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- W1995593212 abstract "If one assumes that solar p- and f-mode oscillations are stochastically excited, then the measured mode properties and solar background noise can be used to calculate maximum-likelihood uncertainties in mode frequency measurements, σ ν , for a given observation time. Such calculations agree quite well with our current data, if I use the measured background noise, which includes instrumental as well as solar contributions" @default.
- W1995593212 created "2016-06-24" @default.
- W1995593212 creator A5066563806 @default.
- W1995593212 date "1992-03-01" @default.
- W1995593212 modified "2023-09-26" @default.
- W1995593212 title "On the ultimate accuracy of solar oscillation frequency measurements" @default.
- W1995593212 doi "https://doi.org/10.1086/171119" @default.
- W1995593212 hasPublicationYear "1992" @default.
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