Dear Leon, I forget to ask for support of TRACE during the April campaign JOP 178 Filament a nd prominence (Hinode, SUMER)
April 23 to 29 (5 days except sunday and monday) from 5 UT to 11 UT.
COuld TRACE support us?
I will send you the study on monday when I will be back to Meudon. My best regards Brigitte
Helen et al.,
I can't let this go uncommented. Even though this paper was accepted (I know, I was the editor) I disagree with the conclusion that hot loops are fuzzier. Yes, that's what you see, but it is also explainable if the hot parts of the AR have many fine threads (unresolved at present resolution) with a large filling factor. That as the conclusion Joan and I came to from analyzing 284A data.
Anyway, this won't be settled until we fly an imager with higher resolution. We're proposing one this year and I'm hoping we get the chance to clear this up, finally. Cheers,
Leon _______________________________________________ Loops mailing list Loops@solar.physics.montana.edu https://mithra.physics.montana.edu/mailman/listinfo/loops