MAX MILLENNIUM NEWS
30 September 2015
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
Spectroscopic observations and modelling of impulsive Alfven
waves along a polar coronal jet
-- P. Jelinek, A. K. Srivastava, K. Murawski, P. Kayshap and
B. N. Dwivedi
A Circular-ribbon Solar Flare Following an Asymmetric Filament
Eruption
-- Chang Liu, Na Deng, Rui Liu, Jeongwoo Lee, Etienne Pariat,
Thomas Wiegelmann, Yang Liu, Lucia Kleint, Haimin Wang
Investigation of Umbral Dots with the New Vacuum Solar Telescope
-- Kaifan Ji, Xia Jiang, Song Feng, Yunfei Yang, Hui Deng, Feng Wang
Cut-off period for slow magnetoacoustic waves in coronal plasma
structures
-- A.N. Afanasyev, V. M. Nakariakov
Flare processes evolution and polarization changes of fine structures
of solar radio emission in the April 11, 2013 event
-- Gennady Chernov, Robert Sych, Baolin Tan, Yihua Yan, Chengming
Tan, Qijun Fu, Marian Karlicky and Valery Fomichev
Model of Local Oscillations in Sunspots
-- Yu. D. Zhugzhda and R.A.Sych
Sunspot waves and flare energy release
-- R. Sych, M. Karlicky, A. Altyntsev, J. Dudik and L. Kashapova
MHD waves in sunspots
-- Robert Sych
Magnetic Reconnection Rates and Energy Release in a Confined X-class
Flare
-- Astrid M. Veronig, Wolfgang Polanec
Flare processes evolution and polarization changes of fine structures
of solar radio emission in the April 11, 2013 event
-- Gennady Chernov, Robert Sych, Baolin Tan, Yihua Yan, Chengming
Tan, Qijun Fu, Marian Karlicky and Valery Fomichev
2. FROM THE EDITOR
==================
The Max Millennium program exists to enhance all aspects of solar
activity 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
MAX MILLENNIUM NEWS
23 September 2015
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
Benchmark Test of Differential Emission Measure Codes and
Multi-Thermal Energies in Solar Active Regions
-- Aschwanden,M.J., Boerner,P., Caspi,A., McTiernan,J.M., Ryan,D.,
and Warren,H.P.
Multiwavelength Observations of a Slow Raise, Multi-Step X1.6 Flare
and the Associated Eruption
-- Yurchyshyn, V., Kumar, P., Cho, K.S., Lim, E.K., & Abramenko, V.
Active region upflows: 1. Multi-instrument observations
-- K. Vanninathan, M.S. Madjarska, K. Galsgaard, Z.Huang, J.G. Doyle
Active region upflows: 2. Data driven MHD modeling
-- K. Galsgaard, M. S. Madjarska, K. Vanninathan, Z. Huang, M. Presmann
A Statistical Study of Distant Consequences of Large Solar Energetic
Events
-- C.J. Schrijver, P.A. Higgins
Coronal response to an EUV wave from DEM analysis
-- K. Vanninathan, A.M. Veronig, K. Dissauer, M.S. Madjarska,
I.G. Hannah, E.P. Kontar
2. FROM THE EDITOR
==================
The Max Millennium program exists to enhance all aspects of solar
activity 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
No. 262, "Fine Structure in Flare Soft X-ray Light Curves," by Brian Dennis and Kim Tolbert: A tool that we’ve had since 1976 now gives us surprisingly precise new information.
No. 261, "Photospheric Electric Fields and Energy Fluxes in the Eruptive Active Region NOAA 11158,” by Maria Kazachenko. Flares need magnetic energy; we can now measure its arrival as Poynting flux across the solar photosphere.
No. 260, “RHESSI and General Relativity,” by Bill Thompson and Hugh Hudson. General-relativistic corrections to RHESSI source positions.
See
http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets
listing the current series, 2008-present, and
http://sprg.ssl.berkeley.edu/~tohban/nuggets/
for the original series, 2005-2008.
We publish these at roughly two-week intervals and welcome contributions,
which should be related, at least loosely, to RHESSI science.
MAX MILLENNIUM NEWS
16 September 2015
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
Why does the apparent mass of a coronal mass ejection increase?
-- Feng, Li; Wang, Yuming; Shen, Fang; Shen, Chenglong; Inhester,
Bernd; Lu, Lei; Gan, Weiqun
Radial Flow Pattern of a Slow Coronal Mass Ejection
-- Feng, Li; Inhester, Bernd; Gan, Weiqun
Heating and cooling of coronal loops observed by SDO
-- Li, L. P., Peter, H., Chen, F., and Zhang, J.
APPEARANCES AND STATISTICS OF CORONAL CAVITIES DURING THE ASCENDING
PHASE OF SOLAR CYCLE 24
-- N. Karna, W. D. Pesnell, and J. Zhang
STUDY OF THE 3D GEOMETRIC STRUCTURE AND TEMPERATURE OF A CORONAL
CAVITY USING THE LIMB SYNOPTIC MAP METHOD
-- N. Karna, J. Zhang, W. Dean Pesnell, and S. A. Hess Webber
Application of Kernel Based Machine Learning to Inversion Problem
of Photospheric Magnetic Fields
-- Fei Teng
Hard X-Ray Imaging of Individual Spectral Components in Solar Flares
-- Amir Caspi, Albert Y. Shih, James M. McTiernan, Sam Krucker
2. FROM THE EDITOR
==================
The Max Millennium program exists to enhance all aspects of solar
activity 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
MAX MILLENNIUM NEWS
09 September 2015
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
Model comparison for the density structure across solar coronal
waveguides
-- I. Arregui, R. Soler, A. Asensio Ramos
Evidence of thermal conduction suppression in a solar flaring loop
by coronal seismology of slow-mode waves
-- Tongjiang Wang, Leon Ofman, Xudong Sun, Elena Provornikova,
Joseph M. Davila
The Role of Erupting Sigmoid in Triggering a Flare with Parallel
and Large-Scale Quasi-Circular Ribbons
-- Navin Chandra Joshi, Chang Liu, Xudong Sun, Haimin Wang, Tetsuya
Magara, Y.-J. Moon
Damped transverse oscillations of interacting coronal loops
-- Roberto Soler and Manuel Luna
2. FROM THE EDITOR
==================
The Max Millennium program exists to enhance all aspects of solar
activity 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
MAX MILLENNIUM NEWS
02 September 2015
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
High-resolution Observations of a Flux Rope with the Interface
Region Imaging Spectrograph
-- Ting Li, Jun Zhang
Spectroscopic Signatures Related to a Sunquake
-- Sarah A. Matthews, Louise K. harra, Sergei Zharkov &
Lucie M. Green
Magnetic Flux and Helicity of Magnetic Clouds
-- Demoulin P., Janvier M., Dasso S.
Depth-dependent global properties of a sunspot observed by Hinode
(SOT/SP)
-- Tiwari, Sanjiv K.; van Noort, Michiel; Solanki, Sami K.;
Lagg, Andreas
2. FROM THE EDITOR
==================
The Max Millennium program exists to enhance all aspects of solar
activity 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