Publications 2020 –


Refereed publications since 2020 (to be completed)

SMTG affiliated authors are listed in boldface

Terradas, J. & Neukirch, T.

Three-dimensional solar active region magnetohydrostatic models and their stability using Euler potentials

Allanson, O., Elsden, T.,  Watt, C. & Neukirch, T.Weak Turbulence and Quasilinear Diffusion for Relativistic Wave-Particle Interactions Via a Markov Approach
Archer, M. O., Southwood, D. J., Hartinger, M. D., Rastaetter, L. & Wright, A. N.How a realistic magnetosphere alters the polarizations of surface, fast magnetosonic, and Alfvén waves
De Pontieu, B., Testa, P., Martínez-Sykora, J., Antolin, P., Karampelas, K., Hansteen, V., Rempel, M., Cheung, M. C. M., Reale, F., Danilovic, S., Pagano, P., Polito, V., De Moortel, I., Nóbrega-Siverio, D., Van Doorsselaere, T., Petralia, A., Asgari-Targhi, M., Boerner, P., Carlsson, M., Chintzoglou, G. & 7 others.Probing the physics of the solar atmosphere with the Multi-slit Solar Explorer (MUSE). I. Coronal heating
Elsden, T. & Wright, A. N.Polarisation properties of 3-D field line resonances
Howson, T. A. & De Moortel, I.The effects of driving time scales on coronal heating in a stratified atmosphere
Madjarska, M., Mackay, D. H., Galsgaard, K., Wiegelmann, T. & Xie, H.Eruptions from coronal bright points: a spectroscopic view by IRIS of a mini-filament eruption, QSL reconnection, and reconnection-driven outflows
Moreno-Insertis, F., Nóbrega-Siverio, D., Priest, E. R. & Hood, A. W.Ambipolar diffusion: self-similar solutions and MHD code testing. Cylindrical symmetry
Pascoe, D. J., Van Doorsselaere, T. & De Moortel, I.Coronal seismology using damping of propagating kink waves
Wright, A., Degeling, A. & Elsden, T.Resonance maps for 3D Alfvén waves in a compressed dipole field
Banerjee, D., Krishna Prasad, S., Pant, V., McLaughlin, J. A., Antolin, P., Magyar, N., Ofman, L., Tian, H., Van Doorsselaere, T., De Moortel, I.& Wang, T. J.Magnetohydrodynamic waves in open coronal structures
Fyfe, L., Howson, T. A., De Moortel, I.,
Pant, V. & Van Doorsselaere, T.
Investigating coronal wave energy estimates using synthetic non-thermal line widths
Fyfe, LE., Howson, TA. & De Moortel, I.Forward modelling of heating within a coronal arcade
Howson, T. A., De Moortel, I. & Pontin, D.Magnetic reconnection and the Kelvin-Helmholtz instability in the solar corona
Johnston, C. D.Cargill, P. J.Antolin, P.Hood, A. W.De Moortel, I.; Bradshaw, S. J.The effects of numerical resolution, heating timescales and background heating on thermal non-equilibrium in coronal loops
Johnston, C. D., Hood, A. W., De Moortel, I.,
Pagano, P. & Howson, T. A.
A fast multi-dimensional magnetohydrodynamic formulation of the transition region adaptive conduction (TRAC) method
Lehmann, L. T., Hussain, G. A. J., Vidotto, A., Jardine, M. M. & Mackay, D. H.Identifying solar-like magnetic cycles with Zeeman-Doppler-Imaging (ZDI)
Mackay, D. H.Solar prominences
Mackay, D. H. & Yeates, A.A comparison of sparse and non-sparse techniques for electric-field inversion from normal-component magnetograms
Prokopyszyn, APK., Wright, AN. & Hood, AW.Line-tied boundary conditions can cause resonant absorption models to generate unphysically large boundary layers
Parnell, C et alCritical Science Plan for the Daniel K. Inouye Solar Telescope (DKIST)
Reid, J., Cargill, P., Johnston, C. D. & Hood, A. W.Linking computational models to follow the evolution of heated coronal plasma
Threlfall, J., Reid, J. & Hood, A. W.Can multi-threaded flux tubes in coronal arcades support a magnetohydrodynamic avalanche?
Viall, N., De Moortel, I., Downs, C., Klimchuk, J. A., Parenti, S. & Reale, F.The heating of the solar corona
Yardley, S. L., Mackay, D. H. & Green, L.Simulating the coronal evolution of bipolar active regions to investigate the formation of flux ropes
Yardley, S. L., Pagano, P., Mackay, D. H.
& Upton, L.
Determining the source and eruption dynamics of a stealth CME using NLFFF modelling and MHD simulations
Zahid, Z., Parnell, C. E. & Qamar, A.3D non-driven magnetic reconnection at multiple separators
Borissov, A., Neukirch, T., Kontar, E.,Threlfall, J. & Parnell, C.Particle acceleration with anomalous pitch angle scattering in 3D separator reconnection
De Moortel, I., Falconer, I. & Stack, R.,Alfvén on heating by waves
Elsden, T. & Wright, A.Evolution of high-m poloidal Alfvén waves in a dipole magnetic field
Fyfe, L., Howson, T. A. & De Moortel, I.Forward modelling of MHD Waves in braided magnetic fields
Howson, T. A., De Moortel, I. & Fyfe, L.The effects of driving time scales on heating in a coronal arcade
Howson, T. A., De Moortel, I. & Reid, J.Phase mixing and wave heating in a complex coronal plasma
Johnston, C. D., Cargill, P. J., Hood, A. W., De Moortel, I., Bradshaw, S. J. & Vaseekar, A. C.
Modelling the solar transition region using an adaptive conduction method
Lehmann, L. T., Hussain, G. A. J., Vidotto, A., Jardine, M. M. & Mackay, D. H.Identifying solar-like magnetic cycles with Zeeman-Doppler-Imaging (ZDI)
Love, T., Neukirch, T. & Parnell, C. E.Analyzing AIA flare observations using convolutional neural networks
Lund, K., Jardine, M., Lehmann, L. T., Mackay, D. H., See, Vidotto, A. A., Donati, J-F., Fares, R., Folsom, C. P., Jeffers, S., Marsden, S. C., Morin, J. & Petit, P.Measuring stellar magnetic helicity density
Mackay, D. H., Schmieder, B., Lopez Ariste, A. & Su, Y.Modelling and observations: a comparison of the magnetic field properties in a prominence
Madjarska, M., Galsgaard, K., Mackay, D. H.,
Koleva, K. & Dechev, M.
Eruptions from coronal hole bright points: observations and non-potential modeling
Meyer, K. A., Mackay, D. H.,
Talpeanu, D-C., Upton, L. & West, M.
Investigation of the middle corona with SWAP and a data-driven non-potential coronal magnetic field model
Neukirch, T., Vasko, I. Y., Artemyev, A. V. & Allanson, O.Kinetic models of tangential discontinuities in the solar wind
Neukirch, T., Wilson, F. & Allanson, O.A family of Vlasov-Maxwell equilibrium distribution functions describing a transition from the Harris sheet to the force-free Harris sheet
Olshevsky, V., Pontin I, D., Williams, B., Parnell, C. E., Fu, H. S., Liu, Y., Yao, S. & Khotyaintsev V, Y.A comparison of methods for finding magnetic nulls in simulations and in situ observations of space plasmas
Pagano, P., Bemporad, A. & Mackay, D. H.Hydrogen non-equilibrium ionisation effects in coronal mass ejections
Pagano, P., De Moortel, I. & Morton,R.Effect of coronal loop structure on wave heating by phase mixing
Patsourakos, S., Vourlidas, A., Török, T., Kliem, B., Antiochos, S. K., Archontis, V., Aulanier, G., Cheng, X., Chintzoglou, G., Georgoulis, M. K., Green, L. M., Leake, J. E., Moore, R., Nindos, A., Syntelis, P., Yardley, S. L., Yurchyshyn, V. & Zhang, JDecoding the pre-eruptive magnetic field configurations of coronal mass ejections
Reid, J., Cargill, P., Hood, A. W., Parnell, C. E. & Arber, T. D.Coronal energy release by MHD avalanches: heating mechanisms
Reid, J., Parnell, C. E., Hood, A. W. & Browning, P. K.Determining whether the squashing factor, Q, would be a good indicator of reconnection in a resistive MHD experiment devoid of null points
Threlfall, J., Wright, A. N. & Hood, A. W.How is helicity (and twist) partitioned in magnetohydrodynamic simulations of reconnecting magnetic flux tubes?
Van Damme, H. J., De Moortel, I., Pagano, P. & Johnston, C. D.Chromospheric evaporation and phase mixing of Alfvén waves in coronal loops
Van Doorsselaere, T., Srivastava, A. K., Antolin, P., Magyar, N., Vasheghani Farahani, S., Tian, H., Kolotkov, D., Ofman, L., Guo, M., Arregui, I., De Moortel, I. & Pascoe, D.Coronal heating by MHD waves
Wiegelmann, T., Neukirch, T., Nickeler, D. & Chifu, I.An optimization principle for computing stationary MHD equilibria with solar wind flow
Wright, A. N. & Elsden, T.Simulations of MHD wave propagation and coupling in a 3D magnetosphere