MAX MILLENNIUM NEWS
7 May 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
Linear analysis of shear-flow instabilities in a prominence-corona interface
with ambipolar diffusion
-- Llorenc Melis, Roberto Soler
Tracking an eruptive …
[View More]intermediate prominence originating from the farside of the Sun
-- Qingmin Zhang, Wenwei Pan, Beili Ying, Li Feng, Yiliang Li, Xiaoli Yan,
Liheng Yang, Ye Qiu, Jun Chen, Suli Ma
Tracing the heliospheric magnetic field via anisotropic radio-wave scattering
-- Daniel L. Clarkson, Eduard P. Kontar, Nicolina Chrysaphi, A. Gordon Emslie,
Natasha L. S. Jeffrey, Vratislav Krupar, Antonio Vecchio
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
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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 March 2025 are as follows:
No. 492, “Metis observations of Alfvénic outflows driven by interchange reconnection in a pseudostreamer,” by Paolo ROMANO and the Metis team: Something that looks exactly as predicted by numerical simulations!
No. 493, “Quasi-Periodic Pulsations in Ionospheric TEC and Flare EUV,” by Aislng O’HARE: The …
[View More]Earth’s ionosphere shows flare-driven QPPs, with a small delay.
No. 494, “On turbulent magnetic reconnection: fast and slow mean steady-states,” by Sage STANISH and David MacTAGGART: In a turbulent medium, magnetic reconnection has two limiting domains
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.
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