Possible effects of signal reception from different electrojet heights
in a skewness of auroral coherent spectra are studied assuming that t
he ''inherent'' spectral line due to plasma turbulence is of type-2 an
d symmetrical. For reasonable ionospheric parameters, the altitude int
egrated spectra are expected to be skewed negatively for positive mean
Doppler shift, in agreement with radar observations at small aspect a
ngles. However, the spectra could be skewed positively if the turbulen
t layer or the electron density profile is shifted to high altitudes o
f similar to 120 km. This change of spectral shape will not be observe
d experimentally if, at the same time, either the electron collision f
requency is enhanced or the ''inherent'' spectral width is increased.
Observational results are discussed in view of the predictions given.