Note on tracking Sun-Earth connection event ICME Event: 2013/01/17 Observer: Suman Dhakal on 2018/11 1. ICME 1.1. Catalog # Identified in ICME catalogs: Richardson & Can List RC catalog: Disturbance start time: 2013/01/17 16:00 UT Ejecta start time: 2013/01/17 16:00 UT Ejecta End time: 2013/01/18 12:00 UT dv = 0 km/s, v = 390 km/s, vmax= 400 km/s MC index: 2 Dst: -52 nT Suggested source CME: 2013/01/13 12:00 UT V_transit: 420 km/s 1.2. Comments Overall ICME quality index: 3 SW type: MC ICME signatures: Bmax: 15.6 nT Bz rotation Others ICME signature: low proton temperature, and low plasma density. Peculiar behavior: velocity was increasing in the middle and high plasma density, it was 16.2 cm^-3 in the center Based on 390 km/s -> search window 106.5 hrs or 4 1/2 days-> 2012/01/13 05:30 UT 2. CME 2.1. A. Candidate A A.1. LASCO: #CME 2013/01/13 12:00 UT, partial halo (from CDAW) angle- 176, velocity- 229 km/s Seeds vel C2: 167 km/s Distinctive LF and unidentifiable core A.2 .STEREO: Seen as a major CME in both COR2-A and COR2 B Front-side halo CME, consistent witht the flare source region A.3. AIA & GOES corresponding flare: M1.7 at 2013/01/13 08:35 UT flare from AR 11652 at N17W22 A.4 Comment: likey the source: the ejecta is in the nother-west quadrant the ejecta does cross the equator in STEREO FOV the ejecta cross the northern-pole in LASCO FOV Peculiar behavior: Eruption started at 08:35 UT on 2013/01/13 as seen from AIA. 2.1. B. Candidate B B.1. LASCO: #CME 2013/01/14 09:24, partial halo (from CDAW) moving with 264 km/s B.2. STEREO: CME was not moving in the front side. B.3. AIA and GOES: B.4. Comments: Due to direction of propagation, unlikely the source. 2.1. C. Candidate C C.1. LASCO: #CME 2013/01/15 08:12, poor event (from CDAW) slow CME with linear velocity of 221 km/s and angular width of 105. Leading front was not sharp. C.2. STEREO: Seen as front side moving CME in both COR2-A and COR2-B. C.3. AIA and GOES: Associated with M-class flare, peaked at 06:58 UT, from AR 11650 C.4. Comments: located at the SE quadrant, unlikely to be the source due to small velocity and direction. 2.1. D. Candidate D D.1. LASCO: #CME 2013/01/15 19:48, partial halo (from CDAW) moving with velocity of 798 km/s. D.2. STEREO: moving northward, unlikely the front side moving CME. D.3. AIA and GOES: D.4. Comments: Unlikely the source of disturbance. 2.1. E. Candidate E E.1. LASCO #CME 2013/01/16 19:00 UT, partial Halo (from CDAW) Fast CME with linear velocity 648 km/s. Sharp LE, crossed the equatorial line. E.2. STEREO Seen as major CME in COR2-A and COR2-B. E.3. AIA and GOES: AIA data is not available. E.4. Comments: less likely be the source of disturbance because of time of eruption. 3. Other Comments 4. Summary SW index 3 Source index 1 Overall index 3.