Global oscillations of the solar brightness

Details Global oscillations of the solar brightness Global oscillations of the solar brightness

Mar 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...212l..95m&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 212, Mar. 1, 1977, p. L95-L99.

Astronomy and Astrophysics

Astrophysics

12

Solar Flux Density, Solar Radiation, Brightness, Cross Correlation, Power Spectra, Solar Atmosphere, Solar Spectra

Scientific paper

The Sacramento Peak Observatory vacuum tower telescope, echelle spectrograph, and diode array were used to search for global solar oscillations. The technique employed compares the relative intensity of a number of points on the solar disk and favors the detection of nonradial modes. In 6 days of observing, no narrow-band oscillations with periods between 15 and 90 minutes were found. The sensitivity per independent frequency interval is 0.0002 in contrast, or 0.3 K in temperature.

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