MAX MILLENNIUM NEWS 26 December 2018 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
Transition from axi- to nonaxisymmetric dynamo modes in spherical convection models of solar-like stars -- Viviani, M., Warnecke, J., Kapyla, M. J., Kapyla, P. J., Olspert, N., Cole-Kodikara, E. M., Lehtinen, J. J., & Brandenburg, A.
Can high-mode magnetohydrodynamic waves propagating in a spinning macrospicule be unstable due to the Kelvin-Helmholtz instability? -- Ivan Zhelyazkov and Ramesh Chandra
The development of lower-atmosphere turbulence early in a solar flare -- N. L. S. Jeffrey, L. Fletcher, N. Labrosse and P. J. A. Simoes
Determining the parameter for the linear force-free magnetic field model with multi-dipolar configurations using deep neural networks -- B. Benson , W. David Pan, G. Allen Gary , Q. Hu , T. Staudinger
2. FROM THE EDITOR ==================
The Max Millennium program exists to enhance all aspects of solar activity 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 richard.canfield at montana.edu