Difference between revisions of "Working Group 4"
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| − | Campaign Event Group led by Nariaki Nitta (USA), Luciano | + | |
| + | Campaign Event Group led by Nariaki Nitta (USA), Luciano Rodriguez (Belgium); At-large leaders: David Webb (USA) | ||
| + | |||
| + | ==Objectives== | ||
| + | |||
| + | *To identify interesting or controversial Earth-Affecting CME/ICME pairs during the STEREO era (from 2007) | ||
| + | |||
| + | *To analyse the complications that arise when linking CMEs to ICMEs | ||
| + | |||
| + | *To obtain new insights that could be applied when forecasting ICME arrivals at the Earth | ||
| + | |||
| + | ==Scientific Questions, Technique Approach/Methodology== | ||
| + | |||
| + | ===What are the common issues when linking ICMEs to CMEs?=== | ||
| + | |||
| + | *Multiple events | ||
| + | |||
| + | *Stealth CMEs | ||
| + | |||
| + | *CME deflection | ||
| + | |||
| + | *etc. | ||
| + | |||
| + | ===Calculating arrival times=== | ||
| + | |||
| + | *Projected vs 3D speeds | ||
| + | |||
| + | *Propagation models (DBM, ENLIL, etc.) | ||
| + | |||
| + | *Error margins | ||
| + | |||
| + | ===When/why will a full halo CME not arrive to the Earth?=== | ||
| + | |||
| + | ===When/why will a narrow CME (as seen from L1) arrive to the Earth?=== | ||
| + | |||
| + | ===What solar parameters can we use to provide an estimation of geoeffectivity?=== | ||
| + | |||
| + | |||
| + | ==Preliminary list of events== | ||
| + | |||
| + | *3 April 2010 | ||
| + | |||
| + | *1-4 August 2010 | ||
| + | |||
| + | *14-15 February 2011 | ||
| + | |||
| + | *12 July 2012 | ||
| + | |||
| + | *23 July 2012 | ||
| + | |||
| + | *28 September 2012 | ||
| + | |||
| + | *5-9 October 2012 | ||
| + | |||
| + | *6 February 2013 | ||
| + | |||
| + | *12-17 March 2013 | ||
| + | |||
| + | *11-14 April, 2013 | ||
| + | |||
| + | *31 May 2013 | ||
| + | |||
| + | *MiniMAx24 list (https://igam02ws.uni-graz.at/mediawiki/index.php?title=Main_Page:Event_Studies) | ||
| + | |||
| + | *WG1 events | ||
| + | |||
| + | ==Future Plan== | ||
| + | TBD | ||
Revision as of 05:07, 4 June 2013
Campaign Event Group led by Nariaki Nitta (USA), Luciano Rodriguez (Belgium); At-large leaders: David Webb (USA)
Contents
Objectives
- To identify interesting or controversial Earth-Affecting CME/ICME pairs during the STEREO era (from 2007)
- To analyse the complications that arise when linking CMEs to ICMEs
- To obtain new insights that could be applied when forecasting ICME arrivals at the Earth
Scientific Questions, Technique Approach/Methodology
What are the common issues when linking ICMEs to CMEs?
- Multiple events
- Stealth CMEs
- CME deflection
- etc.
Calculating arrival times
- Projected vs 3D speeds
- Propagation models (DBM, ENLIL, etc.)
- Error margins
When/why will a full halo CME not arrive to the Earth?
When/why will a narrow CME (as seen from L1) arrive to the Earth?
What solar parameters can we use to provide an estimation of geoeffectivity?
Preliminary list of events
- 3 April 2010
- 1-4 August 2010
- 14-15 February 2011
- 12 July 2012
- 23 July 2012
- 28 September 2012
- 5-9 October 2012
- 6 February 2013
- 12-17 March 2013
- 11-14 April, 2013
- 31 May 2013
- WG1 events
Future Plan
TBD
