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Read more at: About the group

About the group

The group carries out research into a wide range of topics involving astrophysical fluid dynamics and nonlinear dynamics. Specific astrophysical interests include the dynamics of astrophysical discs, planetary formation and evolution, extrasolar planetary systems and stellar magnetohydrodynamics (particularly dynamo theory, magnetoconvection and the physics of sunspots).


Read more at: Vacancies

Vacancies

Applications are welcomed for PhD studentships in the Astrophysics group (closing date 4 January 2024).



Read more at: PhD opportunties

PhD opportunties

A wide range of possible research topics is available and we welcome enquiries from potential applicants. The closing date for applications is 4 January 2024.


Read more at: Astrophysical dynamics

Astrophysical dynamics

Discs are ubiquitous in astrophysics and participate in some of its most important processes. Most, but not all, feed a central mass: by facilitating the transfer of angular momentum, they permit the accretion of material that would otherwise stay in orbit. As a consequence, discs are essential to star, planet and satellite formation. They also regulate the growth of supermassive black holes and thus indirectly influence galactic structure and the intra-cluster medium.



Read more at: Atomic astrophysics

Atomic astrophysics

Atomic physics plays a key role in astrophysics as astronomers' only information about a particular object comes through the light that it emits, and this light arises through atomic transitions. The main astronomical body that we study is the Sun and, in particular, the hot atmosphere of the Sun called the corona. The best parts of the electromagnetic spectrum to study the corona are the extreme ultraviolet (EUV) and X-rays.



 

Recent Publications

CHIANTI -- an atomic database for emission lines -- Paper XVIII. Version 11, advanced ionization equilibrium models: density and charge transfer effects
RP Dufresne, GD Zanna, PR Young, KP Dere, E Deliporanidou, WT Barnes, E Landi
(2024)
Spectral Imager of the Solar Atmosphere: The First Extreme-Ultraviolet Solar Integral Field Spectrograph Using Slicers
A Calcines Rosario, F Auchère, AJ Corso, G Del Zanna, J Dudík, S Gissot, LA Hayes, GS Kerr, C Kintziger, SA Matthews, S Musset, D Orozco Suárez, V Polito, HAS Reid, DF Ryan
– Aerospace
(2024)
11,
208
Chorus wave power at the strong diffusion limit overcomes electron losses due to strong diffusion.
TA Daggitt, RB Horne, SA Glauert, G Del Zanna, JM Albert
– Nature communications
(2024)
15,
1800
Relativistic Phase Space Diffusion of Compact Object Binaries in Stellar Clusters and Hierarchical Triples
C Hamilton, RR Rafikov
– The Astrophysical Journal
(2024)
961,
237
The Solar Particle Acceleration Radiation and Kinetics (SPARK) Mission Concept
HAS Reid, S Musset, DF Ryan, V Andretta, F Auchère, D Baker, F Benvenuto, P Browning, É Buchlin, A Calcines Rosario, SD Christe, AJ Corso, J Dahlin, S Dalla, G Del Zanna, C Denker, J Dudík, R Erdélyi, I Ermolli, L Fletcher, A Fludra, LM Green, M Gordovskyy, SL Guglielmino, I Hannah, R Harrison, LA Hayes, AR Inglis, NLS Jeffrey, J Kašparová, GS Kerr, C Kintziger, EP Kontar, S Krucker, T Laitinen, P Laurent, O Limousin, DM Long, SA Maloney, P Massa, AM Massone, S Matthews, T Mrozek, VM Nakariakov, S Parenti, M Piana, V Polito, M Pesce-Rollins, P Romano, AP Rouillard, C Sasso, AY Shih, M Stęślicki, D Orozco Suárez, L Teriaca, M Verma, AM Veronig, N Vilmer, C Vocks, A Warmuth
– Aerospace
(2023)
10,
1034

DAMTP Astrophysics Seminars

29
Apr
14:00 - 15:00: Title to be confirmed

07
May
14:00 - 15:00: Title to be confirmed

13
May
14:00 - 15:00: Title to be confirmed

20
May
14:00 - 15:00: Title to be confirmed

28
May
14:00 - 15:00: Title to be confirmed