Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...340..599d&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 340, May 1, 1989, p. 599-606.
Astronomy and Astrophysics
Astrophysics
20
Atmospheric Turbulence, Solar Atmosphere, Solar Corona, Solar Spectra, Carbon, Energy Dissipation, Power Spectra, Ultraviolet Spectra
Scientific paper
The power spectrum of the spatial velocity fluctuations of the solar transition zone are determined from high-resolution telescope and spectrograph solar spectra of C IV. It is found that virtually all of the power resides at higher wavenumbers and that the spectrum is flatter than predicted for the inertial range of a turbulent fluid. The results suggest that the small-scale fluctuations are maintained by a driving mechanism such as magnetic reconnection or wave motions produced in the photosphere.
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