03/08/2012 11:00:00 UTC - Revision history

Davidwebb: /* References */

2017-03-10T21:24:59Z

‎References

Davidwebb: /* References */

2017-03-06T18:02:45Z

‎References

Davidwebb: /* References */

2017-03-06T18:02:12Z

‎References

Phess4: /* In-Situ Data */

2013-07-02T17:54:13Z

‎In-Situ Data

Phess4: /* References */

2013-07-01T16:33:12Z

‎References

Phess4: /* Comment Section */

2013-07-01T16:33:02Z

‎Comment Section

Moestlc: /* Comment Section */

2013-06-20T07:24:18Z

‎Comment Section

Phess4: /* Video Data */

2013-06-19T08:59:52Z

‎Video Data

Jie Zhang at 03:56, 3 June 2013

2013-06-03T03:56:17Z

Jie Zhang at 03:55, 3 June 2013

2013-06-03T03:55:04Z

@@ Line 23: / Line 23: @@
 *Liu, Y. D., Luhmann, J. G., Lugaz, N., Möstl, C., Davies, J. A., Bale, S. D., and Lin, R. P., On Sun-to-Earth Propagation of Coronal Mass Ejections, 2013, Astrophys. J., 769, 45 (http://iopscience.iop.org/article/10.1088/0004-637X/769/1/45/pdf)
 *Liu, Y. D., Richardson, J. D., Wang, C., and Luhmann, J. G., Propagation of the 2012 March Coronal Mass Ejections from the Sun to Heliopause, 2014, Astrophys. J. Lett., 788, L28 (http://iopscience.iop.org/article/10.1088/2041-8205/788/2/L28/pdf)
 *Wood, B. E., J. L. Lean, S. E. McDonald, and Y.-M. Wang (2016), Comparative ionospheric impacts and solar origins of nine strong geomagnetic storms in 2010–2015, J. Geophys. Res., 121, 4938–4965, doi:10.1002/2015JA021953.
-*Patsourakos, S. et al., The Major Geoeffective Solar Eruptions of 2012 March 7: Comprehensive Sun-To-Earth Analysis, Astrophys. J., 817, 14, 2016
+*Patsourakos, S. et al., The Major Geoeffective Solar Eruptions of 2012 March 7: Comprehensive Sun-To-Earth Analysis, Astrophys. J., 817, 14, 2016.

@@ Line 20: / Line 20: @@
 =References=
-- Wang, R., Liu, Y. D., Yang, Z., and Hu, H., Magnetic Field Restructuring Associated with Two Successive Solar Eruptions, 2014, Astrophys. J., 791, 84 (http://iopscience.iop.org/article/10.1088/0004-637X/791/2/84/pdf)
+*Wang, R., Liu, Y. D., Yang, Z., and Hu, H., Magnetic Field Restructuring Associated with Two Successive Solar Eruptions, 2014, Astrophys. J., 791, 84 (http://iopscience.iop.org/article/10.1088/0004-637X/791/2/84/pdf)
-- Liu, Y. D., Luhmann, J. G., Lugaz, N., Möstl, C., Davies, J. A., Bale, S. D., and Lin, R. P., On Sun-to-Earth Propagation of Coronal Mass Ejections, 2013, Astrophys. J., 769, 45 (http://iopscience.iop.org/article/10.1088/0004-637X/769/1/45/pdf)
+*Liu, Y. D., Luhmann, J. G., Lugaz, N., Möstl, C., Davies, J. A., Bale, S. D., and Lin, R. P., On Sun-to-Earth Propagation of Coronal Mass Ejections, 2013, Astrophys. J., 769, 45 (http://iopscience.iop.org/article/10.1088/0004-637X/769/1/45/pdf)
-- Liu, Y. D., Richardson, J. D., Wang, C., and Luhmann, J. G., Propagation of the 2012 March Coronal Mass Ejections from the Sun to Heliopause, 2014, Astrophys. J. Lett., 788, L28 (http://iopscience.iop.org/article/10.1088/2041-8205/788/2/L28/pdf)
+*Liu, Y. D., Richardson, J. D., Wang, C., and Luhmann, J. G., Propagation of the 2012 March Coronal Mass Ejections from the Sun to Heliopause, 2014, Astrophys. J. Lett., 788, L28 (http://iopscience.iop.org/article/10.1088/2041-8205/788/2/L28/pdf)
-- Wood, B. E., J. L. Lean, S. E. McDonald, and Y.-M. Wang (2016), Comparative ionospheric impacts and solar origins of nine strong geomagnetic storms in 2010–2015, J. Geophys. Res., 121, 4938–4965, doi:10.1002/2015JA021953.
+*Wood, B. E., J. L. Lean, S. E. McDonald, and Y.-M. Wang (2016), Comparative ionospheric impacts and solar origins of nine strong geomagnetic storms in 2010–2015, J. Geophys. Res., 121, 4938–4965, doi:10.1002/2015JA021953.
-- Patsourakos, S. et al., The Major Geoeffective Solar Eruptions of 2012 March 7: Comprehensive Sun-To-Earth Analysis, Astrophys. J., 817, 14, 2016
+*Patsourakos, S. et al., The Major Geoeffective Solar Eruptions of 2012 March 7: Comprehensive Sun-To-Earth Analysis, Astrophys. J., 817, 14, 2016

← Older revision		Revision as of 18:02, 6 March 2017
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	=References=		=References=

−	*Ying Liu et al. ~~2013 ApJ~~	+	- Wang, R., Liu, Y. D., Yang, Z., and Hu, H., Magnetic Field Restructuring Associated with Two Successive Solar Eruptions, 2014, Astrophys. J., 791, 84 (http://iopscience.iop.org/article/10.1088/0004-637X/791/2/84/pdf)
		+	- Liu, Y. D., Luhmann, J. G., Lugaz, N., Möstl, C., Davies, J. A., Bale, S. D., and Lin, R. P., On Sun-to-Earth Propagation of Coronal Mass Ejections, 2013, Astrophys. J., 769, 45 (http://iopscience.iop.org/article/10.1088/0004-637X/769/1/45/pdf)
		+	- Liu, Y. D., Richardson, J. D., Wang, C., and Luhmann, J. G., Propagation of the 2012 March Coronal Mass Ejections from the Sun to Heliopause, 2014, Astrophys. J. Lett., 788, L28 (http://iopscience.iop.org/article/10.1088/2041-8205/788/2/L28/pdf)
		+	- Wood, B. E., J. L. Lean, S. E. McDonald, and Y.-M. Wang (2016), Comparative ionospheric impacts and solar origins of nine strong geomagnetic storms in 2010–2015, J. Geophys. Res., 121, 4938–4965, doi:10.1002/2015JA021953.
		+	- Patsourakos, S. et al., The Major Geoeffective Solar Eruptions of 2012 March 7: Comprehensive Sun-To-Earth Analysis, Astrophys. J., 817, 14, 2016

@@ Line 7: / Line 7: @@
 ==In-Situ Data==
 A combination of SWEPAM and MAG data from the ACE Satellite: <br />
-[[File:plot_sw_mag_plasma_2012030700.png|350px]]
+[[File:plot_sw_mag_plasma_2012030800.png|350px]]
-[[File:plot_sw_mag_2012030700.png|400px]]
+[[File:plot_sw_mag_2012030800.png|400px]]
-[[File:plot_sw_vel_2012030700.png|350px]] <br />
+[[File:plot_sw_vel_2012030800.png|350px]] <br />
 The blue lines are an approximation of the CME cloud and the red line denotes the shock.

← Older revision		Revision as of 16:33, 1 July 2013
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	=References=		=References=
		+
		+	*Ying Liu et al. 2013 ApJ

@@ Line 3: / Line 3: @@
 **X1 flare, fast CME, originated from the eastern hemisphere (~N18E42)
 **Solar wind plasma data is corrupted.
 =Image Data=

← Older revision		Revision as of 08:59, 19 June 2013
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	=Video Data=		=Video Data=
		+
		+	=References=

← Older revision		Revision as of 03:56, 3 June 2013
Line 2:		Line 2:
	*A fair ICME event, but strong solar source		*A fair ICME event, but strong solar source
	**X1 flare, fast CME, originated from the eastern hemisphere (~N18E42)		**X1 flare, fast CME, originated from the eastern hemisphere (~N18E42)
		+	**Solar wind plasma data is corrupted.

← Older revision		Revision as of 03:55, 3 June 2013
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	=Comment Section=		=Comment Section=
		+	*A fair ICME event, but strong solar source
		+	**X1 flare, fast CME, originated from the eastern hemisphere (~N18E42)
		+

	=Image Data=		=Image Data=