long-standing puzzle of the CO/CH transition in brown dwarfs endures. Although the bulk spectral evolution across an atmosphere can be accounted for through thermal equil…

physics.plasm-ph2025

Negative charge acquisition by isolated single microdroplets from plasma exposure at atmospheric pressure

Nourhan Hendawy, Harold McQuaid, Somhairle Mag Uidhir +4

Charged liquid microdroplets have generated significant interest recently due to the observation of chemical reaction rate enhancement by orders of magnitude. Droplet charging by p…

physics.plasm-ph2025★ 1 cited

Free electron charging of microdroplets in a plasma at atmospheric pressure

Nourhan Hendawy, Harold McQuaid, Somhairle Mag Uidhir +4

Gas-phase microdroplets have recently demonstrated exceptional chemical properties via suspected mechanisms such as contact electrification and surface charge pinning, producing hi…

astro-ph.EP2025

Electrostatic instability of non-spherical dust in sub-stellar clouds

Craig R. Stark, Declan A. Diver, Matthew I. Swayne

Charged dust clouds play an important role in the evolution of sub-stellar atmospheres through electrical discharges such as lightning events or inter-grain discharges. The consequ…

astro-ph.SR2024

An impulsive geomagnetic effect from an early-impulsive flare

Hugh S. Hudson, Edward. W. Cliver, Lyndsay Fletcher +6

The geomagnetic "solar flare effect" (SFE) results from excess ionization in the Earth's ionosphere, famously first detected at the time of the Carrington flare in 1859. This indir…

astro-ph.SR2020★ 2 cited

Evolution of spheroidal dust in electrically active sub-stellar atmospheres

Craig R. Stark, Declan A. Diver

Understanding the source of sub-stellar polarimetric observations in the optical and near-infrared is key to characterizing sub-stellar objects and developing potential diagnostics…