Meilleurs voeux pour 2009, pour le succes du hot channel et aussi plein d'autres choses. Amities, jcv
Jean-François Hochedez a écrit :
Dear all,
I'd like the loop community to know that I still strive to embark a high resolution hot channel as part of the EUI instrument of Solar Orbiter. This is not easy as our overall mass budget has been reduced from 21kg to ~18kg. Yet, there are still a couple of tracks that allow holding on. The active support of some of you will play a role, and a presentation at the third S.O. workshop in Sorrento next May could be one element among other useful actions.
Best wishes,
Jean-François
Jean-Francois Hochedez j-f.hochedez@sidc.be Royal Observatory of Belgium Solar Physics Department Circular Avenue, 3. B1180 Brussels Belgium http://homepage.oma.be/hochedez/
-----Original Message----- From: loops-bounces@mithra.physics.montana.edu [mailto:loops-bounces@mithra.physics.montana.edu] On Behalf Of H.E.Mason@damtp.cam.ac.uk Sent: mercredi 7 janvier 2009 10:28 To: reale@astropa.unipa.it Cc: A mailing list for scientists involved in the observation and modeling ofsolar loop structures; loops@mithra.physics.montana.edu Subject: Re: [Loops] EIS AR Loops - Tripathi et al, 2009, ApJ
Agreed Fabio,
my sentiments exactly, and we definitely endorse higher spatial resolution observations across a broad temperature range.
Best wishes, helen
On Jan 6 2009, reale@astropa.unipa.it wrote:
I agree with Leon, but I also think that the paper only certifies that the loops look fuzzier in hotter lines. There may be no real contradiction with Leon's perspective. Of course, we all sustain Leon's new imager. Ciao Fabio
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
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