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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 stormcontinuum 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 thenon-thermal, plasma emission mechanism. The beam-density of suprathermalelectrons is estimated for the coronal plasma near the source region of stormradiation. Supplementary evidence for the density-estimate is provided by wayof analysing the imaging data from the SXT on-board the Yohkoh spacecraft, andthe LASCO, MDI, and EIT on board the SoHO spacecraft.Comment: 43 pages; 5 tables; 15 figures (9 color). ApJ (Part I : accepted

Spectrum of Solar Type I Continuum Noise Storm in the 50–80 MHz Band and Plasma Characteristics in the Associated Source Region