03/17/2013 05:30:00 UTC - Revision history

Davidwebb: /* References */

2017-03-06T18:13:29Z

‎References

Moestlc: /* Comment Section */

2015-10-19T13:09:53Z

‎Comment Section

Moestlc: /* Comment Section */

2015-10-19T13:07:27Z

‎Comment Section

Moestlc: /* Comment Section */

2015-10-19T13:07:16Z

‎Comment Section

Moestlc: /* Comment Section */

2015-10-19T13:07:02Z

‎Comment Section

Moestlc: /* Interplanetary propagation */

2015-10-19T13:06:24Z

‎Interplanetary propagation

Moestlc: /* Interplanetary propagation */

2015-10-19T13:06:16Z

‎Interplanetary propagation

Moestlc: /* Interplanetary propagation */

2015-10-19T13:05:36Z

‎Interplanetary propagation

Moestlc: /* Interplanetary propagation */

2015-10-19T13:05:28Z

‎Interplanetary propagation

Moestlc: /* Interplanetary propagation */

2015-10-19T13:03:48Z

‎Interplanetary propagation

← Older revision		Revision as of 18:13, 6 March 2017
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	=References=		=References=
		+
		+	*Wu, Chin-Chun, Kan Liou, Angelos Vourlidas, Simon Plunkett, Murray Dryer, S. T. Wu,
		+	and Richard A. Mewald, Global Magnetohydrodynamic Simulation of the March 15, 2013 Coronal Mass Ejection Event - Interpretation of the 30-80 Mev Proton Flux, JGR, 121, doi:10.1002/2015JA021051, 2016.
		+	*Wu, Chin-Chun, Kan Liou, S. T. Wu, Murray Dryer, and Simon Plunkett, Radial Dependence of Solar Energetic Particles Derived from the 15 March 2013 Solar Energetic Particle Event and Global MHD Simulation, in Proceedings of Solar Wind 14, held in Shandong University, 22-26 June 2015, AIP Conf. Proc. 1720, 070008, doi: 10.1063/1.4943845, 2016. http://scitation.aip.org/content/aip/proceeding/aipcp/10.1063/1.4943845.

@@ Line 16: / Line 16: @@
 http://www.helcats-fp7.eu/catalogues/wp3_cat.html  CME ids:  HCME_B__20130315_01   HCME_A__20130315_02
-ElEvo yields an arrival time at the Earth consistent with the observed one, with a drag parameter that is 0.11 (which is slightly lower than average) and a background solar wind of 400 km/s (=normal value).  (Moestl)
+ElEvo yields an arrival time at the Earth consistent with the observed one, with a drag parameter that is 0.11 (which is slightly lower than average) and a background solar wind of 400 km/s (=normal value).
 =Image Data=

@@ Line 11: / Line 11: @@
 *I used the ElEvo model for the interplanetary shock propagation (Moestl et al. 2015 Nat. Comm.) with initial CME parameters of
--- launch time: March 15 2013 1100 UT
+launch time: March 15 2013 1100 UT
--- speed: 1063 km/s at distance 25 Rs
+speed: 1063 km/s at distance 25 Rs
--- direction: W5 => this is the average of interplanetary directions by HI SSEF modeling from STEREO A and B, taken from the STEREO HI CME catalogue
+direction: W5 => this is the average of interplanetary directions by HI SSEF modeling from STEREO A and B, taken from the STEREO HI CME catalogue
 http://www.helcats-fp7.eu/catalogues/wp3_cat.html  CME ids:  HCME_B__20130315_01   HCME_A__20130315_02

@@ Line 11: / Line 11: @@
 *I used the ElEvo model for the interplanetary shock propagation (Moestl et al. 2015 Nat. Comm.) with initial CME parameters of
-- aunch time: March 15 2013 1100 UT
+-- launch time: March 15 2013 1100 UT
-- speed: 1063 km/s at distance 25 Rs
+-- speed: 1063 km/s at distance 25 Rs
-- direction: W5 => this is the average of interplanetary directions by HI SSEF modeling from STEREO A and B, taken from the STEREO HI CME catalogue
+-- direction: W5 => this is the average of interplanetary directions by HI SSEF modeling from STEREO A and B, taken from the STEREO HI CME catalogue
 http://www.helcats-fp7.eu/catalogues/wp3_cat.html  CME ids:  HCME_B__20130315_01   HCME_A__20130315_02

@@ Line 8: / Line 8: @@
 *Depressed density and temperature as well as decreasing velocity are indicative of a flux rope, but with the weak magnetic field it may just be the flank passing through the Earth. Clear shock signatures in temperature and velocity and total B, more of a gradual increase in density. (Hess)
-*The shock arrival time at Wind is 2013-03-17 05:31 UT. The CME propagation from Sun to Earth can be very well modeled with ElEvo. This CME should have impacted Messenger at Mercury (at least with the shock) on early March 16; MESSENGER/Mercury are roughly 30 degrees west of the Sun-Earth line. (Moestl)
+*The CME propagation from Sun to Earth can be very well modeled with ElEvo (see eps plot below). This CME should have impacted Messenger at Mercury (at least with the shock) on early March 16; MESSENGER/Mercury are roughly 30 degrees west of the Sun-Earth line. (Moestl)
 *I used the ElEvo model for the interplanetary shock propagation (Moestl et al. 2015 Nat. Comm.) with initial CME parameters of
-launch time: March 15 2013 1100 UT
+- aunch time: March 15 2013 1100 UT
-speed: 1063 km/s at distance 25 Rs
+- speed: 1063 km/s at distance 25 Rs
-direction: W5 => this is the average of interplanetary directions by HI SSEF modeling from STEREO A and B, taken from the STEREO HI CME catalogue
+- direction: W5 => this is the average of interplanetary directions by HI SSEF modeling from STEREO A and B, taken from the STEREO HI CME catalogue
 http://www.helcats-fp7.eu/catalogues/wp3_cat.html  CME ids:  HCME_B__20130315_01   HCME_A__20130315_02

@@ Line 28: / Line 28: @@
 ==Interplanetary propagation==
 [[File:elevo_2013_march.eps|400px]]
 ==Heliospheric Imager Data==

@@ Line 27: / Line 27: @@
 ==Interplanetary propagation==
-[[File:elevomarch13.png|400px]]
+[[File:elevo_2013_march.eps.png|400px]]
 ==Heliospheric Imager Data==