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The Coronal Mass Ejection of 29 Sep 2013
and Geomagnetic Storm of 2 Oct 2013
Peter T. Gallagher
School of Physics
Trinity College Dublin
Event Summary
• SDO observed a filament lift-off in the northwest quadrant of the Sun
(~W40) starting at ~2013-09-29T21:00Z.
• An asymmetric halo CME was observed in SOHO/LASCO images from22:24
UT. Apex velocity of ~897 km/s (LASCO) and 1097 km/s (STEREO B).
• ACE arrival time (L1): 2013-10-02T01:20Z
• GOES arrival time (1AU): 2013-10-02T02:00Z
• Geomagnetic storm start (Ireland): 2013-10-02T01:58Z
• Earth arrival times (models):
– NASA/GSFC SWRC Ensemble: 2013-10-02T04:1Z (+8/-12 hours)
– STOA:
2013-10-02T06:15Z (+/-10 hours)
STEREO-A

STEREO-B
CME arrival at ACE/L1
(~20131002T01:20Z?)
Pre-CME solar
wind speed
(~375 km/s)
CME arrival at Earth
(~20131002T02:00Z?)
CME arrival at Earth
(~20131002T02:00Z?)
Rough IDL Arrival Time Calculation
t_sdo = '2013-09-29T21:00Z’
au = 149e6
v_cme = 1096.
v_sw = 375.
v_ave = ( v_cme + v_sw ) / 2.
dt = au / v_ave

;
;
;
;
;

km
km/s
km/s
km/s
s

t_au = anytim( anytim( t_sdo ) + dt, /vms )
print, t_au
2-Oct-2013 05:14:05.656
This is ~4 hours later than observed arrival.
Conclusions
• STEREO –B CME velocity of 1097 km/s is less
than actual CME velocity as CME was directed
away from STEREO-B.
• STEREO-A CME velocities therefore likely to be
> STEREO-B velocities.
• From radial propagation model, need STEREOA CME velocity of 1200 km/s to get correct
arrival time at Earth (2-Oct-2013 ~01:00 UT).

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Oct2013 Storm

  • 1. The Coronal Mass Ejection of 29 Sep 2013 and Geomagnetic Storm of 2 Oct 2013 Peter T. Gallagher School of Physics Trinity College Dublin
  • 2. Event Summary • SDO observed a filament lift-off in the northwest quadrant of the Sun (~W40) starting at ~2013-09-29T21:00Z. • An asymmetric halo CME was observed in SOHO/LASCO images from22:24 UT. Apex velocity of ~897 km/s (LASCO) and 1097 km/s (STEREO B). • ACE arrival time (L1): 2013-10-02T01:20Z • GOES arrival time (1AU): 2013-10-02T02:00Z • Geomagnetic storm start (Ireland): 2013-10-02T01:58Z • Earth arrival times (models): – NASA/GSFC SWRC Ensemble: 2013-10-02T04:1Z (+8/-12 hours) – STOA: 2013-10-02T06:15Z (+/-10 hours)
  • 3.
  • 5. CME arrival at ACE/L1 (~20131002T01:20Z?) Pre-CME solar wind speed (~375 km/s)
  • 6. CME arrival at Earth (~20131002T02:00Z?)
  • 7. CME arrival at Earth (~20131002T02:00Z?)
  • 8. Rough IDL Arrival Time Calculation t_sdo = '2013-09-29T21:00Z’ au = 149e6 v_cme = 1096. v_sw = 375. v_ave = ( v_cme + v_sw ) / 2. dt = au / v_ave ; ; ; ; ; km km/s km/s km/s s t_au = anytim( anytim( t_sdo ) + dt, /vms ) print, t_au 2-Oct-2013 05:14:05.656 This is ~4 hours later than observed arrival.
  • 9. Conclusions • STEREO –B CME velocity of 1097 km/s is less than actual CME velocity as CME was directed away from STEREO-B. • STEREO-A CME velocities therefore likely to be > STEREO-B velocities. • From radial propagation model, need STEREOA CME velocity of 1200 km/s to get correct arrival time at Earth (2-Oct-2013 ~01:00 UT).