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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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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KPD: I think the flows were hinted at with Skylab
GAD: True, but the new thing is that they're measurable, although it's difficult to say that we've seen antyyhing new so far.
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PRY: is the density in the outflows different?
PB: haven't done that yet
JTM: just a comment on all three talks: hadn't appreciated how much we've done.
But we've never fulfilled yet the promise of integrating with the other instruments, and I suspect the real discoveries are going to be from doing that. I hope that when we come back next year, we'll have made a start.
HEM: any possibility of having any workshops?
JTM: This could be a good time to start this.
GAD: coalingnments are very challenging for co-observing
JTM: but it can be addressed in some meaningful way.