322 citations
- W. Chaplin2 profiles37 · h 81
- Y. Elsworth3 profiles35 · h 64
- R. New34 · h 36
- A. Broomhall19 · h 31
- S. Fletcher2 profiles17 · h 18
- D. Salabert16 · h 45
- T. Appourchaux2 profiles15 · h 54
- C. Régulo2 profiles13 · h 45
- G. Verner12 · h 37
- R. García2 profiles12 · h 62
- H. Kjeldsen2 profiles11 · h 77
- Bayode Ogunleye10 · h 12
- University of BirminghamGB41 papers
- Instituto de Astrofísica de CanariasES17 papers
- Aarhus UniversityDK16 papers
- Centre National de la Recherche ScientifiqueFR16 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR16 papers
- Universidad de La LagunaES16 papers
- Institut d'Astrophysique SpatialeFR15 papers
- Queen Mary University of LondonGB15 papers
- NSF NCAR High Altitude ObservatoryUS13 papers
- Astrophysique, Instrumentation et ModélisationFR12 papers
- NSF National Center for Atmospheric ResearchUS12 papers
- Centro de Astrofísica da Universidade do PortoPT11 papers
9 papers · 1 filter
The Octave (Birmingham - Sheffield Hallam) automated pipeline for extracting oscillation parameters of solar-like main-sequence stars
S. Hekker, A. -M Broomhall, W. J. Chaplin +6
The number of main-sequence stars for which we can observe solar-like oscillations is expected to increase considerably with the short-cadence high-precision photometric observatio…
Is the current lack of solar activity only skin deep?
A. -M. Broomhall, W. J. Chaplin, Y. Elsworth +2
The Sun is a variable star whose magnetic activity and total irradiance vary on a timescale of approximately 11 years. The current activity minimum has attracted considerable inter…
Corrections of Sun-as-a-star p-mode frequencies for effects of the solar cycle
A. -M. Broomhall, W. J. Chaplin, Y. Elsworth +2
Solar p-mode frequencies vary with solar activity. It is important to take this into account when comparing the frequencies observed from epochs that span different regions of the…
Radius determination of solar-type stars using asteroseismology: What to expect from the Kepler mission
D. Stello, W. J. Chaplin, H. Bruntt +22
For distant stars, as observed by the NASA Kepler satellite, parallax information is currently of fairly low quality and is not complete. This limits the precision with which the a…
Mode lifetimes of stellar oscillations - Implications for asteroseismology
W. J. Chaplin, G. Houdek, C. Karoff +2
Successful inference from asteroseismology relies on at least two things: that the oscillations in the stars have amplitudes large enough to be clearly observable; and that the osc…
Fresh insights on the structure of the solar core
Sarbani Basu, William J. Chaplin, Yvonne Elsworth +2
We present new results on the structure of the solar core, obtained with new sets of frequencies of solar low-degree p modes obtained from the BiSON network. We find that different…