MAX MILLENNIUM NEWS
27 May 2026
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 Robust Deep Learning Framework for Prominence Detection through Composite
Feature Representations
-- Harry Birch, Stephane Regnier, Richard Morton
Signatures of coronal mass ejections in differential emission measure analysis
of the Sun as a star
-- Angelos Michailidis and Spiros Patsourakos
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 SolarNuggets continue the earlier series of RHESSI Nuggets, and are now located at
https://heliowiki.smce.nasa.gov/wiki/index.php/SolarNuggets
No. 524, “Observations of Slow Elemental Abundance Decay in Association to CME,” by Saara TAKALA. Solar X-ray spectroscopy tracks coronal abundance variations associated with a CME.
No. 525, “How Extreme can Solar Flare Get? A Statistical View," by Lapo CECCARELLI and Daniela CASTRO-CAMILO. A proper statistical treatment of the prospects for an extreme solar flare event.
No. 526, ”X-ray Log Letters,” by Hugh HUDSON and Ed CLIVER. Replacing ..ABCMX.. with a new comprehensive and quantitative index, and a QSabcmxyz catalog.
No. 527, “Space Weather Impact of Three Solar Flares Observed at Millimeter Wavelengths," by Adriana VALIO et al.. Radio mm waves tell an interesting new story.
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 news-oriented text and 2-3 nice figures.
MAX MILLENNIUM NEWS
20 May 2026
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
Effect of Solar Flares on Decayless Kink Oscillations in Nearby Coronal Loops
-- Li, Z., Nakariakov, V.M., Yuan, D., Feng, S.
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
Signatures of Large-scale Magnetic Field Disturbances and Switchbacks in Interplanetary Type III Radio Bursts
by Daniel L. Clarkson et al.
https://cesra.net/?p=4215
Dataset for Recognition and Detection Based on Solar Radio Spectrogram Data
by Yan et al
https://cesra.net/?p=4225
The SolarNuggets continue the earlier series of RHESSI Nuggets, and are now located at
https://heliowiki.smce.nasa.gov/wiki/index.php/SolarNuggets
No. 521, "Can EUV Power-Spectral Indices Reveal Imminent Solar Flares?” by Sihui ZHONG et al.: A new flare-precursor observable - power spectra.
No. 522, "Lateral Deformation of Large-scale Coronal Mass Ejections during the Transition from Nonradial to Radial Propagation,” by Huidong HU: Coronal mass ejections can begin their trajectory highly tilted to the vertical, but then straighten themselves out.
No. 523, "An Unusual Long-Lived Radio Burst Oscillating in Frequency,” by Marian Karlický et al.: Remarkable decimetric signatures of structured outflows from a flaring active region.
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 news-oriented text and 2-3 nice figures.
MAX MILLENNIUM NEWS
8 April 2026
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
A comparison of pendulum models for large-amplitude longitudinal prominence oscillations
-- Inigo Arregui
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
1 April 2026
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
Assessing VB_z variations during CME propagation:
a preparatory study for the HENON mission using EUHFORIA
-- Prete G., Niemela A., Poedts S., Zimbardo G., Cicalo S., Marcucci M. F.,
Laurenza M., Stumpo M., Landi S., Sangalli M., Provinciali L., Monferrini D.,
Calcagno D., Di Tana V., Walker R., Pecora F., Nistico G., Carbone V.,
Chiappetta F., Greco A., Lepreti F., Malara F., Perri S., Servidio S.
Magneto-rotational instability in a solar near-surface mean-field dynamo
-- Axel Brandenburg, Gustav Larsson, Fabio Del Sordo, Petri J. Kapyla
Signatures of localised particle acceleration at a global coronal shock wave
-- C. Cuddy, D. M. Long, M. Nedal, S. Bhunia, P. T. Gallagher
Evolution of the Shock Properties of the 2023 March 13 Event
from In-Situ and Remote-Sensing Data
-- Federica Chiappetta, Giuseppe Nistico', Massimo Chimenti, Andrea Larosa,
Francesco Malara, Francesco Pucci, Luca Sorriso-Valvo, Gaetano Zimbardo,
Silvia Perri
Ground level enhancement GLE number77 on 11 November 2025: a data summary
-- A.L. Mishev, B. Heber, K.-L. Klein, R. Vainio, H. Mavromichalaki,
O. Raukunen, N. Larsen, N. Petrov, N. Nikonov, S. Masson, M. Pesce-Rollins,
B.T. Kress, V. Bindi, M. Gerontidou, M. Hoerloeck, S. Koldobskiy,
E. Riihonen, J.V. Rodriguez, I. Usoskin
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 SolarNuggets continue the earlier series of RHESSI Nuggets, and are now located at
https://eur03.safelinks.protection.outlook.com/?url=https%3A%2F%2Fheliowiki…
No. 518, "When Magnetic Field Lines Stretch, Snap, and Expand: A New Look at Solar Flares with L-maps,” by Maria KAZACHENKO et al: A clever new tool tracks magnetic connectivity (and energy) during flare/CME occurrence.
No. 519, “Hinode EIS Observations of Plasma Composition Evolution and Radiative Cooling of Flare Loops,” by Teodora MIHAILESCU, Peter YOUNG, et al: Higher FIP bias than expected in some flare loops, a diagnostically interesting result.
No. 520, “How energetic can solar flares become?” by Natalie KRIVOVA. The history of active-region areas suggests the possibility of solar superflares.
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 news-oriented text and 2-3 nice figures.
MAX MILLENNIUM NEWS
25 March 2026
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
Evolution of Spatial Complexity in Flare Ribbon Substructure and
Its Relationship to Magnetic Reconnection Dynamics
-- Marcel F. Corchado Albelo, Maria D. Kazachenko, Ryan J. French,
Vadim M. Uritsky, Emily Mason, Cole A. Tamburri, Rahul Yadav, and
Benjamin J. Lynch
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
18 March 2026
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
Quasi-Periodic Fast-Mode Wave Trains Associated with the 2015-Jun-22 M6.5 Flare
in AR~12371: Observations and 3D MHD Modeling
-- Tongjiang Wang, Wei Liu, Leon Ofman, Xudong Sun, Meng Jin
SOL2024-07-16: Evidence for the CME-Driven Shock Origin of Late Phase Gamma-Ray Emission
-- Gerald Share
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