Intense auroral kilometric radiation (AKR) is being frequently observe
d with POLRAD from the Auroral Probe (Interball-2). Observations of th
e abrupt upper frequency cutoffs (UFCs) in the spectra of AKR are repo
rted. The UFCs can be observed at a frequency range from 300 to 700 kH
z, corresponding to AKR generation altitudes from approximately 4800 t
o 2100 km, and are distributed in magnetic local time (MLT) hours simi
larly to the AKR events, with a maximum at 1 h MLT. The observed frequ
ency extent of the UFCs is less than or equal to 12 kHz, and is often
determined by the instrumental resolution (4 kHz). It is suggested tha
t the UFC may be associated with an abrupt switching on of the generat
ion mechanism, when the electron density becomes sufficiently low insi
de a plasma depletion at an altitude where the ratio off,,lf,, crosses
some threshold value. The steepness of the UFCs can imply a non-linea
r process of generation. The estimated distance of the e-folding field
aligned wave amplification is between 3 and 8 km. The UFCs are someti
mes, though very seldom (<10%), accompanied by narrow band (less than
4 kHz) ''ridges'' of radiation observed at the cutoff frequency. They
are smoothly drifting in frequncy for several minutes. The power densi
ty of radiation in the ''ridge'' can be up to 2 orders of magnitude st
ronger than in the accompanying wide band emission of AKR. The ''ridge
'' at UFC can imply either energy concentration at the source bottom,
or focusing, if specific conditions for the escape of the radiation ar
e assumed.