03/31/2015 07:31:49 UTC - Revision history

Ytchi: /* Image Data */

2017-09-18T16:14:40Z

‎Image Data

Ytchi: /* Image Data */

2017-09-18T16:11:26Z

‎Image Data

Ytchi: /* Comment Section */

2017-09-18T16:06:31Z

‎Comment Section

Ytchi: /* Image Data */

2017-09-18T15:46:44Z

‎Image Data

Ytchi: /* Comment Section */

2017-09-16T18:28:06Z

‎Comment Section

Ytchi: /* Comment Section */

2017-09-16T18:27:42Z

‎Comment Section

Ytchi: /* Image Data */

2017-09-16T18:09:55Z

‎Image Data

Ytchi: /* Comment Section */

2017-09-16T18:04:38Z

‎Comment Section

Ytchi: /* Comment Section */

2017-09-16T18:03:09Z

‎Comment Section

Ytchi: Created page with "=Comment Section= *Clear shock, followed by most of the standard MC signatures (low beta, low density, rotating magnetic field, etc.), but a fairly weak total magnetic field s..."

2017-09-16T17:55:07Z

Created page with "=Comment Section= *Clear shock, followed by most of the standard MC signatures (low beta, low density, rotating magnetic field, etc.), but a fairly weak total magnetic field s..."

New page

=Comment Section=
*Clear shock, followed by most of the standard MC signatures (low beta, low density, rotating magnetic field, etc.), but a fairly weak total magnetic field strength. The CME probably wasn't passing near the nose (Hess)

=Image Data=
A combination of SWEPAM and MAG data from the ACE Satellite: <br />
[[File:plot_sw_mag_plasma_2014042000.png|350px]]
[[File:plot_sw_mag_2014042000.png|400px]]
[[File:plot_sw_vel_2014042000.png|350px]] <br />
The blue lines are an approximation of the CME cloud and the red line denotes the shock.

=Video Data=

=References=

@@ Line 6: / Line 6: @@
 A combination of MFI and SWE data from the Wind Satellite: <br />
-[[File:Example.jpg]]
+[[File:Example.jpg|400px]]
 The grey region shows an approximation of the CME cloud and the red vertical line denotes the shock.

@@ Line 6: / Line 6: @@
 A combination of MFI and SWE data from the Wind Satellite: <br />
-[[File:0331.jpg]]
+[[File:Example.jpg]]
 The grey region shows an approximation of the CME cloud and the red vertical line denotes the shock.

@@ Line 3: / Line 3: @@
 *At 03/27/2015 15:12:08, there may be a partial halo CME corresponding to this magnetic cloud. The solar source of this CME is unknown. (Yutian)
-[[File:]]=Image Data=
+=Image Data=
 A combination of MFI and SWE data from the Wind Satellite: <br />
-[[File:Example.jpg]]
+[[File:0331.jpg]]
 The grey region shows an approximation of the CME cloud and the red vertical line denotes the shock.

@@ Line 3: / Line 3: @@
 *At 03/27/2015 15:12:08, there may be a partial halo CME corresponding to this magnetic cloud. The solar source of this CME is unknown. (Yutian)
-=Image Data=
+[[File:]]=Image Data=
 A combination of MFI and SWE data from the Wind Satellite: <br />
 The grey region shows an approximation of the CME cloud and the red vertical line denotes the shock.

@@ Line 1: / Line 1: @@
 =Comment Section=
 *Clear shock, followed by most of the standard MC signatures (low beta, low density, smooth magnetic field, etc.), but a fairly weak magnetic field rotation. <br>
-*At 03/27/2015 15:12:08, there may be a partial halo CME corresponding to this magnetic cloud. The solar source of this CME is unknown.
+*At 03/27/2015 15:12:08, there may be a partial halo CME corresponding to this magnetic cloud. The solar source of this CME is unknown. (Yutian)
 =Image Data=

@@ Line 3: / Line 3: @@
 =Image Data=
-A combination of SWEPAM and MAG data from the ACE Satellite: <br />
+A combination of MFI and SWE data from the Wind Satellite: <br />
-[[File:plot_sw_mag_plasma_2014042000.png|350px]]
-[[File:plot_sw_mag_2014042000.png|400px]]
+The grey region shows an approximation of the CME cloud and the red vertical line denotes the shock.
 =Video Data=
 =References=