MAX MILLENNIUM NEWS
21 November 2018
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 EUV observations of impulsive solar energetic particle
event sources
-- R. Bucik, A. Fludra, R. Gómez-Herrero D. E. Innes, B. Kellett,
R. Kumar, S. Mackovjak
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
Non-radial propagation of energetic electrons in solar corona
by A. Klassen et al.
http://cesra.net/?p=1992
Shock location and CME 3-D reconstruction of a solar type II radio burst
with LOFAR
by P. Zucca et al.*
http://cesra.net/?p=2005
Coronal Densities Probed by Type III Radio Burst Imaging
by P. McCauley et al.*
http://cesra.net/?p=2032
---
CESRA Highlights of Solar Radio Physics, aka CESRA Nuggets, are short
communications written in language accessible to a non-expert in the
specific area and designed to keep solar and heliophysics communities
informed and up-to-date about current research. The highlights can be
followed, discussed, commented and shared via
http://www.facebook.com/solarcesra/ and http://twitter.com/CESRA_community
MAX MILLENNIUM NEWS
14 November 2018
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
CME-driven shock and Type II solar radio burst band-splitting
-- Chrysaphi, N., Kontar E. P., Holman, G. D., and Temmer, M.
Signatures of magnetic reconnection at the footpoints of fan shape
jets on a light bridge driven by photospheric convective motions
-- Xianyong Bai, Hector Socas-Navarro, Daniel Nobrega-Siverio,
Jiangtao Su, Yuanyong Deng, Dong Li, Wenda Cao, Kaifan Ji
Drifting of the line-tied footpoints of CME flux-ropes
-- G. Aulanier, J. Dudik
Three-dimensional Magnetic Reconnection Triggering an X-class
Confined Flare in Active Region 12192
-- Ting Li, Yijun Hou, Shuhong Yang & Jun Zhang
Oscillations accompanying a He I 10830 A negative flare in a solar
facula
-- Andrei Chelpanov, Nikolai Kobanov
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
07 November 2018
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
The Origin of Major Solar Activity - Collisional Shearing Between
Nonconjugated Polarities of Multiple Bipoles Emerging Within Active
Regions
-- Georgios Chintzoglou, Jie Zhang, Mark C. M. Cheung, Maria Kazachenko
Probing the Puzzle of Behind-the-limb γ-Ray Flares: Data-driven
Simulations of Magnetic Connectivity and CME-driven Shock Evolution
-- Meng Jin, Vahé Petrosian, Wei Liu, Nariaki V. Nitta, Nicola
Omodei, Fatima Rubio da Costa, Frederic Effenberger, Gang Li,
Melissa Pesce-Rollins, Alice Allafort, and Ward Manchester IV
Transition-region explosive events produced by plasmoid instability
-- Dong Li
Flare Productivity of Major Flaring Solar Active Regions:
A Time-series Study of Photospheric Magnetic Properties
-- Eo-Jin Lee, Sung-Hong Park, Yong-Jae Moon
Physical processes involved in the EUV "Surge" Event of 09
May 2012
-- Marcelo Lopez-Fuentes, Cristina H. Mandrini, Mariano Poisson, Pascal
Demoulin, German Cristiani, Fernando M. Lopez, Maria Luisa Luoni
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 October 2018
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
Formation and Eruption of an Active Region Sigmoid.
II. Magnetohydrodynamic Simulation of a Multistage Eruption
-- Chaowei Jiang, Xueshang Feng, and Qiang Hu
Evolution of Photospheric Vector Magnetic Field Associated with
Moving Flare Ribbons As Seen By GST
-- Chang Liu, Wenda Cao, Jongchul Chae, Kwangsu Ahn, Debi Prasad
Choudhary, Jeongwoo Lee, Rui Liu, Na Deng, Jiasheng Wang, Haimin Wang
On the Extrapolation of Magnetohydrostatic Equilibria on the Sun
-- Xiaoshuai Zhu, Thomas Wiegelmann
Lyman Continuum Observations of Solar Flares Using SDO/EVE
-- Marcos E. Machado, Ryan O. Milligan, Paulo J. A. Simoes
Buoyancy-driven Magnetohydrodynamic Waves in a Partially Ionized
Plasma
-- A. Hague, R. Erdelyi
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
24 October 2018
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
Genesis and impulsive evolution of the 2017 September 10 coronal mass
ejection
-- Astrid M. Veronig, Tatiana Podladchikova, Karin Dissauer, Manuela
Temmer, Daniel B. Seaton, David Long, Jingnan Guo, Bojan Vrsnak,
Louise Harra, Bernhard Kliem
First Detection of Solar Flare Emission in Middle-Ultraviolet
Balmer Continuum
-- Marie Dominique, Andrei N. Zhukov, Petr Heinzel, Ingolf
E. Dammasch, Laurence Wauters, Laurent Dolla, Sergei Shestov,
Matthieu Kretzschmar, Janet Machol, Giovanni Lapenta, Werner Schmutz
First high-resolution look at the quiet Sun with ALMA at 3 mm
-- A. Nindos, C.E. Alissandrakis, T.S. Bastian, S. Patsourakos, B. De
Pontieu, H. Warren, T. Ayres, H.S. Hudson, T. Shimizu, J.-C. Vial,
S. Wedemeyer, V. Yurchyshyn
Dispersive shock waves in partially ionised plasmas
-- I. Ballai, E. Forgacs-Dajka, A. Marcu
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
No. 335, “CORONAS/SPIRIT Mg XII and nanoflares”, by Anton Reva. Monochromatic Mg XII spectroheliography sets severe limits on nanoflare heating models.
No. 334, “White-light Emission and Non-thermal Electrons”, by Kyoung-Sun LEE. An intimiate relationship between accelerated electrons and visible flare continuum.
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.
Announcing CESRA nuggets in September:
Size distributions of solar proton events and their asso-ciated soft
X-ray flares based on the maximum likelihood estimator
by E.W. Cliver and E. D’Huys
http://cesra.net/?p=1971
Decimetric emission 500 arcseconds away from a flaring site: Possible
scenarios from GMRT solar radio observations
by Bisoi et al.*
http://cesra.net/?p=1960
---
CESRA Highlights of Solar Radio Physics, aka CESRA Nuggets, are short
communications written in language accessible to a non-expert in the
specific area and designed to keep solar and heliophysics communities
informed and up-to-date about current research. The highlights can be
followed, discussed, commented and shared via
http://www.facebook.com/solarcesra/ and http://twitter.com/CESRA_community
MAX MILLENNIUM NEWS
10 October 2018
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
Particle acceleration in coalescent and squashed magnetic islands
I. Test particle approach
-- Q.Xia and V. Zharkova
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
MAX MILLENNIUM NEWS
3 October 2018
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
Statistical Analysis of Torus and Kink Instabilities in Solar Eruptions
-- Ju Jing, Chang Liu, Jeongwoo Lee, Hantao Ji, Nian Liu, Yan Xu, and
Haimin Wang
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