We report ground based, low frequency heliograph (80 MHz), spectral MHz) and polarimeter (80 and 40 MHz) observations of drifting, non-thermal radio continuum associated with the 'halo' coronal mass ejection (CME) that occurred in the solar atmosphere on 2013 March 15. The magnetic field strengths (B) near the radio source were estimated to be B ≈ 2.2 ± 0.4 G at 80 MHz and B ≈ 1.4±0.2 G at 40 MHz. The corresponding radial distances (r) are r ≈ 1.9 R ⊙ (80 MHz) and r ≈ 2.2 R ⊙ (40 MHz). Subject headings: Sun -activity: Sun -flares: Sun -corona: Sun -radio radiation: Sun: coronal mass ejections (CMEs): Sun -magnetic topologythe referee for his/her comments that helped to bring out the results more clearly. The SOHO data are produced by a consortium of the Naval Research Laboratory (USA),

No abstract

No abstract

No abstract

No abstract