Observations associated with CME-3. (a) EUV images at 193 Å of source active region observed from SDO. (b) EUV images at 02:56 UT on 02 Nov. 2021 showing the flux rope direction and eruption from active region 12891. (c) and (d) Running difference images from LASCO/SOHO C2 corona graph highlighting the propagation of CME in heliosphere in 2D using segmentation technique and CACtus software (source and description of (c) are as mentioned in Fig. 1). Contemporaneous observations of CME-3 from STEREO-A COR2 and LASCO C2 and the GCS fit (blue) over plotted for each viewpoint.