A new radio spectrograph, dedicated to observe the Sun, has been recently commissioned by the Indian Institute of Astrophysics (IIA) at the Gauribidanur Radio Observatory, about 100 km North of Bangalore. The instrument, called the Gauribidanur Lowfrequency Solar Spectrograph (GLOSS), operates in the frequency range ≈ 40 -440 MHz. Radio emission in this frequency range originates close to the Sun, typically in the radial distance range r ≈ 1.1 -2.0 R . This article describes the characteristics of the GLOSS and the first results. (UK). SOHO is a project of international cooperation between ESA and NASA. The SOHO-LASCO CME catalog is generated and maintained at the CDAW Data Center by NASA and the Catholic University of America in cooperation with the Naval Research Laboratory. The SDO/AIA data are courtesy of the NASA/SDO and the AIA science teams. We are grateful to the referee for his/her comments, which helped us to bring out the results more clearly.