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You can also view live system telemetry and images from the on-site cameras at Bi SON Live!
Patches of the surface of the sun oscillate up and down with a typical period of about 5 minutes.
It contains as well an file with: - column 1: the series index associated to the frequency table; - column 2, 3, 4: respectively the year, month, and day of the starting date of each 365-day time series; - column 5: the associated duty cycle in %; - column 6: the corresponding radio flux averaged over the same 365-day periods. (2015) and were updated as longer time series were available.
They were calculated for 4 different frequency ranges: [1800-3790μHz]; the low-frequency range [1800-2450μHz]; the mid-frequency range [2450-3110μHz]; and the high-frequency range [3110-3790μHz].
The group in Birmingham has been studying the Sun since the 1960's and has built up decades of expertise.
Those simulations, and the seismological evidence with which they are being confronted, are reviewed elsewhere in this volume.
Our understanding of the global dynamics of the radiative interior of the Sun is in a much more primitive state.
The temporal cadence of the time series is of 60 seconds and the starting date on April 11, 1996. (2015) and were updated as longer time series were available.
They were extracted from one-year (365 days) GOLF time series, with a four-time overlap (91.25 days).
The GOLF velocity time series were obtained following Garcia et al. Download the GOLF data from April 11, 1996 to October 31, 2015 below. Also use the following in your acknowledgements in publication: "The GOLF instrument onboard So HO is a cooperative effort of scientists, engineers, and technicians, to whom we are indebted.