MAX MILLENNIUM NEWS 06 September 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

Development and Parameters of a Non-Self-Similar CME Caused by Eruption of a Quiescent Prominence -- Kuzmenko, I.V.; Grechnev, V.V.

Spectroscopy of Very Hot Plasma in Non-flaring Parts of a Solar Limb Active Region: Spatial and Temporal Properties -- Susanna Parenti, Giulio del Zanna, Antonino Petralia, Fabio Reale, Luca Teriaca, Paola Testa, and Helen E. Mason

Time variations of observed Hα line profiles and precipitation depths of non-thermal electrons in a solar flare -- R. Falewicz, K. Radziszewski, P. Rudawy, A. Berlicki

A Solar cycle correlation of coronal element abundances in Sun-as-a-star observations -- David H. Brooks, Deborah Baker, Lidia van Driel-Gesztelyi, Harry P. Warren

A Database of Flare Ribbon Properties from the Solar Dynamics Observatory. I. Reconnection Flux -- Kazachenko, Maria D.; Lynch, Benjamin J.; Welsch, Brian T.; Sun, Xudong

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