MAX MILLENNIUM NEWS
29 May 2019
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
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> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Damping of Propagating Kink Waves in the Solar Corona
-- Ajay K. Tiwari, Richard J. Morton, Stephane Rggnier, and
James A. McLaughlin
Non-equilibrium ionization effects on solar EUV and X-ray imaging
observations
-- Jin-Yi Lee, John C. Raymond, Katharine K. Reeves, Chengcai Shen,
Yong-Jae Moon, and Yeon-Han Kim
Linear waves in a non-equilibrium ionisation partially ionised plasma
-- Istvan Ballai
How Many Twists Do Solar Coronal Jets Release?
-- Jiajia Liu, Yuming Wang, Robertus Erdélyi
Different Signatures of Chromospheric Evaporation in Two Solar Flares
Observed with IRIS
-- Y. Li, M. D. Ding, J. Hong, H. Li, W. Q. Gan
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 solar.physics.montana.edu
No. 351, “The Cosmic-Ray Shadow and Coronal Magnetism”, by Frederik Tenholt: Measuring the coronal magnetic field in Antarctica.
No. 350, “Kristian Birkeland”, by Hugh Hudson and Lyndsay Fletcher: Space weather a century ago.
See http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets .
We publish these at roughly two-week intervals and welcome contributions,
which should be related, at least loosely, to RHESSI science.
The effect of scattering on the apparent positions of solar radio
sources observed by LOFAR
by Mykola Gordovskyy
http://cesra.net/?p=2206
High‐Frequency Communications Response to Solar Activity in September
2017 as Observed by Amateur Radio Networks
by Nathan A. Frissell
http://cesra.net/?p=2198
----
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/http://twitter.com/CESRA_community
MAX MILLENNIUM NEWS
22 May 2019
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 Physical Nature of Spiral Wave Patterns in Sunspots
-- Juhyung Kang, Jongchul Chae, V. M. Nakariakov, Kyuhyoun Cho,
Hannah Kwak, Kyeore Lee
Predicting Solar Flares Using a Long Short-Term Memory Network
-- Hao Liu, Chang Liu, Jason T. L. Wang, 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
15 May 2019
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
Coronal loop transverse oscillations excited by different driver
frequencies
-- Andrey Afanasyev, Konstantinos Karampelas, Tom Van Doorsselaere
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
08 May 2019
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 Center-Limb Variation of the Strengths of Spectral Lines:
Classification and Interpretation of Observed Trends
-- Y. Takeda and S. UeNo
The plasmoid instability in a confined solar flare
-- David MacTaggart, Lyndsay Fletcher
High-frequency dynamics of active region moss as observed by IRIS
-- Nancy Narang, Vaibhav Pant, Dipankar Banerjee, Tom Van Doorsselaere
Extreme-ultraviolet Late Phase Caused by Magnetic Reconnection over
Quadrupolar Magnetic Configuration in a Solar Flare
-- Zhenjun Zhou, Xin Cheng, Lijuan Liu, Yu Dai, Yuming Wang, Jun Cui
Two-step evolution of a rising flux rope resulting in a confined
solar flare
-- Shuhong Yang, Jun Zhang, Qiao Song, Yi Bi, Ting Li
Why torus-unstable solar filaments experience failed eruption?
-- Zhenjun Zhou, Xin Cheng, Jie Zhang, Yuming Wang, Dong Wang,
Lijuan Liu, Bin Zhuang, Jun Cui
The Magnetic Properties of Heating Events on High-Temperature
Active Region Loops
-- Ignacio Ugarte-Urra, Nicholas A. Crump, Harry P. Warren,
Thomas Wiegelmann
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
01 May 2019
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
Pulse-beam heating of deep atmospheric layers, their oscillations and
shocks modulating the flare reconnection
-- P. Jelinek, M. Karlicky
A potential magnetic field calculator for solar physics applications
using staggered grids
-- Callum M. Boocock, David Tsiklauri
E and B polarizations from inhomogeneous and solar surface turbulence
-- Axel Brandenburg, Andrea Bracco, Tina Kahniashvili, Sayan Mandal,
Alberto Roper Pol, Gordon J. D. Petrie, Nishant K. Singh
Oscillations Accompanying a He I 10830 A Negative Flare in a Solar
Facula II. Response of the Transition Region and Corona
-- Nikolai Kobanov and Andrei Chelpanov
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