Cyclotron maser radiation, which according to a present knowledge is r
esponsible for some kinds of radiofrequency emission from the Sun, pla
nets and stars was considered. Using a three-wave representation, a se
t of equations for energy density of high-frequency modes were derived
with account for the main nonlinear effects. Along with known effects
, the equations obtained also describe those, not discussed in the lit
erature previously. Some quantitative estimates, showing the relative
role of different terms in the equations, were given for the case of t
he solar flares.