Dear Colleague,
since the release of CHIANTI Version 7.0, we realized that 4 files
were included in the database that should not have been there. As
a consequence, they caused several routines to crash both in the
stand-alone version and in the SolarSoft distribution.
We removed those files and now the software is working.
If you use CHIANTI through SolarSoft that is automatically mirrored,
the update will occur automatically within the next few days. For a faster
solution, you can manually fix your the SolarSoft directories by removing
the following files:
(chianti top directory)/h/h_1/h_1.reclvl
(chianti top directory)/he/he_1/he_1.reclvl
(chianti top directory)/cl/cl_16/cl_16.reclvl
(chianti top directory)/k/k_18/k_18.reclvl
If you use CHIANTI through the stand-alone tar file, we recommend that
you download and install the new tar file in your CHIANTI directories.
The new tar file can be found at our web site location:
http://www.chiantidatabase.org/
We apologize for any inconvenience this has caused you.
Best regards,
The CHIANTI Team
17. Transverse coronal loop oscillations seen by AIA/SDO
by Rebecca White and Erwin Verwichte, University of Warwick
Probing the coronal plasma with the diagnostic power of kink waves.
http://www.uksolphys.org/?p=3398
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
UKSP Nuggets are published on a monthly basis highlighting solar physics
research in the UK.
http://www.uksolphys.org/uksp-nuggets
Iain Hannah and Lyndsay Fletcher
--
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
Dr. Iain G. Hannah Eml: iain.hannah(a)glasgow.ac.uk
Astronomy & Astrophysics Group, Tel: +44 (0)141 330 6427
School of Physics & Astronomy, Fax: +44 (0)141 330 5183
Kelvin Building,
University of Glasgow,
Glasgow, Scotland, UK
G12 8QQ Web: http://www.astro.gla.ac.uk/~iain/
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
MAX MILLENNIUM NEWS
09 November 2011
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
-----------------------------------
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Constraining the Kinematics of Coronal Mass Ejections in the Inner
Heliosphere with In-Situ Signatures -- T. Rollett, C. M?stl,
M. Temmer, A.M. Veronig, C.J. Farrugia, H.K. Biernat
SDO/AIA Observations of Secondary Waves Generated by Interaction
of the 2011 June 7 Global EUV Wave With Solar Coronal Structures --
Ting Li, Jun Zhang, Shuhong Yang, Wei Liu
What is the true nature of blinkers? -- S. Subramanian,
M. S. Madjarska, J. G. Doyle and D. Bewsher
Thermal Properties of A Solar Coronal Cavity Observed with the X-ray
Telescope on Hinode -- Reeves, K. K., Gibson, S. E., Kucera, T. A.,
Hudson, H. S. and Kano, R.
Frequency drifts of 3-min oscillations in microwave and EUV emission
above sunspots -- R. Sych, T. V. Zaqarashvili, V. M. Nakariakov,
S.A. Anfinogentov, K.Shibasaki and Y. Yan
2. FROM THE EDITOR
------------------
The Max Millennium program exists to enhance all aspects of solar
flare research. If you have news that is of broad interest to that
community, feel free to send your message to the MMScience e-mail
list:
http://solar.physics.montana.edu/max_millennium/mmlists.shtml
Address questions to canfield at physics.montana.edu
Dear Colleague,
We would like to announce the release of version 7.0 of the CHIANTI
database for astrophysical spectroscopy. With Version 7.0, CHIANTI
now includes data for several new ions as well as significant updates to
many ions, including several key Fe species routinely observed by
Hinode/EIS and SDO. Also, a completely new implementation of the
CHIANTI software in the Python programming language has been
developed and is freely available on the web (ChiantiPy). IDL
software updates have been performed to ensure compatibility
with IDL 8.
If you use CHIANTI through SolarSoft that is automatically mirrored,
the update will occur automatically within the next few days. Otherwise,
you will need to manually update your the SolarSoft directories.
If you use CHIANTI through the stand-alone tar file, we recommend that
you download and install the new tar file in your CHIANTI directories.
The new tar file can be found at our new web site location:
http://www.chiantidatabase.org/ - note the new url!
The ChiantiPy software suite can be found at
http://sourceforge.net/projects/chiantipy/
If you have any questions, problems, suggestions regarding CHIANTI,
we are always glad to hear from you by sending email to
chianti_help(a)halcyon.nrl.navy.mil
Best regards,
The CHIANTI Team
MAX MILLENNIUM NEWS
02 November 2011
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
-----------------------------------
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Energy Release and Particle Acceleration in Flares: Summary and
Future Prospects -- R.P. Lin
Deducing Electron Properties From Hard X-Ray Observations --
E.P. Kontar, J.C. Brown, A.G. Emslie, W. Hajdas, G.D. Holman,
G. J. Hurford, J. Kasparova, P. C. V. Mallik, A. M. Massone,
M. L. McConnell, M. Piana, M. Prato, E. J. Schmahl, E. Suarez-Garcia
Recent Advances in Understanding Particle Acceleration Processes in
Solar Flares -- Valentina V. Zharkova, Karpar Arzner, Arnold O. Benz,
Philippa Browning, Cyril Dauphin, A. Gordon Emslie, Lyndsay Fletcher,
Eduard P. Kontar, Gottfried Mann, Marco Onofri, Vahe Petrosian,
Rim Turkmani, Nicole Vilmer, Loukas Vlahos
Microflares and the Statistics of X-ray Flares -- I. G. Hannah,
H. S. Hudson, M. Battaglia, S. Christe, J. Kasparova, S. Krucker,
M. R. Kundu, A. Veronig
The Relationship Between Solar Radio and Hard X-ray Emission --
Stephen M. White, Arnold O. Benz, Steven Christe, Frantisek Farnik,
Mukul R. Kundu, Gottfried Mann, Zongjun Ning, Jean-Pierre Raulin,
Adriana V. R. Silva-Valio, Pascal Saint-Hilaire, Nicole Vilmer,
Alexander Warmuth
Properties of Energetic Ions in the Solar Atmosphere from γ-Ray
and Neutron Observations -- Nicole Vilmer, Alec L. MacKinnon,
Gordon J. Hurford
Implications of X-ray Observations for Electron Acceleration and
Propagation in Solar Flares -- Gordon D. Holman, Markus
J. Aschwanden, Henry Aurass, Marina Battaglia, Paolo C. Grigis,
Eduard P. Kontar, Wei Liu, Pascal Saint-Hilaire, Valentina
V. Zharkova
An Observational Overview of Solar Flares -- Lyndsay Fletcher,
Brian R. Dennis, Hugh S. Hudson, Sam Krucker, Ken Phillips, Astrid
Veronig, Marina Battaglia, Laura Bone, Amir Caspi, Qingrong Chen,
Peter Gallagher, Paolo C. Grigis, Haisheng Ji, Ryan O. Milligan,
Manuela Temmer
High-Energy Aspects of Solar Flares: Overview of the Volume --
Brian R. Dennis, A. Gordon Emslie, Hugh S. Hudson
Transverse coronal loop oscillations seen in unprecedented detail
by AIA/SDO -- R.S. White, E. Verwichte
Spatially resolved hard X-ray polarization in solar flares: effects
of Compton scattering and bremsstrahlung -- Jeffrey, N. L. S.,
Kontar, E. P.
2. FROM THE EDITOR
------------------
The Max Millennium program exists to enhance all aspects of solar
flare research. If you have news that is of broad interest to that
community, feel free to send your message to the MMScience e-mail
list:
http://solar.physics.montana.edu/max_millennium/mmlists.shtml
Address questions to canfield at physics.montana.edu
Dear all,
Announcing a new EIS Nugget:
"Sunspot light-bridges - a bridge from the photosphere to the
corona?" by Sarah Matthews (MSSL-UCL).
Please visit it via URL address - http://msslxr.mssl.ucl.ac.uk:8080/
SolarB/nuggets/nugget_2011nov.jsp
We publish these at roughly one month intervals.
Best wishes,
Lucie
Dr Lucie Green
Mullard Space Science Laboratory
Holmbury St. Mary
Dorking
Surrey
RH5 6NT
+44 (0)1483 204103
www.mssl.ucl.ac.uk
MAX MILLENNIUM NEWS
26 October 2011
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
-----------------------------------
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Solar Stereoscopy with STEREO/EUVI A and B spacecraft from small
(6 deg) to large (170 deg) spacecraft separation angles -- Markus
J. Aschwanden, Jean-Pierre Wuelser, Nariaki Nitta, James Lemen
First 3D Reconstructions of Coronal Loops with the STEREO A+B
Spacecraft: IV. Magnetic Field Modeling with Uniformly Twisted Flux
Tubes -- Markus J. Aschwanden, Jean-Pierre Wuelser, Nariaki V. Nitta,
James R. Lemen, Marc L. DeRosa, and Anna Malanushenko
Interplanetary magnetic structure guiding relativistic particles --
Masson S., Demoulin P., Dasso S., and Klein K.-L.
RADIATIVE HYDRODYNAMIC SIMULATION OF THE CONTINUUM EMISSION IN
SOLAR WHITE-LIGHT -- J. X. Cheng, M. D. Ding, and Mats Carlsson
High time resolution observations of solar H-alpha flares - II
Search for signatures of electron beam heating -- K. Radziszewski,
P. Rudawy, and K. J. H. Phillips
HARD X-RAY AND ULTRAVIOLET OBSERVATIONS OF THE 2005 JANUARY 15
TWO-RIBBON FLARE -- J. X. Cheng, G. Kerr, and J. Qiu
2. FROM THE EDITOR
------------------
The Max Millennium program exists to enhance all aspects of solar
flare research. If you have news that is of broad interest to that
community, feel free to send your message to the MMScience e-mail
list:
http://solar.physics.montana.edu/max_millennium/mmlists.shtml
Address questions to canfield at physics.montana.edu