Note on tracking Sun-Earth connection event

ICME Event: 2013/08/20

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: 2013/08/20 22:27 UT
	Ejecta      start time:	2013/08/21 08:00 UT
	Ejecta      End   time:	2013/08/21 14:00 UT
	dv =  30 km/s, v =  460 km/s, vmax=  470 km/s
      	MC index: 1    
	Dst:       -26  nT
     	Suggested source CME: 
     	V_transit:    km/s
      
  1.2. SW Plots
	Overall ICME quality index: 3
	SW type: EJ+SH
	ICME signatures:  Bmax: 6.1 nT
				varying Bz.
	Other ICME signatures:  low proton temperature, and low plasma beta.
                     
	Peculiar behavior: Variation in velocity is hard to discern 
			   Plasma density plot is not available
			   Fluctuating plasma beta. 
                         
	Search Window:
	Upper bound: Disturbance speed 430 km/s: 91 hrs:
	Lower bound: Transit speed < 700 km/s: 60 hrs <

2. CME
   2.1. A. Candidate A
 	A.1. LASCO:
		#CME 2013/08/16 at 11:48 UT, halo (from CDAW)
		moving with a velocity of 478 km/s
	A.2. STEREO:
		not moving in the front side.
	A.3. AIA and GOES:
			
	A.4. Comments:
		Unlikely the source because of direction.



   2.2. B. Candidate B
 	B.1. LASCO:
		#CME 2013/08/16 at 15:48 UT, halo (from CDAW)
		moving with a velocity of 555 km/s
	B.2. STEREO:
		not moving in the front side.
	B.3. AIA and GOES:
			
	B.4. Comments:
		Unlikely the source because of direction.


   2.3. C. Candidate C
 	C.1. LASCO:
		#CME 2013/08/17 at 19:12 UT, halo (from CDAW)
		moving with a velocity of 1202 km/s
	C.2. STEREO:
		halo CME in COR2-A and COR2-B.
	C.3. AIA and GOES:
		corresponding to M3.3 class flare peaked at 18:24 UT
		from AR 1818 at a location S04W30.	
	C.4. Comments:
		Unlikely the source because of velocity.

  2.4. D. Candidate D
	D.1 LASCO:
		#CME 2013/08/19 23:12, halo (from CDAW)
		moving with a velocity of 877 km/s.

	D.2 STEREO:
		not moving in the front side.

	D.3 AIA and GOES:

	D.4 Comment
		unlikely the source due to direction and time of the eruption.

3. Other Comments
		

4. Summary
  

 SW index 3
    Source index 3  
    Overall index 3.