MAX MILLENNIUM NEWS 29 March 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
High-resolution observations of flare precursors in the low solar atmosphere -- Haimin Wang, Chang Liu, Kwangsu Ahn, Yan Xu, Ju Jing, Na Deng, Nengyi Huang, Rui Liu, Kanya Kusano, Gregory D. Fleishman, Dale E. Gary and Wenda Cao
Solar Energetic Particle transport near a Heliospheric Current Sheet -- Battarbee, M., Dalla, S., and Marsh, M.S.
Investigating the Magnetic Imprints of Major Solar Eruptions with SDO/HMI High-Cadence Vector Magnetograms -- Xudong Sun, J. Todd Hoeksema, Yang Liu, Maria Kazachenko, Ruizhu Chen
Coronal loop density profile estimated by forward modelling of EUV intensity -- D. J. Pascoe, C. R. Goddard, S. Anfinogentov, and V. M. Nakariakov
The magnetic connectivity of coronal shocks to the visible solar surface during long-duration gamma-ray events -- Illya Plotnikov, Alexis P. Rouillard, Gerald H. Share
Dissipative instability in a partially ionised prominence slab -- I. Ballai, B. Pinter, R. Oliver and M. Alexandrou
Significance testing for quasi-periodic pulsations in solar and stellar flares -- C. E. Pugh, A.-M. Broomhall, V. M. Nakariakov
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