MAX MILLENNIUM NEWS
28 April 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
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
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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
-----------------------------------
> 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
MAX MILLENNIUM NEWS
7 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
Alfven wave heating in partially ionized thin threads of solar prominences
-- Llorenc Melis, Roberto Soler, and Jose Luis Ballester
He I 10830A Dimming During Solar Flares, I:
The Crucial Role of Non-Thermal Collisional Ionisations
-- Graham S. Kerr, Yan Xu, Joel C. Allred, Vanessa Polito,
Viacheslav M. Sadykov, Nengyi Huang 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 keiji.yoshimura at montana.edu
Hi, all,
It is vital that high-energy solar physics – covering impulsive energy release, particle acceleration, and plasma heating at the Sun – is well represented at the upcoming Heliophysics 2050 Workshop (May 3–7) and in the white papers submitted to the next Decadal Survey. To be added to a discussion group led by myself, please send me your information using this very short Google form:
https://forms.gle/2pq4YhDr53Dbjgy6A
Everyone in the heliophysics community is welcome. Thanks!
Sincerely,
Albert Y. Shih