01/08/2014-01/09/2014 - Revision history

Davidwebb: /* References */

2017-01-20T22:18:47Z

‎References

2017-01-20T22:18:08Z

‎References

2015-09-09T19:56:50Z

‎References

2015-09-09T19:55:45Z

‎References

2014-09-24T14:32:02Z

‎Comment Section

2014-09-24T14:31:44Z

‎Comment Section

2014-08-29T18:14:33Z

‎Comment Section

2014-08-29T17:03:51Z

Created page with "=Comment Section= =Image Data= =Video Data= =References="

New page

=Comment Section=

=Image Data=

=Video Data=

=References=

@@ Line 15: / Line 15: @@
 - Moestl et al., Nat. Commun., 6, 7135, 2015.
-- Gopalswamy et al., E,P&S, 66, 104, 2014.
+- Gopalswamy et al., EP&S, 66, 104, 2014.
 - Wang, R., Liu, Y. D., Dai, X., Yang, Z., Huang, C., and Hu, H., The role of active region coronal magnetic field in determining coronal mass ejection propagation direction, 2015, Astrophys. J., 814, 80 (http://iopscience.iop.org/article/10.1088/0004-637X/814/1/80/pdf)
 - Mays, M.L., B. J. Thompson, L. K. Jian, R. C. Colaninno, D. Odstrcil, C. Möstl, M. Temmer, N. P. Savani, G. Collinson, A. Taktakishvili, P. J. MacNeice , and Y. Zheng, Propagation of the 2014 January 7 CME and Resulting Geomagnetic Non-Event, Astrophys. J, 812, 145, 2015

@@ Line 8: / Line 8: @@
 =References=
 - Webb, D., An Overview of the 7 January 2014 X-Class Flare-CME and Space Weather Predictions, AGU SH51E-01, 2014.
@@ Line 15: / Line 17: @@
 - Gopalswamy et al., E,P&S, 66, 104, 2014.
+- Wang, R., Liu, Y. D., Dai, X., Yang, Z., Huang, C., and Hu, H., The role of active region coronal magnetic field in determining coronal mass ejection propagation direction, 2015, Astrophys. J., 814, 80 (http://iopscience.iop.org/article/10.1088/0004-637X/814/1/80/pdf)

@@ Line 10: / Line 10: @@
 - Webb, D., An Overview of the 7 January 2014 X-Class Flare-CME and Space Weather Predictions, AGU SH51E-01, 2014.
 - Moestl et al., Nat. Commun., 6, 7135, 2015.
 - Gopalswamy et al., E,P&S, 66, 104, 2014.
+-

← Older revision		Revision as of 19:55, 9 September 2015
Line 8:		Line 8:

	=References=		=References=
		+
		+	- Webb, D., An Overview of the 7 January 2014 X-Class Flare-CME and Space Weather Predictions, AGU SH51E-01, 2014.
		+	- Moestl et al., Nat. Commun., 6, 7135, 2015.
		+	- Gopalswamy et al., E,P&S, 66, 104, 2014.
		+	-

@@ Line 1: / Line 1: @@
 =Comment Section=
 *This event has been included because it has a very strong Halo CME entering LASCO around 17:48 UT on the 7th, but presents no obvious in-situ signatures at L1. (Hess)
-This is thus a “problem” event and is being studied for an AGU session. N. Gopalswamy reports that the January 6 and 7 CMEs are quite intriguing. The Jan. 6 event produced a GLE even though it had a speed <2000 km/s and originated behind the west limb (Thakur et al., ApJ, 2014). The Jan. 7 CME was near disk center and ultrafast (~3000 km/s), but was likely deflected to the south and west so it was not geoefffective although it was a large SEP event.  It was also not a GLE.
+This is thus a “problem” event and is being studied for an AGU session. N. Gopalswamy reports that the January 6 and 7 CMEs are quite intriguing. The Jan. 6 event produced a GLE even though it had a speed <2000 km/s and originated behind the west limb (Thakur et al., ApJ, 2014). The Jan. 7 CME was near disk center and ultrafast (~3000 km/s), but was likely deflected to the south and west so it was not geoefffective although it was a large SEP event.  It was also not a GLE. (D. Webb)
 =Image Data=

← Older revision		Revision as of 18:14, 29 August 2014
Line 1:		Line 1:
	=Comment Section=		=Comment Section=
		+	*This event has been included because it has a very strong Halo CME entering LASCO around 17:48 UT on the 7th, but presents no obvious in-situ signatures at L1. (Hess)

	=Image Data=		=Image Data=