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:
Plot sw mag plasma 2014091100.png Plot sw mag 2014091100.png Plot sw vel 2014091100.png
The blue lines are an approximation of the CME cloud and the red line denotes the shock.

Video Data

References

  • 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
  • Zhao, J., Gilchrist, S.A., Aulanier, G., Schmieder, B., Pariat, E. and Li, H., Hooked flare ribbons and flux-rope related QSL footprints, ApJ, 823 62, DOI http://dx.doi.org/10.3847/0004-637X/823/1/62 (2016).
  • Dudik, J., Polito, V., Janvier, M., Mulay, S.M., Karlicky, M., Aulanier, G., Del Zanna, G., Dzifcakova, E., Mason, H.E. and Schmieder, B., Slipping Magnetic Reconnection, Chromospheric Evaporation, Implosion, and Precursors in the 2014 September 10 X1.6-Class Solar Flare, ApJ, 823 41, DOI http://dx.doi.org/10.3847/0004-637X/823/1/41 (2016).
  • Webb, D., N. Nitta, Study on Understanding Problem Forecasts of ISEST Campaign Flare-CME Events, Solar Phys., submitted.
  • Marubashi, K., K.-S. Cho, H. Ishibashi: 2017, Interplanetary Magnetic Flux Rope as Agent Connecting Solar Eruptions and Geomagnetic Activities, Solar Phys., submitted.