Frequencies, amplitudes and linewidths of solar oscillations from total irradiance observations

Details Frequencies, amplitudes and linewidths of solar oscillations from total irradiance observations Frequencies, amplitudes and linewidths of solar oscillations from total irradiance observations

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983natur.305..589w&link_type=abstract

Nature (ISSN 0028-0836), vol. 305, Oct. 13, 1983, p. 589-593.

Physics

87

Irradiance, Solar Oscillations, Solar Spectra, Amplitudes, Error Analysis, Frequencies, Power Spectra, Solar Maximum Mission, Spectral Line Width

Scientific paper

Ten months of solar total irradiance data from the Solar Maximum Mission satellite have generated accurate frequencies, amplitudes and linewidths for individual about 5-min solar p-mode oscillations of low degree. The modes can be described as independent and chaotically excited oscillators, and provide no evidence for the fine structure taken to imply rapid internal rotation of the sun.

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