EVE Sun-as-a-star Doppler spectra of 26 EUV lines reveal Harvey-like convective continua to 50 mHz, reduced granulation power in coronal lines, ~15 km/s nonthermal RMS, and no Kolmogorov turbulence.
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Signatures of photospheric convection throughout the solar atmosphere: the EVE Sun-as-a-star mHz continuum
EVE Sun-as-a-star Doppler spectra of 26 EUV lines reveal Harvey-like convective continua to 50 mHz, reduced granulation power in coronal lines, ~15 km/s nonthermal RMS, and no Kolmogorov turbulence.