[Loops] EIS AR Loops - Tripathi et al, 2009, ApJ

[Nakariakov, Valery]

Dear Leon, dear all,

I would like to mention that we also have MHD seismological evidence
of fine structuring of the hot corona, e.g.

\bibitem[van Doorsselaere et 
al.(2008)]{2008A&A...491L...9V} van Doorsselaere, T., Brady, C.~S., Verwichte, E., Nakariakov, V.~M.\ 2008.\ Seismological demonstration of perpendicular density structuring in the solar corona.\ Astronomy and Astrophysics 491, L9-L12. 

http://adsabs.harvard.edu/abs/2008A%26A...491L...9V  

All the best,

Valery



-----Original Message-----
From: loops-bounces at mithra.physics.montana.edu on behalf of Leon Golub
Sent: Tue 06/01/2009 18:50
To: loops at mithra.physics.montana.edu
Cc: H.E.Mason at damtp.cam.ac.uk
Subject: Re: [Loops] EIS AR Loops - Tripathi et al, 2009, ApJ
 
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
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