Hello everyone,
it was very nice to meet you all last week in Florence :) In case anyone is interested in some photos, here they are: http://picasaweb.google.com/jaroslav.dudik/Firenze2009# I hope I am not abusing the loops mailing list in this way. If yes, please ignore this message.
My best regards,
- Jaro
-- Jaroslav Dudik PhD. student, fourth year Division of Astronomy and Astrophysics Department of Astronomy, Physics of the Earth and Meteorology Faculty of Mathematics, Physics and Informatics Comenius University Mlynska Dolina F2-203 842 48 Bratislava, Slovakia +421 2 602 95 630
Hi Jaro,
Thanks for the wonderful photos. I was very happy to receive your e-mail, because I wanted to contact you last week and tell you what a nice talk you gave, but I couldn't locate your e-mail address. It was a real pleasure to meet you.
Best wishes, Jim
-----Original Message----- From: loops-bounces@solar.physics.montana.edu [mailto:loops- bounces@solar.physics.montana.edu] On Behalf Of Dudík Jaroslav Sent: Friday, July 10, 2009 6:24 AM To: loops@solar.physics.montana.edu Subject: [Loops] Photos - Loops Workshop IV & Florence
Hello everyone,
it was very nice to meet you all last week in Florence :) In case anyone is interested in some photos, here they are: http://picasaweb.google.com/jaroslav.dudik/Firenze2009# I hope I am not abusing the loops mailing list in this way. If yes, please ignore this message.
My best regards,
- Jaro
-- Jaroslav Dudik PhD. student, fourth year Division of Astronomy and Astrophysics Department of Astronomy, Physics of the Earth and Meteorology Faculty of Mathematics, Physics and Informatics Comenius University Mlynska Dolina F2-203 842 48 Bratislava, Slovakia +421 2 602 95 630 _______________________________________________ Loops mailing list Loops@solar.physics.montana.edu https://mithra.physics.montana.edu/mailman/listinfo/loops
Dear friends, please find at the following site:
http://arxiv.org/abs/0909.2529
the work "Comparison of Hinode/XRT and RHESSI detection of hot plasma in the non-flaring solar corona" by F. Reale http://arxiv.org/find/astro-ph/1/au:+Reale_F/0/1/0/all/0/1, J. M. McTiernan http://arxiv.org/find/astro-ph/1/au:+McTiernan_J/0/1/0/all/0/1, and P. Testa http://arxiv.org/find/astro-ph/1/au:+Testa_P/0/1/0/all/0/1 accepted for publication on ApJ Letters. The abstract is appended. Thank you for your attention Best regards Fabio Reale
Comparison of Hinode/XRT and RHESSI detection of hot plasma in the non-flaring solar corona
Authors: F. Reale http://arxiv.org/find/astro-ph/1/au:+Reale_F/0/1/0/all/0/1, J. M. McTiernan http://arxiv.org/find/astro-ph/1/au:+McTiernan_J/0/1/0/all/0/1, P. Testa http://arxiv.org/find/astro-ph/1/au:+Testa_P/0/1/0/all/0/1
Abstract: We compare observations of the non-flaring solar corona made simultaneously with Hinode/XRT and with RHESSI. The analyzed corona is dominated by a single active region on 12 November 2006. The comparison is made on emission measures. We derive emission measure distributions vs temperature of the entire active region from multifilter XRT data. We check the compatibility with the total emission measure values estimated from the flux measured with RHESSI if the emission come from isothermal plasma. We find that RHESSI and XRT data analyses consistently point to the presence of a minor emission measure component peaking at log T ~ 6.8-6.9. The discrepancy between XRT and RHESSI results is within a factor of a few and indicates an acceptable level of cross-consistency.
loops@solar.physics.montana.edu