Max Millennium News

Richard Canfield canfield at mithra.physics.montana.edu
Wed May 18 21:15:44 MDT 2016


                           MAX MILLENNIUM NEWS
                              18 May 2016
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

Undamped transverse oscillations of coronal loops as a
self-oscillatory process	 
-- Nakariakov, V. M., Anfinogentov, S., Nistico, G., Lee, D.-H.

Particle Acceleration in Solar Flares and Associated CME Shocks
-- Vahe Petrosian

Hard X-ray morphology of the X1.3 April 25, 2014 partially occulted
limb solar flare    
-- Frederic Effenberger, Fatima Rubio da Costa, Vahe Petrosian

Data-driven magnetohydrodynamic modelling of a flux-emerging
active region leading to solar eruption    
-- Chaowei Jiang, S. T. Wu, Xuesheng Feng, Qiang Hu

Global Energetics of Solar Flares: IV. Coronal Mass Ejection
Energetics	   
-- Aschwanden, M.J.

On the Characteristics of Footpoints of Solar Magnetic Flux Ropes
during the Eruption   
-- X. Cheng and M. D. Ding

Dependence of kink oscillation damping on the amplitude
-- Goddard, C.R., Nakariakov, V.M.

Magnetohydrodynamic oscillations in the solar corona and Earth's
magnetosphere: Towards consolidated understanding 
-- V.M. Nakariakov, V. Pilipenko, B. Heilig, P. Jelínek, M. Karlicky,
    D.Y. Klimushkin, D.Y. Kolotkov, D.-H. Lee, G. Nistico, T. Van
    Doorsselaere, G. Verth, I.V. Zimovets

Nonlinear oscillations of coalescing magnetic flux ropes
-- Dmitrii Y. Kolotkov, Valery M. Nakariakov, and George Rowlands

Magnetic reconnection between a solar filament and nearby coronal
loops	      
-- Leping Li, Jun Zhang, Hardi Peter, Eric Priest, Huadong Chen,
    Lijia Guo, Feng Chen, Duncan Mackay

Energetic characterisation and statistics of solar coronal
brightenings	     
-- V. Joulin, E. Buchlin, J. Solomon, C. Guennou

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


More information about the MMScience mailing list