MAX MILLENNIUM NEWS
18 December 2024
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
A model of solar magnetic flux rope eruption initiated primarily
by magnetic reconnection
-- Qingjun Liu, Chaowei Jiang, Xinkai Bian, Xueshang Feng, Pingbing Zuo, Yi Wang
Are Solar Active Regions Born with Neutralized Currents?
-- Aiying Duan, Yaoyu Xing and Chaowei Jiang
Why are non-radial solar eruptions less frequent than radial ones?
-- Qingjun Liu, Chaowei Jiang, Xueshang Feng, Pingbing Zuo, Yi Wang
From Fundamental Theory to Realistic Modeling of the Birth of Solar Eruptions
-- Chaowei Jiang
An explanation for the slow-rise phase of solar eruptions
-- Yaoyu Xing, Aiying Duan, Chaowei Jiang
A New Approach of Data-driven Simulation and Its Application
to Solar Active Region 12673
-- Zhi-Peng Liu, Chao-Wei Jiang, Xin-Kai Bian, Qing-Jun Liu, Peng Zou and
Xue-Shang Feng
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
Please find the new SolarNuggets, extending our old RHESSI Nuggets, at
https://heliowiki.smce.nasa.gov/wiki/index.php/SolarNuggets.
Entries for October and November 2024:
No. 479, "Remarkable NUV Spectrum of an M-star Megaflare,” by Adam KOWALSKI
No. 478, "Revised Point-Spread Functions of AIA and their effect on DEM analyses,” by Stefan HOFMEISTER, Daniel Wolf SAVIN, and Michael HAHN
No. 477, "How much of the energy in flare-accelerated electrons reaches the chromosphere?” by Meriem ALAOUI and Gordon HOLMAN
No. 476, "Spatially resolved plasma composition evolution in a solar flare,” by Andy S. H. To
No. 475, “HOPE during high activity,” by Hugh HUDSON and Alphonse STERLING
No. 474, "Simulated heliospheric electron spectra show sensitivity to plasma properties of a source region in the flaring corona,” by Ross PALLISTER and Natasha JEFFREY
No. 473, "An extremely complex active region with very strong non-neutralized electric currents," by Ioannis KONTOGIANNIS
No. 472, “An X9 flare and its huge crochet (SFE)” by Hugh HUDSON
We apologize for the interruption of service and thank Damian Barrous and Steven Christe for major help in getting re-started. As always, we welcome new items and encourage opinion pieces and news items as well as descriptions of new discoveries.
Just email Hugh Hudson with a page of text and 2-3 nice figures.
Temporally resolved Type III solar radio bursts in the frequency range 3-13 MHz
by A. Vecchio et al.
https://www.astro.gla.ac.uk/users/eduard/cesra/?p=3896
Spectral cleaving in solar type II radio bursts: Observations and interpretation
by A. Koval et al.
https://www.astro.gla.ac.uk/users/eduard/cesra/?p=3902
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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
11 December 2024
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
Non-local thermal transport impact on compressive waves
in two-temperature coronal loops
-- S. A. Belov, T. Goffrey, T. D. Arber, D. Y. Kolotkov
Universal Constants and Energy Integral in Self-Organized Criticality Systems
-- Markus J. Aschwanden
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
4 December 2024
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
Sympathetic solar eruption on 2024 February 9
-- Shu-Yue Li, Qing-Min Zhang, Bei-Li Ying, Li Feng, Ying-Na Su, Mu-Sheng Lin,
Yan-Jie Zhang
On the Instrumental Discrepancies in Lyman-Alpha Observations of Solar Flares
-- Harry J. Greatorex, Ryan O. Milligan and Ingolf E. Dammasch
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
I'm forwarding a message from Hugh.
Keiji Yoshimura
----- Forwarding message -------------------------------------------
From: Hugh Hudson <hshudson(a)gmail.com>
Subject: The RHESSI Nuggets have moved!
Date: December 3, 2024 at 3:24:00 PM GMT
To: mmscience(a)solar.physics.montana.edu
We have re-named our unpolished gems (The RHESSI Nuggets), now to be known as “SolarNuggets”, and they have a new URL: https://heliowiki.smce.nasa.gov/SolarNuggets. As always, anybody with interesting solar discoveries, news or views, can contribute material - typically a simple page of text and 2-3 figures.
MAX MILLENNIUM NEWS
27 November 2024
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
Observation of an Extraordinary Type V Solar Radio Burst:
Nonlinear Evolution of the Electron Two-Stream Instability
-- Benz, A. O.; Huber, C. R.; Timmel, V.; Monstein, C.
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
20 November 2024
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
Limb Observations of Global Solar Coronal Extreme-ultraviolet Wavefronts:
The Inclination, Kinematics, Coupling with the Expanding Coronal Mass Ejections,
and Connection with the Coronal Mass Ejection Driven Shocks
-- Huidong Hu, Bei Zhu, Ying D. Liu, Chong Chen, Rui Wang, Xiaowei Zhao
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
13 November 2024
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
Tracking an eruptive prominence using multiwavelength and multiview observations
on 2023 March 7
-- Qingmin Zhang, Yudi Ou, Zhenghua Huang, Yongliang Song, Suli Ma
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
6 November 2024
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
Modeling the Effects of a Light Bridge on Properties of Magnetohydrodynamic Waves
in Solar Pores
-- L. A. C. A. Schiavo, M. Gordovskyy, P. K. Browning, S. S. A. Silva, G. Verth,
I. Ballai, S. Shelyag, S. N. Ruzheinikov, J. A. McLaughlin, V. Fedun
Estimating early coronal mass ejection propagation direction with DIRECD
during the severe May 8 and follow-up June 8, 2024 events
-- Shantanu Jain, Tatiana Podladchikova, Astrid M. Veronig, Galina Chikunova,
Karin Dissauer, Mateja Dumbovic, Amaia Razquin
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