We have analysed the Rhodes/HartRAO survey at 2326 MHz and derived the glob
al angular power spectrum of Galactic continuum emission. In order to measu
re the angular power spectrum of the diffuse component, point sources were
removed from the map by median filtering. A least-square fit to the angular
power spectrum of the entire survey with a power law spectrum C-l proporti
onal to l(-alpha), gives alpha = 2.43 +/- 0.01 in the l range 2 -100. The a
ngular power spectrum of radio emission appears to steepen at high Galactic
latitudes and for observed regions with \b\ > 20 degrees, the fitted spect
ral index is alpha = 2.92 +/- 0.07. We have extrapolated this result to 30
GHz (the lowest frequency channel of Planck) and estimate that no significa
nt contribution to the sky temperature fluctuation is likely to come from s
ynchrotron at degree-angular scales.