Working Group 3 - Revision history

Jie Zhang at 01:59, 1 February 2015

2015-02-01T01:59:08Z

2013-06-24T19:01:56Z

2013-06-20T09:25:43Z

‎Future Plan and Action Items

2013-06-20T09:24:40Z

‎Future Plan and Action Items

2013-06-20T09:23:40Z

‎Future Plan and Action Items

2013-06-20T08:22:13Z

‎Future Plan and Action Items

2013-06-20T08:15:26Z

‎Forecasting the CME Arrival and Impact (with WG4 Campaign Events)

2013-06-20T08:14:23Z

‎Forecasting the CME Arrival and Impact (with WG4 Campaign Events)

2013-06-20T08:12:19Z

‎Impact on Geospace

2013-06-20T08:02:31Z

‎Scientific and Modeling Questions

← Older revision		Revision as of 01:59, 1 February 2015
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−	Simulation group led by Dusan Odstrcil (USA~~) and Fang Shen (China~~); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)	+	Simulation group led by Fang Shen (China) and Dusan Odstrcil (USA); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)

	A brief summary of the activity of WG3 at the workshop can be found [http://solar.gmu.edu/wiki/presentations/WG3_summary.pdf here]. <br>		A brief summary of the activity of WG3 at the workshop can be found [http://solar.gmu.edu/wiki/presentations/WG3_summary.pdf here]. <br>

← Older revision		Revision as of 19:01, 24 June 2013
Line 1:		Line 1:
	Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)		Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)
		+
		+	A brief summary of the activity of WG3 at the workshop can be found [http://solar.gmu.edu/wiki/presentations/WG3_summary.pdf here]. <br>

	=='''Scientific Objectives'''==		=='''Scientific Objectives'''==

@@ Line 123: / Line 123: @@
 *Investigate Mechanisms, Processes, Forces, Energies, and Interactions (with WG2 Theory)
 *Forecast and validate the CME Arrival and Impact (with WG4 Campaign Events)
-*standard outputs for observer (synthetic in situ plots and data, height-time plots and data of shock and leading edge of the driver, other  structures on request)
+*standard outputs for observers (synthetic in situ plots and data, height-time plots and data of shock and leading edge of the driver)
 <br/>

@@ Line 123: / Line 123: @@
 *Investigate Mechanisms, Processes, Forces, Energies, and Interactions (with WG2 Theory)
 *Forecast and validate the CME Arrival and Impact (with WG4 Campaign Events)
-*standard outputs for observer (synthetic in situ plots, height-time plots of leading edges, other structures on request)
+*standard outputs for observer (synthetic in situ plots and data, height-time plots and data of shock and leading edge of the driver, other  structures on request)
 <br/>

@@ Line 123: / Line 123: @@
 *Investigate Mechanisms, Processes, Forces, Energies, and Interactions (with WG2 Theory)
 *Forecast and validate the CME Arrival and Impact (with WG4 Campaign Events)
 <br/>

@@ Line 118: / Line 118: @@
 =='''Future Plan and Action Items '''==
 <br/>
-In the next 16 months, we will:
+In the next 16 months (by the next ISEST workshop), we will:
 * Make simulation of the ISEST Event Periods (with WG1) for all (ENLIL model), and for major CME events (COIN-TVD model)
@@ Line 124: / Line 124: @@
 *Forecast and validate the CME Arrival and Impact (with WG4 Campaign Events)
 <br/>
 =='''Overview of the models used in ISEST '''==
 *COIN-TVD (Corona-Interplanetary Total Variation Diminishing ): 1Rs-beyond 1AU: 3D MHD model, transients: magnetized plasma blob model

@@ Line 50: / Line 50: @@
 * Arrival time (ejecta, shocks)
-* Geo-effectiveness (Bz events)
+* Geo-effectiveness (Bz for single and multi-events)
 * Energetic particles (IMF connectivity to shock front)

@@ Line 36: / Line 36: @@
 * What are the key model-input parameters for CME simulation? Direction? Speed?
 * What can be done regarding the geomagnetic-activity forecasting?
-* What are the conditions for propagation of long-duration solar energetic particles (SEPs)?
+* What are the conditions for long-duration solar energetic particles (SEPs) events?
 <br/>
 === Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ===

@@ Line 21: / Line 21: @@
 <br/>
-===Propagation and interaction===
+===Propagation and interaction of ICMEs===
 *How the corona heating process affect the Propagation?
 *How to control the div(B) during the simulation?
@@ Line 31: / Line 31: @@
 *How successive CMEs exchanges momentum, energies with each other?
 <br/>
-===Impact===
+===Impact on Geospace===
 * What are forecasting-performances of different empirical, analytical, and numerical models?
 * How well models reproduce heliospheric kinematics of ICMEs?