The measurement of long-period oscillations at Sacramento Peak Observatory and South Pole

Details The measurement of long-period oscillations at Sacramento Peak Observatory and South Pole The measurement of long-period oscillations at Sacramento Peak Observatory and South Pole

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...82...43s&link_type=abstract

(International Astronomical Union and Akademiia Nauk SSSR, Colloquium on Problems of Solar and Stellar Oscillations, 66th, Nauch

Physics

5

Solar Cycles, Solar Limb, Solar Oscillations, Space Observations (From Earth), Antarctic Regions, Atmospheric Effects, Brightness, Fourier Transformation, Solar Flux, Solar Observatories

Scientific paper

Encouraging results have been obtained for the verification of the existence and origin of oscillatory signals, in the course of a program devoted to the measurement of long period brightness oscillations at the solar limb over several years. The length of the observing sequences imposed by the day/night cycle has, however, presented a significant difficulty. In order to circumvent it, the South Pole is considered as a site for extended observations, and a telescope specifically designed for observation and data analyses there is under development. Pertinent South Pole site parameters are presented which suggest the possibility of observing cycles longer than 150 hours.

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