Continuous observation of solar oscillations from two suitably spaced ground stations

Details Continuous observation of solar oscillations from two suitably spaced ground stations Continuous observation of solar oscillations from two suitably spaced ground stations

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mmsai..55...63c&link_type=abstract

(European Physical Society, Ministero della Pubblica Istruzione, and Universita di Catania, EPS Study Conference on Oscillations

Other

10

Solar Oscillations, Space Observations (From Earth), Data Correlation, Ground Stations, Power Spectra

Scientific paper

By operating two observing stations, one at Izana on Tenerife and the other at Haleakala on Maui, up to 22 hours of continuous solar surface velocity data per day are obtained. Correlation of two station data provides confirmation of the solar origin of the signals and the improved window function and long time span of data collection yield clear power spectra of the 5 minute oscillations. Detailed analysis of a prominent l1 mode indicates that coherence exists over the 88 days of observation.

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