09/11/2014 23:00:00 UTC

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Comment Section

  • Weak shock arrival on the 11th, with another stronger shock apparent around 15:00 UT on the 12th. These are followed by a strong magnetic field and velocity enhancement, that show indications of magnetic field rotation and expansion. Very strong magnetic field, but very little of it was pointed southward (Hess)

Image Data

A combination of SWEPAM and MAG data from the ACE Satellite:

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The blue lines are an approximation of the CME cloud and the red line denotes the shock.

Video Data

References

  • Marubashi, K., K.-S. Cho, H. Ishibashi: 2017, Interplanetary Magnetic Flux Rope as Agent Connecting Solar Eruptions and Geomagnetic Activities, Solar Phys., submitted.
  • McKenna-Lawlor, S., W. Ip, B. Jackson, D. Odstrcil, P. Nieminen, H. Evans, J. Burch, K. Mandt, R. Goldstein, I. Richter, M. Dryer: 2016, Space Weather at Comet 67P/Churyumov–Gerasimenko Before its Perihelion, Earth Moon & Planets, 117, 1–22, DOI 10.1007/s11038-015-9479-5
  • Webb, D., N. Nitta, Study on Understanding Problem Forecasts of ISEST Campaign Flare-CME Events, Solar Phys., submitted.
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