LOFAR imaging spectroscopy reveals spike-like repeating radio burst pairs in the solar corona
by Suli Ma et al.
https://cesra.net/?p=4461
First Observational Evidence for Meridional Flow-like Profile in 17 GHz: Magnetic Trees on the Sun?
by Srinjana Routh et al.
https://cesra.net/?p=4475
A 19-day solar radio burst: a corotating radio reservoir in the outer corona
by Vratislav Krupar et al.
https://cesra.net/?p=4432
MAX MILLENNIUM NEWS
17 June 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
Polarity Reversal of the Polar Magnetic Fields in Solar Cycle 25
-- Li Y., Yang S. H., Zhang Y. Z., Song Q., Zhou G. P., Deng Y. Y., Wang J. X.
Comparative Analysis of Ellerman and Quiet Sun Ellerman Bombs
in the Solar Atmosphere
-- Ravi Chaurasiya, Ankala Raja Bayanna and Jayant Joshi
The Effect of Anomalous Resistivity on Tearing Instability
-- D. Tsiklauri
On the Relationship between Solar Spicules and Propagating Coronal Disturbances:
The Role of Shocks
-- Ravi Chaurasiya, Sankalp Srivastava, Piyali Chatterjee, Sahel Dey,
Robertus Erdelyi, Ankala Raja Bayanna
Interactions between fast Down-flows and Fan-shaped Jets above a Penumbral
Light Bridge using the Goode Solar Telescope
-- Kristina Brocklebank, Erwin Verwichte, and Juie Shetye
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
10 June 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
Peristaltic Flow in Compressible, Ideal Magnetohydrodynamics:
A Mechanism For Solar Spicules
-- D. Tsiklauri
Entropy-mode imprints in the solar corona: non-exponential damping and
phase shifts of compressive oscillations
-- Dmitrii Kolotkov, Sergey Belov, Mohamed Sherif
On the Relationship between Solar Spicules and Propagating Coronal Disturbances:
The Role of Shocks
-- Ravi Chaurasiya, Sankalp Srivastava, Piyali Chatterjee, Sahel Dey,
Robertus Erdelyi, Ankala Raja Bayanna
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
3 June 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
The Ly-alpha Emission in Solar Flares. II.
A Statistical Study on Its Relationship with the White-light plus Soft X-Ray Emission
-- De-Chao Song, Ying Li, Qiao Li, and Xiaofeng Liu
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
27 May 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 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
-----------------------------------
> 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