MAX MILLENNIUM NEWS
23 July 2025
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
Observations of microwave emission from solar jets and
comparison with MHD simulations
-- Costas E. Alissandrakis, Vasilis Archontis, and Kostas Moraitis
Solar Alfvenic Pulses and Mesoscale Solar Wind
-- Jeongwoo Lee, Manolis K. Georgoulis, Rahul Sharma, Nour E. Raouafi, Qin Li,
Haimin Wang
Solar Spicules, Filigrees and Solar Wind Switchbacks
-- Jeongwoo Lee, Haimin Wang, Jiasheng Wang, Meiqi Wang
Solar Chromospheric Network as a Source for Solar Wind Switchbacks
-- Jeongwoo Lee, Vasyl Yurchyshyn, Haimin Wang, Xu Yang, Wenda Cao,
Juan Carlos Martinez Oliveros
Large-amplitude Oscillations of a Quiescent Filament
Excited by an Extreme-ultraviolet Wave
-- W. W. Pan, Q. M. Zhang, and Y. Qiu
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
16 July 2025
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
Ion-rich acceleration during an eruptive flux rope event
in a multiple null-point configuration
-- Melissa Pesce-Rollins, Alexander MacKinnon, Karl-Ludwig Klein,
Alexander Russell, Hugh Hudson, Alexander Warmuth, Thomas Wiegelmann,
Sophie Masson, Clare Parnell, Nariaki V. Nitta, Nicola Omodei
Spectropolarimetric synthesis of forbidden lines in MHD models
of coronal bright points
-- Ernest Alsina Ballester, Daniel Nobrega-Siverio, Fernando Moreno-Insertis,
and Supriya Hebbur Dayananda
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 would like to draw your attention to an AGU Fall Meeting (15-19 Dec 2025) session relevant to high-energy solar physics. While the meeting is still six months away, the abstracts are due 30th July 2025. Hope to see you in New Orleans!
https://agu.confex.com/agu/agu25/prelim.cgi/Session/248818
SH028. Solar Flares in the High-Resolution, High-Cadence Era: Observations, Modelling and Future Prospects
“Solar flares are fundamentally multi-scale phenomena that result from the dramatic and dynamic evolution of the Sun’s atmosphere and magnetic field, from photosphere through corona. Flares are now being observed with unprecedented spatial resolution at very high cadence, and sometimes from multiple viewpoints, providing remarkable new insights into flare energetics and evolution. Recent exciting observations include those from Solar Orbiter’s coordinated major flare campaigns, from IRIS’ high-cadence campaigns, and from ground-based observatories such as DKIST, SST and BBSO. These observations are challenging longstanding views of the flare energy release, transport and dissipation process, and have further revealed the significant sub-structure appearing within flare sources. Equal advancements in flare modeling are required to interpret the observations, and to demonstrate what future observations are required. We seek abstracts covering fine-scale flare structures, rapid temporal evolution, and future prospects for flare-optimized observations. Observational, modeling, instrumentation, and theoretical studies are all applicable and welcomed.”
Best,
Graham Kerr, Andrew Inglis, Gianna Cauzzi and Hannah Collier
--
Dr. Graham S. Kerr,
Research Scientist
PHaSER co-operative scientist
The Catholic University of America
Based at NASA Goddard Space Flight
620 Michigan Ave., NE
Washington DC
20064
O: 301.286.6745
E: kerrg(a)cua.edu

The SolarNuggets continue the earlier series of RHESSI Nuggets, and are now located at
https://heliowiki.smce.nasa.gov/wiki/index.php/SolarNuggets
The entries for June/July 2025 are as follows:
No. 498, “High-Resolution Observations of a C3 class White-Light Flare,” by Xiaoli YAN: Wonderful observations of a feeble flare
No. 499, “Quasiperiodic Pulsations in the Balmer Continuum in an X-class Solar White-light Flare,” by De-Chao SONG et al.: Penetrating observations reveal the pulsating heartbeat of a major flare.
No. 500, “Five Hundred Nuggets,” by Hugh HUDSON: A Nuggets milestone, with links to more Nuggets
No. 501, “The Aulanier Effect: drifting footpoints of CME flux ropes, by Jaroslav DUDÍK, Juray LÖRINČÍK, and Brigitte SCHMIEDER: Declaration of the need for 3D models of flares.
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
9 July 2025
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
Time evolution of white-light flare accompanied by probable postflare loops
on M-type dwarf EV Lacertae
-- Shinnosuke Ichihara, Daisaku Nogami, Kosuke Namekata, Hiroyuki Maehara,
Yuta Notsu, Kai Ikuta, Satoshi Honda, Takato Otsu, Kazunari Shibata
Relationship between prominence eruptions and coronal mass ejections
during solar cycle 24
-- Devi, Pooja ; Gopalswamy, Nat ; Yashiro, Seiji ; Akiyama, Sachiko ;
Chandra, Ramesh ; Koleva, Kostadinka
Counter-Streaming Velocities in a Quiescent Filament
-- Karki, Garima ; Schmieder, Brigitte ; Demoulin, Pascal ; Devi, Pooja ;
Chandra, Ramesh ; Joshi, Reetika
How the Solar Dynamic Observatory Revolutionized our Physical Understanding
of the Sun
-- 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
2 July 2025
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
NICER study of the low-ionized Fe K alpha line on RS Canum Venaticorum type stars
-- Shun Inoue, Teruaki Enoto, Yuta Notsu, Hiroyuki Uchida, Wataru Buz Iwakiri,
Kosuke Namekata, Keith Gendreau
The Relation between Solar Spicules and Magnetohydrodynamic Shocks
-- Sankalp Srivastava, Piyali Chatterjee, Sahel Dey, 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