Jie Format:
Note on tracking Sun-Earth connection event

ICME Event: 2009/06/03

Observer: Taylor Cox on 2018/11/27

1. ICME
  1.1. Catalog
     # Identified in ICME catalogs: Richardson & Cain List
      RC catalog
      Disturbance start time: 2009/06/03 16:00 UT
      Ejecta      Start time: 2009/06/04 02:00 UT
      Ejecta      End   time: 2009/06/05 16:00 UT
      dv = 20 km/s, v = 310 km/s, vmax= 330 km/s
      MC index:     1
      Dst:        -21 nT
      Suggested source CME: N/A
      V_transit:  300

  1.2. Comments
      Overall ICME quality index: #
      ICME signatures: Bmax:  # nT
                       Bz rotation
      Others ICME signature: 
      Peculiar behavior: density and temperature data is lost within the ejecta

      Disturbance time 300 km/s  -> search window 138 hrs -> 2009/05/29 22:00 UT

2. CME
   2.1.A.  Candidate A
    A.1. LASCO:
      #CME 2009/05/30 17:00 UT, partial halo CDAW
	  CME off of the right limb seems to expand in a way to indicate a partial halo.
     A.2. STEREO:
	    on STEREO A, a clear SME leaves in the direction away from earth, while in STEREO B, a fainter signiture can also be seen in the Earthward direction. This likely indicates that this event was on the Earth-facing side of the sun, but is likely not Earthbound.

     A.3. AIA & GOES:
	    

     A.4. Comments:
             given the STEREO observations, this likely is not the source CME of the ICME.

   2.1.B. Candidate B.
	#CME 2009/05/31 00:00 UT, partial halo CDAW
	  CME off of the left limb seems to expand in a way to indicate a partial halo.
     B.2. STEREO:
	on STEREO A, a clear SME leaves in the direction towards earth, while in STEREO B, a fainter outflow can also be seen in the 		Earthward direction. The outflow is not a promising signature, but the direction is in agreement with STEREO A for an Earthbound CME. 

     B.3. AIA & GOES:
	    

     B.4. Comments:
             The stereo B observations agree in direction here and the CDAW observations show expansion that could become a partial halo. This is the most likely candidate observed.

   2.2 Decided Source
       The most likely solar source is Candidate B.

3. Other Comments



4. Summary
    SW index _
    Source index _
    Overall index _