  We study the spatial power spectra of Nikolaevskii turbulence in
one-dimensional space. First, we show that the energy distribution in
wavenumber space is extensive in nature. Then, we demonstrate that, when
varying a particular parameter, the spectrum becomes qualitatively
indistinguishable from that of Kuramoto-Sivashinsky turbulence. Next, we derive
the critical exponents of turbulent fluctuations. Finally, we argue that in
some previous studies, parameter values for which this type of turbulence does
not appear were mistakenly considered, and we resolve inconsistencies obtained
in previous studies.
