MAX MILLENNIUM NEWS 18 May 2022
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 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 ------------------
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