MAX MILLENNIUM NEWS 11 Ocober 2017 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

Reconstruction of a Large-scale Pre-flare Coronal Current Sheet Associated with an Homologous X-shaped Flare -- Chaowei Jiang, Xiaoli Yan, Xueshang Feng, Aiying Duan, Qiang Hu, Pingbing Zuo, Yi Wang

Comparison of Two Coronal Magnetic Field Models for Reconstructing a Sigmoidal Solar Active Region With Coronal Loops -- Aiying Duan, Chaowei Jiang, Qiang Hu, Huai Zhang, G. Allen Gary, S. T. Wu, Jinbin Cao

A Magnetic Bald-Patch Flare in Solar Active Region 11117 -- Chaowei Jiang, Xueshang Feng, S. T. Wu, Qiang Hu

Reply to comment by Usoskin (2017) on the paper "On a role of quadruple component of magnetic field in defining solar activity in grand cycles" -- Zharkova V.V., Popova E., Shepherd S.J. and Zharkov S.

Non-thermal hydrogen Balmer and Paschen emission in solar flares generated by electron beams -- Druett M. and Zharkova V.V.

Pulsations in the Earth's Lower Ionosphere Synchronized with Solar Flare Emission -- Laura A. Hayes, Peter T. Gallagher, Joseph McCauley, Brian R. Dennis, Jack Ireland, Andrew Inglis

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