Note on tracking Sun-Earth connection event

ICME Event: 2013/11/08

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: 2013/11/08 22:00 UT
	Ejecta      start time:	2013/11/08 22:00 UT
	Ejecta      End   time:	2013/11/09 07:00 UT
	dv =  0 km/s, v =  420 km/s, vmax=  460 km/s
      	MC index: 2    
	Dst:       -80  nT
     	Suggested source CME: 
     	V_transit:    km/s
      
  1.2. SW Plots
	Overall ICME quality index: 3
	SW type: EJ
	ICME signatures:  smoothly varying Bz.
	Other ICME signatures:  small plasma beta, low proton temperature for some part.
                     
	Peculiar behavior: increasing velocity, high plasma density, high proton temperature for some part of the ICME.
                         
	Search Window:
	Upper bound: Disturbance speed 420 km/s: 99 hrs:
	Lower bound: Transit speed < 700 km/s: 60 hrs <

2. CME
   2.1. A. Candidate A
	A.1. LASCO:
		#CME 2013/11/02 21:25 UT, angular width of 105 (from CDAW)
		moving with a linear velocity of 377 km/s in CDAW
		velocity in seeds C2: 234 km/s
	A.2. STEREO:
		moving in the front side. Partial halo in COR2-A, velocity: 272 km/s
	A.3. AIA and GOES
		from AR 11884 located around S12 W12
	A.4. Comments:
		likely the source of disturbance. 



   2.1. B. Candidate B
	B.1. LASCO:
		#CME 2013/11/05 02:48 UT, partial halo (from CDAW)
		moving with 512 km/s in northward direction.
	B.2. STEREO:
		moving in northward direction.
	B.3. AIA and GOES
		eruption from the northern hemisphere, near the eastern limb.
	B.4. Comments:
		unlikely the source of disturbance due to the direction of the CME.


  2.1. C. Candidate C
	C.1. LASCO:
		#CME 2013/11/05 08:24 UT, partial halo (from CDAW)
		moving with a velocity of 850 km/s
	C.2. STEREO:
		moving northward.
	C.3. AIA and GOES:
		corresponding to M2.5 flare peaked at 08:19 UT
		from AR 1890 at S16E51
	C.4. Comments:
		Unlikely the source, because of the direction and velocity.

  2.1. D. Candidate D
	D.1. LASCO:
		#CME 2013/11/06 14:24 UT, partial halo (from CDAW)
		moving with 347 km/s
	D.2. STEREO:
		hardly visible in COR2-A and COR2-B.
	D.3. AIA and GOES:
	D.4. Comments:
		unlikely the source due to the velocity. 


  2.1. E. Candidate E
	E.1. LASCO:
		#CME 2013/11/07 00:00 UT, halo (from CDAW)
		moving with 1033 km/s
	E.2. STEREO:
		not moving in the front side.
	E.3. AIA and GOES:
	E.4. Comments:
		unlikely the source due to the velocity. source region was behind (stereo-B, 195)


  2.1. F. Candidate F
	F.1. LASCO:
		#CME 2013/11/07 10:36 UT, halo (from CDAW)
		moving with 1405 km/s
	F.2. STEREO:
		partial halo in COR2-A and halo in COR2-B. 
	F.3. AIA and GOES:
	 	source is probably on the back side
	F.4. Comments:
		unlikely the source due to the velocity. source region was behind (stereo-B, 195)

  2.1. G. Candidate G
	G.1. LASCO:
		#CME 2013/11/07 15:12 UT, halo (from CDAW)
		moving with 411 km/s
	G.2. STEREO:
		probably moving in the front side, not discernable in COR2-A
	G.3. AIA and GOES:
		front side source in SE quardant.
	G.4. Comments:
		unlikely the source due to the velocity. 



 

3. Other Comments

source is unidentified
4. Summary
  
  SW index 3
    Source index 1  
    Overall index 3.