The change in the signal absorptions by rare gas afterglow plasmas as a DC magnetic field is varied in the range 0-400 G is studied in the frequency range 200-1500 MHz. The measurements are made using large aluminium cavities excited in the TM0m0 family of modes with a uniform DC magnetic field, B, applied along the direction of the alternating electric field. Signal absorptions are observed to occur, B=0, at several successive times during the afterglow for signal frequency, fM, when the pulsed plasma is excited by means of an 8 ms pulse of high frequency energy at 54 MHz. The absorptions get smaller as the magnetic field is increased slowly in magnitude, and disappear, in turn, for certain critical values of field, Bcrit. Plots of fM against Bcrit fall on straight lines having almost integrally related slopes, the lowest slope having a value close to 2.80*106 HzG-1 in magnitude. The phenomena are believed to be explicable in terms of the oscillations of a low energy gas of electron pairs which break up at critical values of B. The plasma oscillations of a free electron gas are also briefly discussed.