Note on tracking Sun-Earth connection event ICME Event: 2013/11/11 Observer: Suman Dhakal on 2019/05 (part 1); 1. ICME 1.1. Catalog # Identified in ICME catalogs: Richardson & Can List RC catalog: Disturbance start time: 2013/11/11 17:00 UT Ejecta start time: 2013/11/11 17:00 UT Ejecta End time: 2013/11/12 03:00 UT dv = 0 km/s, v = 460 km/s, vmax= 480 km/s MC index: 1 Dst: -30 nT Suggested source CME: V_transit: km/s 1.2. SW Plots Overall ICME quality index: 2 (B is less than 10 nT) SW type: ejecta ICME signatures: varying Bz. Other ICME signatures: decreasing velocity, low proton temperature, and small plasma beta. Peculiar behavior: variation of Bz is not smooth, high density Search Window: Upper bound: Disturbance speed 460 km/s: 91 hrs: Lower bound: Transit speed < 700 km/s: 60 hrs < 2. CME 2.1. A. Candidate A A.1. LASCO: #CME 2013/11/07 15:12 UT, halo (from CDAW) moving with 411 km/s A.2. STEREO: moving in the frontside of the Sun. slight difficult to follow in COR2-A. A.3. AIA and GOES: corresponding to M2.4 flare , starting at 2013/11/07 14:15 from AR 11890, located around S13 E22 A.4. Comments: possible source of the disturbance. 2.1. B. Candidate B B.1. LASCO: #CME 2013/11/08 03:24 UT, halo (from CDAW) moving with 497 km/s C2 velocity: 203 km/s B.2. STEREO: direction is mostly southward COR2-A velocity (seeds): 381 km/s B.3. AIA and GOES: corresponding to X flare peaked at 02:40 UT from AR 1891 from S13 E13 B.4. Comments: could be the source of disturbance. 2.1. C. Candidate C C.1. LASCO: #CME 2013/11/08 05:36 UT, partial halo (from CDAW) moving with 682 km/s C.2. STEREO: seems like front side moving CME. C.3. AIA and GOES: source is not identifiable. C.4. Comments: unlikely the source, because of time and velocity. 3. Other Comments Possibility of multiple sources. 4. Summary SW index 2 Source index 3 Overall index 3.