05/28/2010 21:00:00 UTC - Revision history

Phess4: /* In-Situ Data */

2013-07-02T20:47:12Z

‎In-Situ Data

2013-07-02T17:28:48Z

‎In-Situ Data

2013-07-01T16:29:50Z

‎Comment Section

2013-06-19T09:53:02Z

‎Comment Section

2013-06-19T09:47:25Z

2013-06-19T08:36:57Z

‎Video Data

2013-06-02T05:07:07Z

2013-03-19T15:15:32Z

‎Image Data

2013-03-08T13:58:11Z

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

New page

=Comment Section=

=Image Data=

=Video Data=

@@ Line 6: / Line 6: @@
 ==In-Situ Data==
 A combination of SWEPAM and MAG data from the ACE Satellite: <br />
-[[File:plot_sw_mag_plasma_2010052800.png|350px]]
+[[File:plot_sw_mag_plasma_2010052700.png|350px]]
-[[File:plot_sw_mag_2010052800.png|400px]]
+[[File:plot_sw_mag_2010052700.png|400px]]
-[[File:plot_sw_vel_2010052800.png|350px]] <br />
+[[File:plot_sw_vel_2010052700.png|350px]] <br />
 The blue lines are an approximation of the CME cloud and the red line denotes the shock.

@@ Line 6: / Line 6: @@
 ==In-Situ Data==
 A combination of SWEPAM and MAG data from the ACE Satellite: <br />
-[[File:plot_sw_mag_plasma_2010052700.png|350px]]
+[[File:plot_sw_mag_plasma_2010052800.png|350px]]
-[[File:plot_sw_mag_2010052700.png|400px]]
+[[File:plot_sw_mag_2010052800.png|400px]]
-[[File:plot_sw_vel_2010052700.png|350px]] <br />
+[[File:plot_sw_vel_2010052800.png|350px]] <br />
 The blue lines are an approximation of the CME cloud and the red line denotes the shock.

@@ Line 2: / Line 2: @@
 *A "well-behaved" CME-ICME event
 *Two consecutive halo CMEs originated from the Sun from almost the same region, one at ~ 18 UT, May 23, and the other at ~ 14 UT, May 24. The question is we should expect to find two consecutive ICMEs at 1 AU, as well as in SECCHI HI observations. Is this kind of double CMEs showing up?
 =Image Data=

@@ Line 1: / Line 1: @@
 =Comment Section=
 *A "well-behaved" CME-ICME event
 *Two consecutive halo CMEs originated from the Sun from almost the same region, one at ~ 18 UT, May 23, and the other at ~ 14 UT, May 24. The question is we should expect to find two consecutive ICMEs at 1 AU, as well as in SECCHI HI observations. Is this kind of double CMEs showing up?
 =Image Data=

← Older revision		Revision as of 09:47, 19 June 2013
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	=References=		=References=
		+	*Lugaz, N., Farrugia, C. J., Davies, J. A., Möstl, C., Davis, C. J., Roussev, I. I., & Temmer, M. (2012). The Deflection of the Two Interacting Coronal Mass Ejections of 2010 May 23-24 as Revealed by Combined in Situ Measurements and Heliospheric Imaging. Astrophysical Journal, 759(1), 68. doi:10.1088/0004-637X/759/1/68

← Older revision		Revision as of 05:07, 2 June 2013
Line 1:		Line 1:
	=Comment Section=		=Comment Section=
		+	*A "well-behaved" CME-ICME event
		+	*Two consecutive halo CMEs originated from the Sun from almost the same region, one at ~ 18 UT, May 23, and the other at ~ 14 UT, May 24. The question is we should expect to find two consecutive ICMEs at 1 AU, as well as in SECCHI HI observations. Is this kind of double CMEs showing up?

	=Image Data=		=Image Data=

← Older revision		Revision as of 15:15, 19 March 2013
Line 2:		Line 2:

	=Image Data=		=Image Data=
		+	==In-Situ Data==
		+	A combination of SWEPAM and MAG data from the ACE Satellite: <br />
		+	[[File:plot_sw_mag_plasma_2010052700.png\|350px]]
		+	[[File:plot_sw_mag_2010052700.png\|400px]]
		+	[[File:plot_sw_vel_2010052700.png\|350px]] <br />
		+	The blue lines are an approximation of the CME cloud and the red line denotes the shock.

	=Video Data=		=Video Data=