| 2024 | |
| Allanson, O., Ma, D., Osmane, A., Albert. J. M., Bortnik, J., Watt, C. E. J., Chapman, S. C., Spencer, J., Ratliff, D. J., Meredith, N. P., Elsden, T., Neukirch, T., Hartley, D. P., Black, R., Watkins, N. W. & Elvidge, S. | The challenge to understand the zoo of particle transport regimes during resonant wave-particle interactions for given survey-mode wave spectra |
| Doorsselaere, T. V., Prasad, S. K., Pant, V., Banerjee, D. & Hood, A. | Multithermal apparent damping of slow waves due to strands with a Gaussian temperature distribution |
| Enerhaug, E., Howson, T. A. & De Moortel, I. | Identifying Alfvén wave modes in the solar corona |
| Mondal, S., Srivastava, A.K., Pontin, D.I., Yuan, D. and Priest, E.R | 2.5D MHD simulation of the formation and evolution of plasmoids in coronal current sheets |
| Mondal, S., Srivastava, A.K., Pontin, D.I., Yuan, D. and Priest, E.R. | MHD simulation of the formation and evolution of plasmoids in coronal current sheets |
| Pontin, D. I., Priest, E.R., Chitta, L. P. & Titov, V. S. | Coronal heating and solar wind generation by flux cancellation reconnection |
| Pontin, D.I. and Priest, E.R. | Magnetic Reconnection |
| Wright, A. N., Hartinger, M., Takahashi, K. & Elsden, T. | Alfven waves in the Earth’s magnetosphere |
| 2023 |
| Archer, M. O., Hartinger, M. D., Rastätter, L., Southwood, D. J., Heyns, M., Eggington, J. W. B., Wright, A. N., Plaschke, F. & Shi, X. | Auroral, ionospheric and ground magnetic signatures of magnetopause surface modes |
| Breu, C., Peter, H., Cameron, R. & Solanki, S. K. | Swirls in the solar corona |
| Mulay, S. M., Tripathi, D., Mason, H., Del Zanna, G. & Archontis, V. | Formation and thermodynamic evolution of plasmoids in active region jets |
| Browning, P., Gordovskyy, M. & Hood, A., | Helicity-conserving relaxation in unstable and merging magnetic flux ropes |
| Cheng, X., Priest, E. R., Li, H. T., Chen, J., Aulanier, G., Chitta, L. P., Wang, Y. L., Peter, H., Zhu, X. S., Xing, C., Ding, M. D., Solanki, S. K., Berghmans, D., Teriaca, L., Aznar Cuadrado, R., Zhukov, A. N., Guo, Y., Long, D., Harra, L., Smith, P. J., Rodriguez, L., Verbeeck, C., Barczynski, K. & Parenti , S. | Ultra-high-resolution observations of persistent null-point reconnection in the Solar corona |
| Chitta, L.P., Solanki, SK, del Toro Iniesta, J. C., Woch, J., Calchetti, D., Gandorfer, A., Hirzberger, J., Kahil, F., Valori, G., Orozco Suárez, D. Strecker, H., Appourchaux, T., Volkmer, R., Peter, H., Mandal, S., Aznar Cuadrado, R., Teriaca, L., Schühle, U., Berghmans, D., Verbeeck, C., Zhukov, A.N., Priest, E.R. | Fleeting Small-scale Surface Magnetic Fields Build the Quiet-Sun Corona |
| Cozzo, G., Reid, J., Pagano, P., Reale, F. & Hood, A. W. | Coronal energy release by MHD avalanches: effects on a structured, active region, multi-threaded coronal loop |
| Chouliaras, G., Syntelis, P., Archontis, A. | Effects of Partial Ionization on Magnetic Flux Emergence in the Sun |
| Davies, R. & Wright, A. N. | Alfvén-fast wave coupling in a 2D non-uniform medium |
| Elsden, T. & Southwood, D. | Modeling features of field line resonance observable by a single spacecraft at Saturn |
| Fogg, A, Lester, M., Yeoman, T., Carter, J., Milan, S., Sangha, H., Elsden, T., Wharton, S. J., James, M., Malone-Leigh, J., Paxton, L. J., Anderson, B. J. & Vines, S. K. | Multi-instrument observations of the effects of a solar wind pressure pulse on the high latitude ionosphere: a detailed case study of a geomagnetic sudden impulse |
| Gunár, S., Labrosse, N., Luna, M., Schmieder, B., Heinzel, P., Kucera, T. A., Levens, P. J., López Ariste, A., Mackay, D. H. & Zapiór, M. | On the physical nature of the so-called prominence tornadoes |
| Hartinger, M., Elsden, T., Archer, M., Takahashi, K., Wright, A. N., Artemyev, A., Zhang, X. & Angelopoulos, V. | Properties of magnetohydrodynamic normal modes in the Earth’s magnetosphere |
| Howson, T. & De Moortel, I. | Heating and cooling in transversely oscillating coronal loops powered by broadband, multi-directional wave drivers
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| Howson, T. A. & Breu, C. A. | How numerical treatments of the transition region modify energy flux into the solar corona |
| Priest, E.R. | Human uniqueness: debates in science and theology |
| Priest, E.R. | Magnetic reconnection on the Sun: ESPD Senior Prize Lecture |
| Priest, E.R. | Biography of John Campbell Brown |
| Priest, E.R., Henrich, J., Deane-Drummond, C. and Meyers, M.A. | Introduction to Symposium on “Just How Special are Humans?” |
| Reid, J., Threlfall, J. & Hood, A. W. | Self-consistent nanoflare heating in model active regions: MHD avalanches in curved coronal arcades |
| Russell, A. J. B. | Alfvén waves in solar flares |
| Sandhu, J., Degeling, A. W., Elsden, T., Murphy, K. R., Rae, I. J., Wright, A. N., Hartley, D. P. & Smith, A. | Van Allen probes observations of a three-dimensional field line resonance at a plasmaspheric plume |
| Takahashi, K., Elsden, T., Wright, A. N. & Degeling, A. | Polarization of magnetospheric ULF waves excited by an interplanetary shock on 27 February 2014 |
| Terradas, J. & Neukirch, T. | Three-dimensional solar active region magnetohydrostatic models and their stability using Euler potentials |
| Wright, A. N. & Elsden, T. | Resonant fast-Alfvén wave coupling in a 3D coronal arcade |
| Wright, A. N. | Efficient resonant fast-Alfvén wave coupling as a minimization principle |
| 2022 |
| 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 |
| Barczynski, K., Meyer, K. A., Harra, L. K., Mackay, D. H., Auchère, F. & Berghmans, D. | A statistical comparison of EUV brightenings observed by SO/EUI with simulated brightenings in nonpotential simulations |
| De Moortel, I. & Howson, T. A. | (When) Can wave heating balance optically thin radiative losses in the corona? |
| 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 |
| Elsden, T., James, M., Sandhu, J. & Watt, C. | RAS specialist discussion meeting report |
| Elsden, T., Wright, A. N. & Degeling, A. | A review of the theory of 3D Alfvén (field line) resonances |
| Elsden, T., Yeoman, T.K., Wharton, S.J., Rae, I.J., Sandhu, J.K., Walach, M-T., James, M.K., & Wright, D.M. | Modeling the varying location of field line resonances during geomagnetic storms |
| Howson, T. A. & De Moortel, I. | The effects of driving time scales on coronal heating in a stratified atmosphere |
| Mackay, D. H. & Upton, L. | A comparison of global magnetofrictional simulations of the 2015 March 20 solar eclipse |
| 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., De Moortel, I., Pagano, P. & Howson, T. A. | Propagating Alfvén waves in open structures with random structuring |
| Pascoe, D. J., Van Doorsselaere, T. & De Moortel, I. | Coronal seismology using damping of propagating kink waves |
| Pontin, D.I. and Priest, E.R. | Magnetic reconnection: MHD theory and modelling |
| Reid, J., Threlfall, J. & Hood, A. W. | MHD avalanches in magnetized solar plasma: proliferation and heating in coronal arcades |
| Sakurai, T., Wright, A. N., Takahashi, K., Elsden, T., Ebihara, Y., Sato, N., Kadokura, A., Tanaka, Y. & Hori, T. | Poleward moving auroral Arcs and Pc5 oscillations |
| Wright, A., Degeling, A. & Elsden, T. | Resonance maps for 3D Alfvén waves in a compressed dipole field |
| Yan, X., Xue, Z., Jiang, C., Priest, E.R., Kliem, B., Yang, L., Wang, J., Kong, D., Song, Y., Feng, X., and Liu, Z. | Fast plasmoid-mediated reconnection in a solar flare |
| Zhu, X., Neukirch, T. & Wiegelmann, T. | Magnetohydrostatic modeling of the solar atmosphere |
| 2021 |
| 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 |
| Rast, M.P., González, N.B., Rubio, L.B., Cao, W., Cauzzi, G., DeLuca, E., De Pontieu, B., Fletcher, L., Gibson, S.E., Judge, P.G., Parnell, C.E., et al | Critical 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 |
| 2020 |
| 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, J | Decoding 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 |