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91探花
A spacecraft landing on Mars

Dr Ben Fernando

Postdoctoral Fellow - Christ Church College

Research theme

  • Exoplanets and planetary physics

Sub department

  • Atmospheric, Oceanic and Planetary Physics

Research groups

  • Solar system
benjamin.fernando@physics.ox.ac.uk
Atmospheric Physics Clarendon Laboratory, room 209h
  • About
  • Research
  • Teaching
  • Publications

COVID-19 highlights why UK-EU collaboration is so vital

Nature

Authors:

Benjamin Fernando, Gordon Brown, Emily Thomas, Michael Head, Martin Rees, Paul Nurse

Abstract:

Oceanic high-frequency global seismic wave propagation with realistic bathymetry

Geophysical Journal International

Authors:

Benjamin Fernando, Kuangdai Leng, Tarje Nissen-Meyer

Abstract:

Oceanic high-frequency global seismic wave propagation with realistic bathymetry

Geophysical Journal International 91探花 University Press 222:2 (2020) 1178-1194

Authors:

Benjamin Fernando, Kuangdai Leng, Tarje Nissen-Meyer

Abstract:

We present a new approach to simulate high-frequency seismic wave propagation in and under the oceans. Based upon AxiSEM3D (Leng et al. 2019), this method 91探花s a fluid ocean layer, with associated water-depth phases and seafloor topography (bathymetry). The computational efficiency and flexibility of this formulation means that high-frequency calculations may be carried out with relatively light computational loads. A validation of the fluid ocean implementation is shown, as is an evaluation of the oft-used ocean loading formulation, which we find breaks down at longer periods than was previously believed. An initial consideration of the effects of seafloor bathymetry on seismic wave propagation is also given, wherein we find that the surface waveforms are significantly modified in both amplitude and duration. When compared to observed data from isolated island stations in the Pacific, synthetics which include a global ocean and seafloor topography appear to more closely match the observed waveform features than synthetics generated from a model with topography on the solid surface alone. We envisage that such a method will be of use in understanding the new and exciting ocean-bottom and floating seismometer datasets now being regularly collected.

Training martian seismologists for InSight

Astronomy and Geophysics 59:5 (2018) 5.17-5.21

Authors:

B Fernando, M Tsekhmistrenko, K Hosseini

Training martian seismologists for InSight

ASTRONOMY & GEOPHYSICS 59:5 (2018) 17-21

Authors:

Benjamin Fernando, Kasra Hosseini, Maria Tsekhmistrenko

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