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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* HEM would be interested to put together a joint EIS XRT temperature distribution.
* LKH thinks there's a disconnect between horizontal magnetic fields
** EIS could potentially do something there
* GAD: SOT discovered spicular material that's moving at very high
* JTM we have great difficulty at getting quantitative information
** JLC is the filter ratio method working quantitatvely
*** think the XRT filter ratio people have confidence, but when you compare that with EIS
** JTM: I just want to know where the hot plasma is
** JLC: if you see it at all in XRT, it's hot, but that's qualitative
** HPW in principle should be able to put these things together. We w
* LKH: Outflow areas: what does Ca II H look like?
* HPW: could SOT provide a measure of the vector magnetic field
* LKH: how do the horizontal magnetic fields impact on heating the atmosphere
* GAD: how accurate are the XRT filter ration?
** And do we know what their temperature responses. We should get XRT to explain how they're getting these.
* HPW: think we should do what Helen has done and get cross-calibrated joint observations
* JTM: does unusual flux emergence have correspondence in EIS data.
* GAD: any energetic stuff seen in SOT: flux cancellation, we could try to tie in with something we see in EIS.
This page (revision-83) was last changed on 02-Feb-2017 13:19 by David R WilliamsTop