Solar atmospheric temperature inhomogeneities induce a 13-day oscillation in full-disk Doppler measurements

Details Solar atmospheric temperature inhomogeneities induce a 13-day oscillation in full-disk Doppler measurements Solar atmospheric temperature inhomogeneities induce a 13-day oscillation in full-disk Doppler measurements

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983natur.302..810e&link_type=abstract

Nature (ISSN 0028-0836), vol. 302, April 28, 1983, p. 810-812.

Computer Science

16

Doppler Effect, Solar Atmosphere, Solar Oscillations, Solar Temperature, Atmospheric Temperature, Cores, Line Spectra, Solar Rotation, Solar Spectra, Stellar Models

Scientific paper

Claverie et al. (1982) have reported a 13-day oscillation in full-disk solar spectrum-line shifts, which they claim to be evidence for rapid rotation of the sun's core. The authors point out that the passage of active regions across the disk could be responsible for oscillations of this kind. Variations in line shifts and in irradiance are expected with frequencies comparable to both the photospheric rotation rate and to higher harmonics.

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