We report here on high angular resolution observations of solar noise storm sources at a frequency of 75MHz. The data for the study were obtained at the Gauribidanur Radio Observatory (long.: 77 deg26'12''E, lat.: 13 deg36'12''N) about 100km north of Bangalore, India, during the solar eclipse of 24October 1995. Our main conclusion is that there are structures of angular size <=2.5arcmin in the outer solar corona.
