Abstract
Wavenummer spectra of spatial velocity fluctuations measured in selected high resolution solar photospheric spectrograms are presented. The statistical stability of the power estimates of particular ‘peaks’ in these spectra is discussed.
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Mitteilungen aus dem Fraunhofer Institut Nr. 126.
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Deubner, FL. On the energy distribution in wavenumber spectra of the granular velocity field. Sol Phys 36, 299–301 (1974). https://doi.org/10.1007/BF00151198
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DOI: https://doi.org/10.1007/BF00151198