  We report here our observations at 35 MHz and 327 MHz made in the direction
of the Gamma Ray pulsar Geminga. Based on the observed absence of any
significant pulsed emission from this source above our detection thresholds at
the two frequencies, we obtain useful upper-limits for the average flux to be
75-100 mJy at 35 MHz, and 0.2-0.3 mJy at 327 MHz. We discuss a few possible
reasons for the ``radio-quiet'' nature of this pulsar at frequencies other than
around 100 MHz.
