[Loops] new paper

[Durgesh Tripathi]

Dear all,

Please find attached a new paper on 'Active Region Moss: Basic physical parameters and their temporal variation' which has been accepted for publication in Astronomy and Astrophysics. Below is the abstract of the paper.

Context: Active region moss are transition region phenomena, first noted in the images recorded by the Transition Region and Coronal Explorer (TRACE) in $\lambda$171. Moss regions are thought to be the footpoints of hot loops (3-5~MK) seen in the core of active regions. These hot loops appear 'fuzzy' (unresolved). Therefore, it is difficult to study the physical plasma parameters in individual hot core loops and hence their heating mechanisms. Moss regions provide an excellent opportunity to study the physics of hot loops. In addition, they allow us to study the transition region dynamics in the footpoint regions.
Aim: To derive the physical plasma parameters such as temperature, electron density, and filling factors in moss regions and to study their variation over a short (an hour) and a long time period (5 consecutive days).
Methods: Primarily, we have analyzed spectroscopic observations recorded by the Extreme-ultraviolet Imaging Spectrometer (EIS) aboard Hinode. In addition we have used supplementary observations taken from TRACE and the X-Ray Telescope (XRT) aboard Hinode.
Results: The moss emission is strongest in the \ion{Fe}{xii} and \ion{Fe}{xiii} lines. Based on analyses using line ratios and emission measure we found that moss regions have a characteristic temperature of log~T[K]~=~ 6.2. The temperature structure in moss region remains almost identical from one region to another and it does not change with time. The electron densities measured at different locations in the moss regions using \ion{Fe}{xii} ratios are about 1-3~$\times$~10$^{10}$~cm$^{-3}$ and about 2-4~$\times$~10$^{9}$~cm$^{-3}$ using \ion{Fe}{xiii} and \ion{Fe}{xiv}. The densities in the moss regions are similar in different places and show very little variation over short and long time scales. The derived electron density substantially increased (by a factor of about 3-4 or even more in some cases) when a background subtraction was performed. The filling factor of the moss plasma can vary between 0.1-1 and the path length along which the emission originates is from a few 100 to a few 1000 kms long. By combining the observations recorded by TRACE, EIS and XRT, we find that the moss regions correspond to the footpoints of both hot and warm loops.

Best wishes, 
-Durgesh Tripathi








Durgesh Tripathi
Department of Applied Maths and Theoretical Physics
Centre for Mathematical Sciences
University of Cambridge
Wilberforce Road
Cambridge CB3 0WA

Ph. +44 - (0) - 1223 - 337-916

-------------- next part --------------
An HTML attachment was scrubbed...
URL: <http://mithra.physics.montana.edu/pipermail/loops/attachments/20100611/cbc388a2/attachment-0002.html>
-------------- next part --------------
A non-text attachment was scrubbed...
Name: tripathi_etal_moss_2010.pdf
Type: application/pdf
Size: 684930 bytes
Desc: not available
URL: <http://mithra.physics.montana.edu/pipermail/loops/attachments/20100611/cbc388a2/attachment-0001.pdf>
-------------- next part --------------
An HTML attachment was scrubbed...
URL: <http://mithra.physics.montana.edu/pipermail/loops/attachments/20100611/cbc388a2/attachment-0003.html>