  The spectra of the coronal hole radio emission in solar cycles 23 and 24 have
been studied based on RATAN-600 data in the 4-16.5 GHz range at frequencies of
5.7 and 17 GHz and 327 MHz. It has been found that bright features of coronal
hole microwave emission at 17 GHz and dark features at 5.7 GHz can exist in
coronal holes when the spectral index is 1.25-1.5 in the 6.5-16.5 GHz range;
the radio spectrum in this range is flat when coronal holes are indiscernible
against the background of a quiet Sun. The possible vertical scale of the solar
atmosphere over coronal holes is discussed.
