Note on tracking Sun-Earth connection event ICME Event: 2013/04/13 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: 2013/04/13 22:54 UT Ejecta start time: 2013/04/14 17:00 UT Ejecta End time: 2013/04/15 23:00 UT dv = 100 km/s, v = 410 km/s, vmax= 520 km/s MC index: 2 Dst: -6 nT Suggested source CME: 2013/04/11 07:24 H V_transit: 660 km/s 1.2. SW Plots Overall ICME quality index: 1 SW type: MC+SH ICME signatures: Bmax: 13.1 nT Smoothly changing Bz. Other ICME signatures: decreasing velocity, low density, low proton temperature, and low plasma beta Peculiar behavior: Search Window: Upper bound: Disturbance speed 410 km/s: 102 hrs: Lower bound: Transit speed < 700 km/s: 60 hrs < 2. CME 2.1. A. Candidate A A.1. LASCO: #CME 2013/04/09 at 12:24 UT, partial halo (from CDAW) A.2. STEREO: CME was moving in the same direction in COR2-A and COR2-B,therefore wasn't moving in the front side. A.3. AIA and GOES: A.4. Comment: not the source of the disturbance. 2.2. B. Candidate B B.1. LASCO: #CME 2013/04/11 at 07:24 UT, halo (from CDAW) Major CME moving with 861 km/s velocity. B.2. STEREO: partial halo in COR2-B and halo in COR2-A, front side moving CME. B.3. AIA and GOES: correspondig flare of M6.5 class from the AR 1719 at N07E13 B.4. Comment: Likely the source of the disturbance. 2.1. C. Candidate C C.1. LASCO: #CME 2013/04/12 at 02:00 UT, partial halo (from CDAW) Major CME moving with 391 km/s C.2. STEREO: CME was moving in the same direction in COR2-A and COR2-B,therefore wasn't moving in the front side. C.3. AIA and GOES: C.4. Comment: not the source of the disturbance, because of direction and velocity. 3. Other Comments Starting and ending time of disturbance and ejecta are different from GMU catalog. 4. Summary SW index 1 Source index 1 Overall index 1.