MAX MILLENNIUM NEWS
28 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
Si IV Resonance Line Emission During Solar Flares: Non-LTE,
Non-equilibrium, Radiation Transfer Simulations
-- Graham S. Kerr, Mats Carlsson, Joel C. Allred, Peter R. Young,
and Adrian N. Daw
Study of current sheets in the wake of two crossing filaments
eruption
-- Dai, J., Yang, J. Y., Li, L. P., Zhang, J.
Quasi-periodic fast propagating magnetoacoustic waves during the
magnetic reconnection between solar coronal loops
-- Li, L. P., Zhang, J., Peter, H., Chitta, L. P., Su, J. T.,
Song, H. Q., Xia, C., Hou, Y. J.
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. 336, “Remembering Marcos Machado via his research”, by Hugh Hudson: Recalling a friend and colleague, and admiring his final paper,
No. 337 “Cycle 25 Strikes Again”, by Kamil Bicz: A second, larger, Cycle 25 sunspot.
No. 338 “Neutron Production in Solar Flares”, by Ron Murphy and Gerry Share: Neutron astronomy helps us understand solar flares.
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
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