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habitat and connectivity as streams dry out is particularly important (Dugdale et al. 2022) for process hydrology, river ecology (e.g. refugia during drought, loss of physical in-channel habitat, loss
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Terahertz (THz) is a rapidly expanding field with notable importance for a myriad of disciplines such as physics, chemistry and biology. In the context of material science, optical-pump terahertz
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concern is the presence of marine organisms that settle and grow on submerged structures – a process known as biofouling. Biofouling will increase drag and mass loading on dSPCs but will vary with many
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of Physics & Astronomy Scholarship, providing the award of full academic fees, together with a tax-free maintenance grant at the standard UKRI rate (currently £20,780 in academic session 2025/26) per
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engineering or physics (preferably with first class honours or equivalent) and we expect the PhD candidate to develop the expertise required to lead an experimental research project, to train students
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easier to detect and measured experimentally. However, it is not well known yet how this process emerges and how one can control it. This PhD project will focus on developing the necessary theoretical
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-physics-and-astronomy/astronomy-and-experimental-gravity/sun-stars-and-exoplanets . Our group has 5 permanent academics, 12 postdoctoral researchers, and 10 PhD students and is gender-balanced. In 2024, a
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the Sun, Stars & Exoplanets research group in Birmingham can be found at https://www.birmingham.ac.uk/research/centres-institutes/research-in-physics-and-astronomy/astronomy-and-experimental-gravity/sun
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found at https://www.birmingham.ac.uk/research/centres-institutes/research-in-physics-and-astronomy/astronomy-and-experimental-gravity/sun-stars-and-exoplanets . Our group has 5 permanent academics, 12
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://www.birmingham.ac.uk/research/centres-institutes/research-in-physics-and-astronomy/astronomy-and-experimental-gravity/sun-stars-and-exoplanets . Our group has 5 permanent academics, 12 postdoctoral researchers, and 10