Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Birmingham, UK
Birmingham, U.K.
The University of Manchester, Schuster Laboratory, Manchester, UK
School of Physics and Space Research, The University of Birmingham
School of Physics and Astronomy, University of Birmingham
The School of Physics and Space Research, The University of Birmingham Birmingham B15 1TT, UK
U.Birmingham, UK
University of Birmingham
University of Birmingham, UK
School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT
Birmingham, University, England
School of physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK
School of Physics and Space Research, University of Birmingham, Edgbaston, Birmingham B15 2TT
School of Physics and Space Research, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK
School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK of Birmingham, Edgbaston, Birmingham, UK
Birmingham University
School of Physics and Astronomy, University of Birmingham, Edgbaston, B15 2TT Birmingham, UK
School of Physics and Astronomy, University of Birmingham, Birmingham, UK of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham, B15 2TT UK
School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK
School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmi
A comparison of frequentist and Bayesian inference: Searching for low-frequency p modes and g modes in Sun-as-a-star data
A comparison of the use of genetic and hill-climbing algorithms to fit low-l solar p-mode spectra
A devil in the detail: parameter cross-talk from the solar cycle and estimation of solar p-mode frequencies
A framework for describing correlated excitation of solar p modes
A fresh look at the seismic spectrum of HD49933: analysis of 180 days of CoRoT photometry
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Profile ID: LFWR-SCP-P-17188