Max Millennium News

Keiji YOSHIMURA yosimura at solar.physics.montana.edu
Wed May 18 08:54:24 MDT 2022


                          MAX MILLENNIUM NEWS
                             18 May 2022

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

A first look at the submillimeter Sun with ALMA
-- C. E. Alissandrakis, T. S. Bastian, and A. Nindos

Data-driven modeling of solar coronal magnetic field evolution and eruptions
-- Chaowei Jiang, Xueshang Feng, Yang Guo, Qiang Hu

Properties and Energetics of Magnetic Reconnection: I. Evolution of Flare Ribbons
-- J. Qiu & J. Cheng

A new look at the frequency-dependent damping of slow-mode waves in the solar corona
-- Dmitrii Y. Kolotkov, Valery M. Nakariakov

What determines active region coronal plasma composition?
-- Teodora Mihailescu, Deborah Baker, Lucie M. Green, Lidia van Driel-Gesztelyi,
   David M. Long, David H. Brooks, Andy S. H. To

Characteristics and evolution of sheath and leading edge structures
of interplanetary coronal mass ejections in the inner heliosphere
based on Helios and Parker Solar Probe observations
-- Manuela Temmer and Volker Bothmer


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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