MAX MILLENNIUM NEWS
28 June 2017
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
Beam electrons as a source of H-alpha flare ribbons
-- Malcolm Druett, Eamon Scullion, Valentina Zharkova,
Sarah Matthews, Sergei Zharkov & Luc Rouppe Van der Voort
A hybrid supervised/unsupervised machine learning approach to solar
flare prediction
-- Federico Benvenuto, Michele Piana, Cristina Campi,
Anna Maria Massone
Magnetohydrodynamic Simulations for Studying Solar Flare Trigger
Mechanism
-- Johan Muhamad, Kanya Kusano, Satoshi Inoue, Daikou Shiota
Sunspot Light Walls Suppressed by Nearby Brightenings
-- Shuhong Yang, Jun Zhang, Robertus Erdelyi, Yijun Hou,
Xiaohong Li, Limei Yan
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 richard.canfield at montana.edu
MAX MILLENNIUM NEWS
21 June 2017
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
Double arc instability in the solar corona
-- N. Ishiguro, K. Kusano
Variation of Coronal Activity from the Minimum to Maximum of
Solar Cycle 24 using Three Dimensional Coronal Electron Density
Reconstructions from STEREO/COR1
-- Tongjiang Wang, Nelson L. Reginald, Joseph M. Davila,
O. Chris St. Cyr, William T. Thompson
Electron plasma wake field acceleration in solar coronal and
chromospheric plasmas
-- David Tsiklauri
Non-Maxwellian analysis of the transition-region line profiles
observed by the Interface Region Imaging Spectrograph
-- J. Dudik, V. Polito, E. Dzifcakova, G. Del Zanna, and P. Testa
Non-Equilibrium Processes in the Solar Corona, Transition Region,
Flares, and Solar Wind (Invited Review)
-- J. Dudik, E. Dzifcakova, N. Meyer-Vernet, G. Del Zanna,
P. R. Young, A. Giunta, B. Sylwester, J. Sylwester, M. Oka,
H. E. Mason, C. Vocks, L. Matteini, S. Krucker, D. R. Williams,
S. Mackovjak
Expanding and Contracting Coronal Loops as Evidence of Vortex
Flows Induced by Solar Eruptions
-- J. Dudik, F. P. Zuccarello, G. Aulanier, B. Schmieder,
P. Demoulin
Testing predictors of eruptivity using parametric flux emergence
simulations
-- Chloe Guennou, Etienne Pariat, Nicole Vilmer and James E. Leake
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 richard.canfield at montana.edu
MAX MILLENNIUM NEWS
14 June 2017
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
Investigation of Relationship Between High-Energy X-ray Sources
and Photospheric and Helioseismic Impacts of X1.8 Solar Flare of
October 23, 2012
-- Ivan N Sharykin, Alexander G Kosovichev, Viacheslav M Sadykov,
Ivan V Zimovets, Ivan I Myshyakov
Small electron acceleration episodes in the solar corona
-- Tomin James, Prasad Subramanian, Eduard P Kontar
Detection and Interpretation Of Long-Lived X-Ray Quasi-Periodic
Pulsations in the X-Class Solar Flare on 2013 May 14
-- Brian R. Dennis, Anne K. Tolbert, Andrew Inglis, Jack Ireland,
Tongjiang Wang, Gordon D. Holman, Laura A. Hayes,
Peter T. Gallagher
Witnessing a Large-scale Slipping Magnetic Reconnection along a
Dimming Channel during a Solar Flare
-- Ju Jing, Rui Liu, Mark C. M. Cheung, Jeongwoo Lee, Yan Xu,
Chang Liu, Chunming Zhu, Haimin Wang
Investigation of Relationship Between High-Energy X-ray Sources
and Photospheric and Helioseismic Impacts of X1.8 Solar Flare of
October 23, 2012
-- Ivan N Sharykin, Alexander G Kosovichev, Viacheslav M Sadykov,
Ivan V Zimovets, Ivan I Myshyakov
Non-potential field formation in the X-shaped quadrupole magnetic
field configuration
-- Kawabata, Yusuke; Inoue, Satoshi; Shimizu, Toshifumi
Predicting Solar Flares Using SDO/HMI Vector Magnetic Data Product
and Random Forest Algorithm
-- Chang Liu, Na Deng, Jason T. L. Wang, Haimin Wang
Coronal rain in magnetic bipolar weak fields
-- Chun Xia, Rony Keppens, and Xia Fang
Dong Li Quasi-periodic pulsations with multiple periods in hard
X-ray emission
-- Li, Dong; Zhang, Qingmin
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 richard.canfield at montana.edu
“The Solar X-ray Limb III”, by Marina Battaglia and Gordon Hurford. RHESSI succeeds with an entirely new way to measure the solar diameter.
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
07 June 2017
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
Exploring the potential of microwave diagnostics in SEP forecasting:
The occurrence of SEP events
-- Pietro Zucca, Marlon Nunez, and Karl-Ludwig Klein
The Solar X-ray Limb
-- M. Battaglia, H. S. Hudson, G. J. Hurford, S. Krucker,
R. A. Schwartz
HIGH-RESOLUTION OBSERVATIONS OF DOWNFLOWS AT ONE END OF A
PRE-ERUPTION FILAMENT
-- Qin Li, Na Deng, Ju Jing, Haimin Wang
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 richard.canfield at montana.edu
MAX MILLENNIUM NEWS
31 May 2017
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
Estimating Solar Flux Density at Low Radio Frequencies Using a Sky
Brightness Model
-- Divya Oberoi, Rohit Sharma and Alan E.E. Rogers
Center-to-limb observations of the Sun with ALMA
-- C. E. Alissandrakis, S. Patsourakos, A. Nindos, T. S. Bastian
Increase in the amplitude of line-of-sight velocities of the
small-scale motions in a solar filament before eruption
-- Daikichi Seki, Kenichi Otsuji, Hiroaki Isobe, Takako T. Ishii,
Takahito Sakaue, Kumi Hirose
Observing the Sun with the Atacama Large Millimeter-submillimeter
Array (ALMA): Fast-Scan Single-Dish Mapping
-- S.M. White, K. Iwai, N.M. Phillips, R.E. Hills, A. Hirota,
P. Yagoubov, G. Siringo, M. Shimojo, T.S. Bastian, A.S. Hales,
T. Sawada, S. Asayama, M. Sugimoto, R.G. Marson, W. Kawasaki,
E. Muller, T. Nakazato, K. Sugimoto, R. Brajsa, I. Skokic,
M. Barta, S. Kim, A.J. Remijan, I. de Gregorio, S.A. Corder,
H.S. Hudson, M. Loukitcheva, B. Chen, B. De Pontieu,
G.D. Fleishmann, D.E. Gary, A. Kobelski, S. Wedemeyer, Y. Yan
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 richard.canfield at montana.edu