Global oscillation measurements at Kumbel station in frame of the IRIS programme

Details Global oscillation measurements at Kumbel station in frame of the IRIS programme Global oscillation measurements at Kumbel station in frame of the IRIS programme

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soph..133...51b&link_type=abstract

(IRIS /International Research on the Interior of the Sun/ Workshop, 2nd, Tashkent, Uzbek SSR, Sept. 1989, Proceedings. A91-37551

Physics

6

Helioseismology, Solar Instruments, Solar Observatories, Solar Oscillations, Power Spectra, Velocity Measurement

Scientific paper

The atmospheric conditions on Kumbel mountain (near Tashkent, USSR), which is the site of the second of the International Research on the Interior of the Sun (IRIS) network instruments installed in August 1988 for measuring global oscillations are described along with the operating conditions of the IRIS instrument and the preliminary results from the station's solar oscillation measurements. The power specta obtained exhibit a very low level of noise for all frequency above 1 mHz, with the frequency resolution of the order of 23 microHz.

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