  Continuum observations of a solar noise storm in the frequency range of 50 -
80 MHz observed with the Gauribidanur radio spectrograph during 2000 September,
26 & 27, are presented here. The radio spectral index of the noise storm
continuum in the band 50 - 80 MHz is found to be ~3.65 during the above period.
The Noise Storm continuum radiation is explained as a consequence of the
non-thermal, plasma emission mechanism. The beam-density of suprathermal
electrons is estimated for the coronal plasma near the source region of storm
radiation. Supplementary evidence for the density-estimate is provided by way
of analysing the imaging data from the SXT on-board the Yohkoh spacecraft, and
the LASCO, MDI, and EIT on board the SoHO spacecraft.
