The current status of the Birmingham solar seismology network

Details The current status of the Birmingham solar seismology network The current status of the Birmingham solar seismology network

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..157a&link_type=abstract

In ESA, Seismology of the Sun and Sun-Like Stars p 157-160 (SEE N89-25819 19-92)

Computer Science

Performance

8

Helioseismology, P Waves, Solar Activity Effects, Solar Observatories, Data Acquisition, Ground Stations, Signal To Noise Ratios, Solar Spectra, Space Observations (From Earth)

Scientific paper

Aspects of the performance of a network of solar seismology stations are presented. Duty cycles for 1986 and 1987 are given and examples of window functions and p-mode spectra are shown. Sideband powers down to 2 percent of peak power are achieved for spans of 16 days and 3 percent for 64 days. Noise levels of 7 and 13 (m/sec)sq/Hz are achieved in regions just above and below the p-mode spectrum. A station in Birmingham (UK) is discussed. Its importance as a testing and training station is outlined and plans to deploy replicas around the globe are described.

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