This page (revision-83) was last changed on 02-Feb-2017 13:19 by David R Williams

This page was created on 27-Jan-2009 03:17 by David R Williams

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Version Date Modified Size Author Changes ... Change note
83 02-Feb-2017 13:19 43 KB David R Williams to previous
82 19-Mar-2009 13:50 41 KB David R Williams to previous | to last
81 18-Mar-2009 21:12 40 KB David R Williams to previous | to last

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__N.B.__ There is now enough time for 20 minutes per presentation.
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* 13:50 The thermal structure of active regions (Harry Warren)
* 14:10 Multi-component active region flows (Paul Bryans)
* 13:45 The thermal structure of active regions (Harry Warren)
* 14:00 Multi-component active region flows (Paul Bryans)
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* 14:30 Evaporated Plasma (Ryan Milligan)
* 14:15 Evaporated Plasma (Ryan Milligan)
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!!2.3 Analysis Techniques
* 14:50 Line identifications with EIS and CHIANTI (Peter Young)
!!2.3 Where to next for EIS science?
14:15 to 15:00
Not only having listened to the contributions given this afternoon, but also having considered our progress in achieving EIS's main science goals — both pre- and post-launch — it would be good to have a discussion before and after coffee on what burning questions we think are obviously being left unanswered.
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I'd like to budget 45 minutes for this.
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15:10 to 15:40
15:00
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!!2.3 Analysis Techniques (continued)
* 15:40 Diagnostics with the slot (Ignacio Ugarte)
!!2.4 Analysis Techniques
* 15:30 Line identifications with EIS and CHIANTI (Peter Young)
* 15:50 Diagnostics with the slot (Ignacio Ugarte)
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* 16:00 Some techniques for observing (David Williams)
* 16:10 Some techniques for observing (David Williams)
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** 16:15 Flares (Ryan Milligan)
** 16:35 Very active regions (Harry Warren / John Mariska)
* 16:55 Observation Planning - Core Team proposals and HOPS (Len Culhane)
** 16:25 Flares (Ryan Milligan)
** 16:45 Very active regions (Harry Warren / John Mariska)
* 17:05 Observation Planning - Core Team proposals and HOPS (Len Culhane)
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