Hi everyone,
In the spirit of a number of recent papers that have been focused on trying to determine the dominant components of the emission in the wavelength channels of imaging instruments (AIA, in particular), Jim and I would like to share with you all a link to a paper on this very topic that was recently published in the ApJ Supplement Series:
http://iopscience.iop.org/0067-0049/194/2/26/pdf/apjs_194_2_26.pdf
Our aim in carrying out the work described in this paper was to provide a large amount of quantitative data from our modeling studies that we hope will be of use in the analysis of observationally gathered data.
Best wishes,
Steve
-----Original Message----- From: loops-bounces@solar.physics.montana.edu [mailto:loops-bounces@solar.physics.montana.edu] On Behalf Of Paola Testa Sent: Tuesday, September 20, 2011 10:00 AM To: A mailing list for scientists involved in the observation and modeling of solar loop structures Cc: Juan Martinez Sykora Subject: [Loops] Forward modeling of emission in SDO/AIA passbands from dynamic 3D simulations
Hello all,
here is a link to a preprint of a paper, accepted for publication on ApJ, that is also discussing issues related to the interpretation of AIA observations:
http://adsabs.harvard.edu/abs/2011arXiv1109.0704M
cheers, Paola
On 9/9/11 12:03 PM, Giulio Del Zanna wrote:
Dear colleagues,
here is a link to a preprint that discusses various (important) issues related to the interpretation of AIA data:
http://solar.physics.montana.edu/cgi-bin/eprint/index.pl?entry=15555
Those of you that were present at the excellent Mallorca meeting might recall the issues we raised there. The paper, which follows on from O'Dwyer et al., contains more.
I encourage all to follow the example in the Appendix to calculate your own AIA responses using CHIANTI. We will soon release v.7, but do not expect huge differences. We are working to try and improve the atomic data for AIA, more to come.
best wishes,
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