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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TeamSciMeetingMar09
TeamSciMeetingMar09

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PB:
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* 15:30 Line identifications with EIS and CHIANTI (Peter Young)
* 15:50 Diagnostics with the slot (Ignacio Ugarte)
* 16:20 Line identifications with EIS and CHIANTI (Peter Young)
The chances are in the last few years that if you've observed Fe XI 188.8, yo've probabluy also picked up 188.5 in the same window, so it's a little messy in that region of the spectrum.
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If my ident of Fe IX 197 is correct, it's probably a good line for temperature diagnostics.
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Can also "fix" the TRACE temperature response, so it's an important role for EIS to help better science from the imagers.
* 16:40 Diagnostics with the slot (Ignacio Ugarte)
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What we’ve learned to date on observing with the S-band antenna
* 16:10 Some techniques for observing (David Williams)
* 16:20 Raster stitching (David Brooks)
** Problems
** Some examples of studies that have proven useful in overcoming these problems
** Prospects & challenges for the future:
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** 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)
** 16:50 Flares (Ryan Milligan)
** 17:05 Very active regions (Harry Warren / John Mariska)
* 17:20 Observation Planning - Core Team proposals and HOPS (Len Culhane)
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This page (revision-83) was last changed on 02-Feb-2017 13:19 by David R WilliamsTop