MAX MILLENNIUM NEWS 03 April 2019 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

Do Kepler superflare stars really include slowly-rotating Sun-like stars ? - Results using APO 3.5m telescope spectroscopic observations and Gaia-DR2 data -- Yuta Notsu, Hiroyuki Maehara, Satoshi Honda, Suzanne L. Hawley, James R. A. Davenport, Kosuke Namekata, Shota Notsu, Kai Ikuta, Daisaku Nogami, Kazunari Shibata

Magnetically Induced Current Piston for Generating Extreme-ultraviolet Fronts in the Solar Corona -- Pakorn Wongwaitayakornkul, Magnus A. Haw, Hui Li, Paul M. Bellan

Magnetic Field Dynamics and Varying Plasma Emission in Large-scale Coronal Loops -- S. Sahin, V. Yurchyshyn , P. Kumar, A. Kilcik, K. Ahn, and X. Yang

Nonlinear Evolution of Ion Kinetic Instabilities in the Solar Wind -- Leon Ofman

What determines the X-ray intensity and duration of a solar flare? -- Jeffrey W. Reep & Kalman J. Knizhnik

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