07/14/2012 17:00:00 UTC - Revision history

Davidwebb: /* References */

2017-03-02T23:41:01Z

‎References

2017-03-02T23:28:05Z

‎References

2017-01-20T22:10:44Z

‎References

2015-09-09T19:44:51Z

‎References

2015-07-28T15:26:39Z

‎References

2014-10-18T07:43:08Z

‎In-Situ Data from Wind

2014-10-18T07:40:16Z

‎Image Data

2014-10-03T15:54:30Z

‎Comment Section

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‎References

2014-09-29T20:19:23Z

← Older revision		Revision as of 23:41, 2 March 2017
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	9. Gopalswamy, N., Mäkelä, P., Xie, H., Yashiro, S.: 2013,Testing the empirical shock arrival model using quadrature observations, Space Weather, 11, 661–669, doi:10.1002/2013SW000945.		9. Gopalswamy, N., Mäkelä, P., Xie, H., Yashiro, S.: 2013,Testing the empirical shock arrival model using quadrature observations, Space Weather, 11, 661–669, doi:10.1002/2013SW000945.
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		+	10. Webb, D., N. Nitta: 2017, Study on Understanding Problem Forecasts of ISEST Campaign Flare-CME Events, Solar Phys., submitted.

← Older revision		Revision as of 23:28, 2 March 2017
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	6. Wang, R.; Liu, Y. D.; Wiegelmann, T.; Cheng, X.; Hu, H.; Yang, Z., Relationship between Sunspot Rotation and a Major Solar Eruption on 2012 July 12, Solar Phys., DOI: 10.1007/s11207-016-0881-6, 2016.		6. Wang, R.; Liu, Y. D.; Wiegelmann, T.; Cheng, X.; Hu, H.; Yang, Z., Relationship between Sunspot Rotation and a Major Solar Eruption on 2012 July 12, Solar Phys., DOI: 10.1007/s11207-016-0881-6, 2016.
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		+	7. Hu, H., Liu, Y.D., Wang, R., Möstl, C., Yang, Z.: 2016, Sun-To-Earth Characteristics of the 2012 July 12 Coronal Mass Ejection and Associated Geo-Effectiveness, Astrophys. J., 829, 97, doi:10.3847/0004-637X/829/2/97.
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		+	8. Marubashi, K., K.-S. Cho, H. Ishibashi: 2017, Interplanetary Magnetic Flux Rope as Agent Connecting Solar Eruptions and Geomagnetic Activities, Solar Phys., submitted.
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		+	9. Gopalswamy, N., Mäkelä, P., Xie, H., Yashiro, S.: 2013,Testing the empirical shock arrival model using quadrature observations, Space Weather, 11, 661–669, doi:10.1002/2013SW000945.

← Older revision		Revision as of 22:10, 20 January 2017
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	5. Shen, F. et al., JGR, 119, 7128, 2014		5. Shen, F. et al., JGR, 119, 7128, 2014
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		+	6. Wang, R.; Liu, Y. D.; Wiegelmann, T.; Cheng, X.; Hu, H.; Yang, Z., Relationship between Sunspot Rotation and a Major Solar Eruption on 2012 July 12, Solar Phys., DOI: 10.1007/s11207-016-0881-6, 2016.

← Older revision		Revision as of 19:44, 9 September 2015
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	4. Hess, Phillip & Zhang, Jie, ApJ, 792, 49, 2014,[http://adsabs.harvard.edu/abs/2014ApJ...792...49H Stereoscopic Study of the Kinematic Evolution of a Coronal Mass Ejection and Its Driven Shock from the Sun to the Earth and the Prediction of Their Arrival Times]		4. Hess, Phillip & Zhang, Jie, ApJ, 792, 49, 2014,[http://adsabs.harvard.edu/abs/2014ApJ...792...49H Stereoscopic Study of the Kinematic Evolution of a Coronal Mass Ejection and Its Driven Shock from the Sun to the Earth and the Prediction of Their Arrival Times]
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		+	5. Shen, F. et al., JGR, 119, 7128, 2014

@@ Line 126: / Line 126: @@
 . Cheng, X. et al., ApJ, 2014,[http://adsabs.harvard.edu/abs/2014arXiv1405.4923C Formation of a Double-decker Magnetic Flux Rope in the Sigmoidal Solar Active Region 11520]
-. Moestl, C. et al., ApJ, 787, 119, 2014
+. Moestl, C. et al., Connecting speeds, directions and arrival times of 22 coronal mass ejections from the Sun to 1 AU, ApJ, 787, 119, 2014
 . Hess, Phillip & Zhang, Jie, ApJ, 792, 49, 2014,[http://adsabs.harvard.edu/abs/2014ApJ...792...49H Stereoscopic Study of the Kinematic Evolution of a Coronal Mass Ejection and Its Driven Shock from the Sun to the Earth and the Prediction of Their Arrival Times]

@@ Line 33: / Line 33: @@
 [[File:ejectal.jpg|300px]]
 [[File:ejecta2.jpg|300px]]
-[[test.png]]
 ** The fitted coefficients of ejecta 1 are:

@@ Line 20: / Line 20: @@
 ** There are possible two ejecta. The insitu data and Flux rope fitting could be found in the section of in-situ data from Wind below (2014/04/18, Yuming Wang)
-The event produced an intense geomagnetic storm, Dst = -127nT. [added by D. Webb]
+*The event produced an intense geomagnetic storm, Dst = -127nT. [added by D. Webb]
 =Image Data=

← Older revision		Revision as of 00:41, 2 October 2014
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	3. Moestl, C. et al., ApJ, 787, 119, 2014		3. Moestl, C. et al., ApJ, 787, 119, 2014
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		+	4. Hess, Phillip & Zhang, Jie, ApJ, 792, 49, 2014,[http://adsabs.harvard.edu/abs/2014ApJ...792...49H Stereoscopic Study of the Kinematic Evolution of a Coronal Mass Ejection and Its Driven Shock from the Sun to the Earth and the Prediction of Their Arrival Times]

← Older revision		Revision as of 20:19, 29 September 2014
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	*04/17 Discussion in Hefei-China workshop		*04/17 Discussion in Hefei-China workshop
	** There are possible two ejecta. The insitu data and Flux rope fitting could be found in the section of in-situ data from Wind below (2014/04/18, Yuming Wang)		** There are possible two ejecta. The insitu data and Flux rope fitting could be found in the section of in-situ data from Wind below (2014/04/18, Yuming Wang)
		+
		+	The event produced an intense geomagnetic storm, Dst = -127nT. [added by D. Webb]