Working Group 5 - Revision history

Ns902: sentence inclusion for new CME event added to list

2018-07-18T19:54:35Z

sentence inclusion for new CME event added to list

Spatsour at 09:31, 12 June 2015

2015-06-12T09:31:15Z

Spatsour at 13:30, 24 January 2015

2015-01-24T13:30:37Z

Spatsour at 11:48, 23 December 2014

2014-12-23T11:48:53Z

Spatsour at 18:23, 20 December 2014

2014-12-20T18:23:11Z

Spatsour at 18:21, 20 December 2014

2014-12-20T18:21:31Z

Spatsour at 18:07, 20 December 2014

2014-12-20T18:07:58Z

Spatsour at 18:07, 20 December 2014

2014-12-20T18:07:23Z

Spatsour at 19:40, 24 November 2014

2014-11-24T19:40:33Z

Spatsour at 13:26, 24 November 2014

2014-11-24T13:26:31Z

@@ Line 42: / Line 42: @@
 * Prepare a list of CMEs of which their near-Sun magnetic field has been already been deduced by at least one method.
 <b> Please fill in the table below by the end of August 2015. </b> Events that you also plan to deduce  their magnetic fields could be also included in the table.
-[[List of CMEs for WG5 Analysis]]
+[[List of CMEs for WG5 Analysis]].  4 New CME events added from CCMC international forum Bz team for MHD model metric coordination [edit: July 2018]
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@@ Line 41: / Line 41: @@
 ----
 * Prepare a list of CMEs of which their near-Sun magnetic field has been already been deduced by at least one method.
-<b> Please fill in the table below by the end of February 2015. </b> Events that you also plan to deduce  their magnetic fields could be also included in the table.
+<b> Please fill in the table below by the end of August 2015. </b> Events that you also plan to deduce  their magnetic fields could be also included in the table.
 [[List of CMEs for WG5 Analysis]]
 ----

← Older revision		Revision as of 13:30, 24 January 2015
Line 1:		Line 1:
−	This page is a summary of Working Group 5 (WG5) led by Spiros Patsourakos (Greece). WG5 is dedicated to predicting the southern magnetic field component of CMEs.	+	This page is a summary of Working Group 5 (WG5) led by Spiros Patsourakos (Greece). WG5 is dedicated to predicting the southern magnetic field component of CMEs at 1 AU.

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@@ Line 21: / Line 21: @@
 =='''Methodology'''==
-* Deduce/estimate near-Sun |B| of CMEs (e.g., radio, flux-rope model, magnetic helicity, CME-driven shocks)
+* Deduce/estimate near-Sun |B| of CMEs (e.g., radio, coronal polarization, flux-rope model, magnetic helicity, CME-driven shocks)
 * Deduce near-Sun orientation of CMEs (e.g., geometrical CME modeling)
 * Propagate near-Sun |B| to 1 AU (e.g., theoretical/observational scaling-laws, MHD modeling)

@@ Line 14: / Line 14: @@
 rope structure
 of CMEs/ICMEs from observations and models. It also aims to
-predict the intensity and possibly the duration of  the Bs in ICMEs
+predict the intensity and possibly the duration of the Bs in ICMEs
 upon arrival at Earth.

@@ Line 1: / Line 1: @@
-This page is a summary of the work of Working Group 5  (WG5) led by Spiros Patsourakos (Greece). WG5 is dedicated to predicting the southern magnetic field component of CMEs.
+This page is a summary of Working Group 5  (WG5) led by Spiros Patsourakos (Greece). WG5 is dedicated to predicting the southern magnetic field component of CMEs.
 ----
@@ Line 5: / Line 5: @@
 =='''WG5 Statement'''==
-The presence of southward magnetic fields in ICMEs are
+The presence of southward magnetic fields (Bs) in ICMEs is
 the most important factor in producing geomagnetic storms.
-The challenge is that direct observations of magnetic fields near the Sun
+The challenge is that direct observations of the magnetic field vectors near the Sun
 are extremely limited: currently possible only in the
 photosphere/chromosphere
-at the solar end and by in-situ observations at 1 AU.
+in the solar end and by in-situ observations at 1 AU.
-WG5 aims to understand and reconstruct the possible flux
+WG5 aims to understand and reconstruct the possible  magnetic flux
-rope magnetic structure
+rope structure
 of CMEs/ICMEs from observations and models. It also aims to
-predict the intensity and the duration of of the Bs in ICMEs
+predict the intensity and possibly the duration of  the Bs in ICMEs
-upon arriving at the Earth.
+upon arrival at Earth.
 ----
@@ Line 21: / Line 21: @@
 =='''Methodology'''==
-* Deduce near-Sun |B| of CMEs (e.g., radio, flux-rope model, magnetic helicity, CME-driven shocks)
+* Deduce/estimate near-Sun |B| of CMEs (e.g., radio, flux-rope model, magnetic helicity, CME-driven shocks)
 * Deduce near-Sun orientation of CMEs (e.g., geometrical CME modeling)
-* Propagate near-Sun |B| to 1 AU (theoretical/observational scaling-laws, MHD modeling)
+* Propagate near-Sun |B| to 1 AU (e.g., theoretical/observational scaling-laws, MHD modeling)
 * Propagate near-Sun orientation to 1 AU (MHD modeling)
 * Compare predictions with observations at 1 AU (MC fitting)
@@ Line 31: / Line 31: @@
 ==='''Preliminary Work Plan'''===
 ----
-* Find suitable datasets for near-Sun |B| field calculations applicable to as many of the available methods as possible --- <b> start with events already analysed </b> by the various team members ----coordinate w/ the data and campaign WGs (yrs 1-2)
+* Find suitable datasets for near-Sun |B| field calculations applicable to as many of the available methods as possible --- <b> start with events already analysed </b> by  various team members ----coordinate w/ the data and campaign WGs (yrs 1-2)
 * Assess the pros & cons of the various methods of near-Sun |B| determination -- coordinate w/ the theory and modeling WGs (yrs 1-2)
 * Apply methods (existing or improved) to a sample of CMEs and determine near-Sun |B| -> paper and list of events/data (yrs 2-3)
@@ Line 40: / Line 40: @@
 ==='''Current Action Items'''===
 ----
-* Prepare a list of CMEs of which their near-Sun magnetic field has been already been deduced, by at least one method.
+* Prepare a list of CMEs of which their near-Sun magnetic field has been already been deduced by at least one method.
-<b> Please fill in the table below by end of January 2015. </b> Events that you also plan to analyze their magnetic fields could be also included in the table.
+<b> Please fill in the table below by the end of February 2015. </b> Events that you also plan to deduce  their magnetic fields could be also included in the table.
 [[List of CMEs for WG5 Analysis]]
 ----

← Older revision		Revision as of 18:07, 20 December 2014
Line 1:		Line 1:
−	This page is a summary of the work by Working Group 5 led by Spiros Patsourakos (Greece). WG5 is dedicated to predicting the southern magnetic field component of CMEs.	+	This page is a summary of the work of Working Group 5 (WG5) led by Spiros Patsourakos (Greece). WG5 is dedicated to predicting the southern magnetic field component of CMEs.

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← Older revision		Revision as of 19:40, 24 November 2014
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−	This page is a summary of the work by Working Group 5, dedicated to predicting the southern magnetic field component of CMEs	+	This page is a summary of the work by Working Group 5, dedicated to predicting the southern magnetic field component of CMEs.

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← Older revision		Revision as of 13:26, 24 November 2014
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−	~~[[http://solar.gmu.edu/heliophysics/index.php/MYNEWTABLE Link to this]]~~