View source for 09/11/2014 23:00:00 UTC

=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: <br />
[[File:plot_sw_mag_plasma_2014091100.png|350px]]
[[File:plot_sw_mag_2014091100.png|400px]]
[[File:plot_sw_vel_2014091100.png|350px]] <br />
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.