Confirmation of solar cycle-dependent intermediate-degree p-mode frequency shifts

Details Confirmation of solar cycle-dependent intermediate-degree p-mode frequency shifts Confirmation of solar cycle-dependent intermediate-degree p-mode frequency shifts

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...406..714r&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 406, no. 2, p. 714-722.

Astronomy and Astrophysics

Astrophysics

18

Frequency Shift, Solar Cycles, Solar Magnetic Field, Solar Oscillations, Correlation Coefficients, Solar Maximum Mission, Sunspots

Scientific paper

Results of intercomparisons of seven different sets of frequencies of intermediate-degree p-modes obtained at several different locations between 1981 and 1989 are presented. It is shown that the frequency shifts exhibited by all of these intermediate-degree p-modes are consistent with the intermediate-degree frequency shifts presented by Libbrecht and Woodward (1990) and also with the low-degree frequency shifts presented by Elsworth et al. (1990). It is also shown that these frequency shifts correlate with solar cycle-dependent changes in sunspot number, area, and irradiance. Unbinned and binned differences between 1984 Mount Wilson Observatory and revised 1981 South Pole frequencies are illustrated.

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