MAX MILLENNIUM NEWS
26 May 2021
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
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1. E-PRINTS POSTED IN THE PAST WEEK
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> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
FOXSI-2 Solar Microflares. II.
Hard X-ray Imaging Spectroscopy and Flare Energetics
-- Juliana T. Vievering, Lindsay Glesener, P. S. Athiray,
Juan Camilo Buitrago-Casas, Sophie Musset, Daniel F. Ryan,
Shin-nosuke Ishikawa, Jessie Duncan, Steven Christe, and Sam Krucker
Structure and Evolution of an Inter–Active Region Large-scale Magnetic Flux Rope
-- Aiying Duan, Chaowei Jiang, Peng Zou, Xueshang Feng, and Jun Cui
Variation of Magnetic Flux Ropes through Major Solar Flares
-- Aiying Duan, Chaowei Jiang, Zhenjun Zhou, Xueshang Feng, and Jun Cui
MHD Modeling of Solar Coronal Magnetic Evolution Driven by Photospheric Flow
-- Chaowei Jiang, Xinkai Bian, Tingting Sun, Xueshang Feng
The Causes of Peripheral Coronal Loop Contraction and Disappearance
Revealed in a Magnetohydrodynamic Simulation of Solar Eruption
-- Juntao Wang, Chaowei Jiang, Ding Yuan, and Peng Zou
The Sun's Dynamic Extended Corona Observed in Extreme Ultraviolet
-- Daniel B. Seaton, J. Marcus Hughes, Sivakumara K. Tadikonda, Amir Caspi,
Craig DeForest, Alexander Krimchansky, Neal E. Hurlburt, Ralph Seguin,
Gregory Slater
Magnetohydrodynamic Simulations of Spicular Jet Propagation Applied to
Lower Solar Atmosphere Model
-- Fionnlagh Mackenzie Dover, Rahul Sharma and Robertus Erdelyi
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 keiji.yoshimura at montana.edu
Parametric simulation studies on the wave propagation of solar radio
emission: the source size, duration, and position
by Zhang et al.*
http://www.astro.gla.ac.uk/users/eduard/cesra/?p=2860
Harmonic Electron Cyclotron Maser Emission Excited by Energetic
Electrons Traveling inside a Coronal Loop
by M. Yousefzadeh et al.*
http://www.astro.gla.ac.uk/users/eduard/cesra/?p=2856
---
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
19 May 2021
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
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1. E-PRINTS POSTED IN THE PAST WEEK
-----------------------------------
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Thermal Trigger for Solar Flares II: Effect of the Guide Magnetic Field
-- Leonid Ledentsov
The role of non-axisymmetry of magnetic flux rope in constraining solar eruptions
-- Ze Zhong, Yang Guo, M. D. Ding
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 keiji.yoshimura at montana.edu
MAX MILLENNIUM NEWS
5 May 2021
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
Energy budget of plasma motions, heating, and electron acceleration
in a three-loop solar flare
-- Gregory D. Fleishman, Lucia Kleint, Galina G. Motorina, Gelu M. Nita,
Eduard P. Kontar
Space weather: the solar perspective - an update to Schwenn (2006)
-- M. Temmer
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 keiji.yoshimura at montana.edu
The deadline for registration and abstract submission to the May 24-26, 2021, meeting on Solar Flare Energy Release has been extended to May 12. The link for abstract submission can be found either on the conference website (https://agenda.infn.it/event/26094/overview) or the SolFER website (solfer.umd.edu). Abstracts from early career scientists and students are especially welcome.
The SolFER DRIVE Science Center is announcing a web-based science meeting on Solar Flare Energy Release to take place on May 24-26, 2021. The meeting is open to all scientists working on the topic. The meeting will include invited talks, submitted oral talks as well as poster presentations and will provide substantial time for informal scientific discussion. We encourage paper submissions that are based on remote and in situ observational data as well as those based on theory and modeling. Extensive use will be made of Gather meeting software to facilitate interactive poster sessions as well as informal discussion between meeting participants. The meeting will be organized around the key scientific topics listed as follows:
* What mechanisms facilitate the fast release of magnetic energy in impulsive solar flares?
* What controls the onset of fast flare energy release?
* Why and how do flares transfer a large fraction of the released magnetic energy into energetic electrons?
* What mechanism drives the energization of ions and the measured abundance enhancements of some species during impulsive flares?
* What mechanisms control energetic particle transport in flares?
* How does reconnection heat plasma in flares and the small events (nanoflares) that may be responsible for heating the corona?
More information on these scientific topics can be found on the SolFER website (solfer.umd.edu). The list of confirmed invited speakers for the meeting is below:
* Jiong Qiu (Montana State University)
* Mark Linton (Naval Research Laboratory)
* Lyndsay Fletcher (University of Glasgow)
* Harry Arnold (University of Maryland)
* Marina Battaglia (FHNW)
* Qile Zhang (Los Alamos National Laboratory)
* George Ho (Johns Hopkins University)
* Loukas Vlahos (Aristotle University of Thessaloniki)
* Natasha Jeffrey (Northumbria University)
* Dana Longcope (Montana State University)
* Li-Jen Chen (NASA/GSFC)
* Mike Shay (University of Delaware)
MAX MILLENNIUM NEWS
28 April 2021
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
Mixed properties of slow magnetoacoustic and entropy waves in a plasma
with heating/cooling misbalance
-- D.I. Zavershinskii, D.Y. Kolotkov, D.S. Riashchikov, N.E. Molevich
The morphology of average solar flare time profiles from observations
of the Sun's lower atmosphere
-- Larisa K. Kashapova, Anne-Marie Broomhall, Alena I. Larionova,
Elena G. Kupriyanova, Ilya D. Motyk
Indications of stellar coronal mass ejections through coronal dimmings
-- Astrid M. Veronig, Petra Odert, Martin Leitzinger, Karin Dissauer,
Nikolaus C. Fleck, Hugh S. Hudson
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 keiji.yoshimura at montana.edu
http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets
No. 406 “Negative He 10830 Flare Ribbons and Non-thermal Electrons,” by Graham Kerr: A 1D radiation hydrodynamics model can explain the dark leading edges of He I flare ribbons.
No. 407 “Subsecond Spikes in Solar Flare X-ray Flux as seen by Fermi/GBM,” by Trevor Knuth and Lindsay Glesener: A new analysis technique pushes hard X-ray time scales to 0.1 s or faster.
No. 408 “Effects of Flares on Solar p-modes,” by Maria-Cristina Rabello Soares and Frederic Baudin: No detectable p-mode amplitude changes due to solar flares.
We welcome contributions to the RHESSI Nuggets, and the topics may wander some distance away from specifically RHESSI results if they are generally interesting. See http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggetsf… these and others. Comments about specific flares can often be found by searching for their SOLyyyy-mm-dd identifier from this home page.
The SolFER DRIVE Science Center will hold a web-based science meeting on Solar Flare Energy Release on May 24-26, 2021. The meeting is open to all scientists working on this topic. The meeting will include invited talks, submitted oral talks as well as poster presentations, and will provide substantial time for informal scientific discussion. We encourage paper submissions that are based on remote and in situ observational data as well as those based on theory and modeling. Registration to participate in the workshop is free.
To view the details of the meeting, and to submit an abstract, please visit the meeting website at https://agenda.infn.it/event/26094/overview
The abstract is due on 3 May, 2021, 23:59.
We look forward to your participation.
SOC of SolFER Spring Meeting
MAX MILLENNIUM NEWS
21 April 2021
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
Could switchbacks originate in the lower solar atmosphere?
II. Propagation of switchbacks in the solar corona
-- Magyar, Norbert; Utz, Dominik; Erdelyi, Robertus; Nakariakov, Valery M.
Solar large-scale magnetic field and cycle patterns in solar dynamo
-- V.N. Obridko, V.V. Pipin, D.D. Sokoloff, A.S. Shibalova
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 keiji.yoshimura at montana.edu
MAX MILLENNIUM NEWS
14 April 2021
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
Three-dimensional magnetic reconnection in astrophysical plasmas
-- Ting Li, Eric Priest and Ruilong Guo
Energy partition in a confined flare with an extreme-ultraviolet late phase
-- Q. M. Zhang, J. X. Cheng, Y. Dai, K. V. Tam, and A. A. Xu
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 keiji.yoshimura at montana.edu