ISEST - Revision history

Jie Zhang at 15:40, 15 May 2015

2015-05-15T15:40:20Z

Jie Zhang at 15:33, 15 May 2015

2015-05-15T15:33:57Z

Jie Zhang at 15:33, 15 May 2015

2015-05-15T15:33:09Z

Jie Zhang at 15:31, 15 May 2015

2015-05-15T15:31:31Z

Jie Zhang at 15:29, 15 May 2015

2015-05-15T15:29:28Z

Jie Zhang at 15:28, 15 May 2015

2015-05-15T15:28:47Z

Jie Zhang at 03:01, 1 February 2015

2015-02-01T03:01:28Z

Jie Zhang at 02:54, 1 February 2015

2015-02-01T02:54:58Z

Jie Zhang at 02:53, 1 February 2015

2015-02-01T02:53:45Z

Jie Zhang at 02:53, 1 February 2015

2015-02-01T02:53:16Z

@@ Line 15: / Line 15: @@
 '''Working Group Leaders''':  (1) WG1 (Data Group): Jie Zhang (George Mason University, USA); (2) WG2 (Theory Group): Bojan Vrsnak  (Hvar Observatory, Croatia); (3) WG4 (Simulation Group): Fang Shen (CSSAR, China); (4) WG4 (Event Campaign Group): David Webb (Boston College, USA); (5) WG5 (Bs Challenge Group): Spiros Patsourakos (University of Ioannina, Greece); (6) WG6 (SEP Group): Olga Malandraki (National Observatory of Athens, Greece); (7) MiniMax24 Campaign: Manuela Temmer ( University of Graz, Austria)
-'''Scientific Organization Committee members''': Ayumi Asai                                      Kyoto University  (Japan)
+'''Scientific Organization Committee members''': (1) Ayumi Asai (Kyoto University, Japan);  (2) Mario M. Bisi ( RAL, UK);  (3) Kyungsuk Cho (KASI; South Korea);
-Mario M. Bisi                                   RAL (UK)
+(4) Peter Gallagher (Trinity College Dublin, Ireland);  (5) Manolis K. Georgoulis (Academy of Athens, Greece); (6) Nat Gopalswamy (co-leader) (NASA/GSFC, USA); (7) Alejandro Lara (National Autonomous University, Mexico);  (8) Noe Lugaz (University of New Hampshire, USA);  (9) Alexis Rouillard  (CNRS/IRAP, France); (10)  Nandita Srivastava (Physical Research Lab, India); (11)  Manuela Temmer  (co-leader) (University of Graz, Austria); (12)  Yuri Yermolaev (Space Research Institute, Russia); (13)  Yu-Ming Wang (Univ. of Science and Technology, China); (14)  David Webb (Boston College, USA); (15)  Bojan Vrsnak (Hvar Observatory, Croatia); (16)  Jie Zhang (co-leader) (George Mason University, USA)

← Older revision		Revision as of 15:33, 15 May 2015
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	'''Working Group Leaders''': (1) WG1 (Data Group): Jie Zhang (George Mason University, USA); (2) WG2 (Theory Group): Bojan Vrsnak (Hvar Observatory, Croatia); (3) WG4 (Simulation Group): Fang Shen (CSSAR, China); (4) WG4 (Event Campaign Group): David Webb (Boston College, USA); (5) WG5 (Bs Challenge Group): Spiros Patsourakos (University of Ioannina, Greece); (6) WG6 (SEP Group): Olga Malandraki (National Observatory of Athens, Greece); (7) MiniMax24 Campaign: Manuela Temmer ( University of Graz, Austria)		'''Working Group Leaders''': (1) WG1 (Data Group): Jie Zhang (George Mason University, USA); (2) WG2 (Theory Group): Bojan Vrsnak (Hvar Observatory, Croatia); (3) WG4 (Simulation Group): Fang Shen (CSSAR, China); (4) WG4 (Event Campaign Group): David Webb (Boston College, USA); (5) WG5 (Bs Challenge Group): Spiros Patsourakos (University of Ioannina, Greece); (6) WG6 (SEP Group): Olga Malandraki (National Observatory of Athens, Greece); (7) MiniMax24 Campaign: Manuela Temmer ( University of Graz, Austria)
		+
		+	'''Scientific Organization Committee members''': Ayumi Asai Kyoto University (Japan)
		+	Mario M. Bisi RAL (UK)
		+	Kyungsuk Cho KASI (South Korea)
		+	Peter Gallagher Trinity College Dublin (Ireland)
		+	Manolis K. Georgoulis Academy of Athens (Greece)
		+	Nat Gopalswamy (co-leader) NASA (USA)
		+	Alejandro Lara National Autonomous University (Mexico)
		+	Noe Lugaz, University of New Hampshire (USA)
		+	Alexis Rouillard CNRS/IRAP (France) (confirmed)
		+	Nandita Srivastava Physical Research Lab (India)
		+	Manuela Temmer (co-leader) University of Graz (Austria)
		+	Yuri Yermolaev Space Research Institute (Russia)
		+	Yu-Ming Wang Univ. of Science and Technology (China)
		+	David Webb Boston College (USA)
		+	Bojan Vrsnak Hvar Observatory (Croatia)
		+	Jie Zhang (co-leader) George Mason University (USA)

← Older revision		Revision as of 15:33, 15 May 2015
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	'''Co-leaders''': Jie Zhang (USA) (jzhang7@gmu.edu), Manuela Temmer (Austria), Nat Gopalswamy (USA)		'''Co-leaders''': Jie Zhang (USA) (jzhang7@gmu.edu), Manuela Temmer (Austria), Nat Gopalswamy (USA)

−	'''Working Group Leaders''': (1) WG1 (Data Group): Jie Zhang (George Mason University, USA); (2) WG2 (Theory Group): Bojan Vrsnak (Hvar Observatory, Croatia); (3) WG4 (Simulation Group): Fang Shen (CSSAR, China)	+	'''Working Group Leaders''': (1) WG1 (Data Group): Jie Zhang (George Mason University, USA); (2) WG2 (Theory Group): Bojan Vrsnak (Hvar Observatory, Croatia); (3) WG4 (Simulation Group): Fang Shen (CSSAR, China); (4) WG4 (Event Campaign Group): David Webb (Boston College, USA); (5) WG5 (Bs Challenge Group): Spiros Patsourakos (University of Ioannina, Greece); (6) WG6 (SEP Group): Olga Malandraki (National Observatory of Athens, Greece); (7) MiniMax24 Campaign: Manuela Temmer ( University of Graz, Austria)

← Older revision		Revision as of 15:31, 15 May 2015
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	'''Co-leaders''': Jie Zhang (USA) (jzhang7@gmu.edu), Manuela Temmer (Austria), Nat Gopalswamy (USA)		'''Co-leaders''': Jie Zhang (USA) (jzhang7@gmu.edu), Manuela Temmer (Austria), Nat Gopalswamy (USA)

−	'''Working Group Leaders'''	+	'''Working Group Leaders''': (1) WG1 (Data Group): Jie Zhang (George Mason University, USA); (2) WG2 (Theory Group): Bojan Vrsnak (Hvar Observatory, Croatia); (3) WG4 (Simulation Group): Fang Shen (CSSAR, China)
−	== WG1 (Data Group): Jie Zhang (George Mason University, USA)==

@@ Line 13: / Line 13: @@
 '''Co-leaders''': Jie Zhang (USA) (jzhang7@gmu.edu), Manuela Temmer (Austria), Nat Gopalswamy (USA)
-'''Working Group Leaders"""
+'''Working Group Leaders'''
-== WG1 (Data Group): Jie Zhang (George Mason University, USA)
+== WG1 (Data Group): Jie Zhang (George Mason University, USA)==

← Older revision		Revision as of 15:28, 15 May 2015
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	'''Co-leaders''': Jie Zhang (USA) (jzhang7@gmu.edu), Manuela Temmer (Austria), Nat Gopalswamy (USA)		'''Co-leaders''': Jie Zhang (USA) (jzhang7@gmu.edu), Manuela Temmer (Austria), Nat Gopalswamy (USA)
		+
		+	'''Working Group Leaders"""
		+	== WG1 (Data Group): Jie Zhang (George Mason University, USA)

@@ Line 1: / Line 1: @@
-'''This wiki is specifically for data sharing and discussion forum of the ISEST program. We encourage everyone to upload any data pertaining to ICMEs to this wiki and to discuss events freely in the discussion section of each page. Please do not alter any data that is not yours without the express permission of the uploader'''
+'''This wiki is specifically for data sharing and discussion forum of the ISEST program. We encourage everyone to upload any data pertaining to ICMEs to this wiki and to discuss events freely in the discussion section of each page. Please do not alter any data that is not yours without the express permission of the uploader. For any questions of using this Wiki, email Phillip Hess at phess4@gmu.edu'''
 The '''ISEST/MiniMax24''' (International Study of Earth-Affecting Solar Transients) is one of the four projects of the [http://varsiti.org VarSITI (Variability of the Sun and Its Terrestrial Impact)] program, which runs from 2014 to 2018. The VarSITI is the current scientific program of [http://www.yorku.ca/scostep SCOSTEP (Scientific Committee on Solar-Terrestrial Physics].
@@ Line 11: / Line 11: @@
 '''Anticipated outcome''': A comprehensive database of Earth -affecting solar transients will be created, and space weather prediction capability will be significantly improved.
-'''Co-leaders''': Jie Zhang (USA), Manuela Temmer (Austria), Nat Gopalswamy (USA)
+'''Co-leaders''': Jie Zhang (USA) (jzhang7@gmu.edu), Manuela Temmer (Austria), Nat Gopalswamy (USA)

@@ Line 5: / Line 5: @@
 '''Goals and objectives''': Understand the propagation of solar transients through the space between the Sun and the Earth, and develop space weather prediction capability.
-Questions: How do coronal mass ejections (CMEs) and corotating interaction regions (CIRs) propagate and evolve, drive shocks and accelerate energetic particles in the heliosphere?
+'''Questions''': How do coronal mass ejections (CMEs) and corotating interaction regions (CIRs) propagate and evolve, drive shocks and accelerate energetic particles in the heliosphere?
-Data/theory/modeling: Establish a database of Earth -affecting solar transient events including CMEs, CIRs, flares, and energetic particle events based on remote sensing and in-situ observations from an array of spacecraft, run observation campaigns such as MiniMax24, develop empirical, theoretical, and numerical models of CME propagation and prediction, validate models using observations.
+'''Data/theory/modeling''': Establish a database of Earth -affecting solar transient events including CMEs, CIRs, flares, and energetic particle events based on remote sensing and in-situ observations from an array of spacecraft, run observation campaigns such as MiniMax24, develop empirical, theoretical, and numerical models of CME propagation and prediction, validate models using observations.
-Anticipated outcome: A comprehensive database of Earth -affecting solar transients will be created, and space weather prediction capability will be significantly improved.
+'''Anticipated outcome''': A comprehensive database of Earth -affecting solar transients will be created, and space weather prediction capability will be significantly improved.
-Co-leaders: Jie Zhang (USA), Manuela Temmer (Austria), Nat Gopalswamy (USA)
+'''Co-leaders''': Jie Zhang (USA), Manuela Temmer (Austria), Nat Gopalswamy (USA)

@@ Line 3: / Line 3: @@
 The ISEST/MiniMax24 (International Study of Earth-Affecting Solar Transients) is one of the four projects of the [http://varsiti.org VarSITI (Variability of the Sun and Its Terrestrial Impact)] program, which runs from 2014 to 2018. The VarSITI is the current scientific program of [http://www.yorku.ca/scostep SCOSTEP (Scientific Committee on Solar-Terrestrial Physics].
-Goals and objectives: Understand the propagation of solar transients through the space between the Sun and the Earth, and develop space weather prediction capability.
+'''Goals and objectives''': Understand the propagation of solar transients through the space between the Sun and the Earth, and develop space weather prediction capability.
 Questions: How do coronal mass ejections (CMEs) and corotating interaction regions (CIRs) propagate and evolve, drive shocks and accelerate energetic particles in the heliosphere?