activity
20082023
most citedThe radial variation of the solar wind turbulence spectra near the kinetic break scale from Parker Solar Probe measurements

31 citations · 144 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.SR2023★ 19 cited

Oscillatory reconnection as a plasma diagnostic in the solar corona

Konstantinos Karampelas, James A. McLaughlin, Gert J. J. Botha +1

Oscillatory reconnection is a relaxation process in magnetised plasma, with an inherent periodicity that is exclusively dependent on the properties of the background plasma. This s…

astro-ph.SR2022★ 31 cited

The radial variation of the solar wind turbulence spectra near the kinetic break scale from Parker Solar Probe measurements

S. Lotz, A. E. Nel, R. T. Wicks +7

In this study we examine the radial dependence of the inertial and dissipation range indices, as well as the spectral break separating the inertial and dissipation range in power d…

astro-ph.SR2022

The independence of oscillatory reconnection periodicity from the initial pulse

Konstantinos Karampelas, James A. McLaughlin, Gert J. J. Botha +1

Oscillatory reconnection can manifest through the interaction between the ubiquitous MHD waves and omnipresent null points in the solar atmosphere and is characterized by an inhere…

astro-ph.SR2021★ 25 cited

Oscillatory Reconnection of a 2D X-point in a hot coronal plasma

Konstantinos Karampelas, James A. McLaughlin, Gert J. J. Botha +1

Oscillatory reconnection (a relaxation mechanism with periodic changes in connectivity) has been proposed as a potential physical mechanism underpinning several periodic phenomena…

physics.plasm-ph2021★ 8 cited

Shock identification and classification in 2D MHD compressible turbulence -- Orszag-Tang vortex

B. Snow, A. Hillier, G. Murtas +1

Compressible magnetohydrodynamic (MHD) turbulence is a common feature of astrophysical systems such as the solar atmosphere and interstellar medium. Such systems are rife with shoc…

astro-ph.SR2018★ 7 cited

Predictions of DKIST/DL-NIRSP observations for an off-limb kink-unstable coronal loop

B. Snow, G. J. J. Botha, E. Scullion +3

Synthetic intensity maps are generated from a 3D kink-unstable flux rope simulation using several DKIST/DL-NIRSP spectral lines to make a prediction of the observational signatures…