New analysis of the solar p-mode frequency change from 1980 to 1986

Details New analysis of the solar p-mode frequency change from 1980 to 1986 New analysis of the solar p-mode frequency change from 1980 to 1986

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...200l..29g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 200, no. 1-2, July 1988, p. L29-L31.

Astronomy and Astrophysics

Astrophysics

9

Solar Diameter, Solar Oscillations, Cross Correlation, Frequency Ranges, Frequency Stability, Power Spectra

Scientific paper

Using a method of power spectra cross-correlation, the authors were able in 1986 to confirm a 0.39 μHz decrease of solar low degree p-mode frequencies between 1980 and the end of 1984. With the same method applied to their 1984/85 south pole data and to all Acrim data obtained until April 1986, they again confirm this decrease, and on the other hand, they find an extreme stability of these frequencies from spring 1984 to spring 1986, with an accuracy of 0.02 μHz.

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