MAX MILLENNIUM NEWS
28 January 2026
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
High-Resolution Solar X-ray Spectroscopy from Archived Solar Maximum Mission Data
-- K. J. H. Phillips, B. Sylwester, J. Sylwester
Fast Magnetoacoustic Wave Behavior within Gravitationally Stratified,
Magnetically Inhomogeneous Media
-- Ryan T. Smith, James A. McLaughlin, and Gert J. J. Botha
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
MAX MILLENNIUM NEWS
21 January 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
Magnetic flux cancellation in a flux-emergence magnetohydrodynamics simulation
of coronal hole eruptions and jets
-- Spiros Patsourakos, Vasilis Archontis
Observation and Modeling of Shear Evolution of Post-reconnection Flare Loops
-- Drake Osaben, Jiong Qiu, Dana Longcope
Cycle dependence of helioseismic oscillations above the acoustic cut-off frequency
-- Dmitrii Kolotkov, Anne-Marie Broomhall, Laura Jade Millson, Sergey Belov
Thread separation and expansion observed in multi-stranded solar coronal loops
--David H. Brooks, Harry P. Warren
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 January 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
Spatial Variation of Energy Transport Mechanisms Within Solar Flare Ribbons
-- Graham S. Kerr, Sam Krucker, Joel C. Allred, Jenny M. Rodriguez-Gomez,
Andrew Inglis, Daniel F. Ryan, Laura A. Hayes, Ryan O. Milligan,
Adam F. Kowalski, Joeseph E. Plowman, Peter R. Young, Therese A. Kucera, and
Jeffrey W. Brosius
A Sudden Fine-scale Bright Kernel Captured by Hi-C Flare in 11 MK Emission
during an M1.6-class Solar Flare's Postmaximum Phase
-- Sanjiv K. Tiwari, Navdeep K. Panesar, Ron Moore, Sabrina Savage,
Amy Winebarger, Genevieve Vigil, et al.
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. 512, “Iron Flourescence in X-Class Flares” by Abhilash SARWADE: A new spectroscopic capability for Iron K-alpha flourescence radiation.
No. 513, “The M- and X-class White Light Flares in Super Active Region NOAA 13644/13697” by Zhichen JING and Ying Li: “Super” active regions have relatively more frequent X-class flares, which correlate well with visible continuum (white-light flare) emission.
No. 514, “Fine structures in solar flare ribbons” by Jonas THOEN FABER: Elongated “riblets” commonly rise out of flare ribbons, and have characteristic Doppler shifts.
No. 515, “On the relationship between nanoflare energy and delay in the closed solar corona” by Shanwlee SOW MONDAL et al: Nanoflaring implies energy storage and sudden release, suggesting correlation between event energy and its timing.
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
7 January 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
Particle Kinetics and Dynamics in Flaring Atmospheres Leading to Sunquakes
-- V. Zharkova and S.Zharkov
Statistical Study of Appearance Timing of H-alpha Postflare Loops:
Simple Scaling Law Based on Radiative Cooling
-- Takato Otsu, Ayumi Asai, Kai Ikuta, Kazunari Shibata
On the Connection of Coronal Loop Plasma with the Ambient Magnetic Field
-- Fabio Reale, Gabriele Cozzo, Paolo Pagano, Paola Testa
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