MAX MILLENNIUM NEWS 04 February 2015 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

KAPPA: A Package for Synthesis of optically thin spectra for the non-Maxwellian kappa-distributions based on the CHIANTI database -- Dzifcakova, E., Dudik, J., Kotrc, P., Farnik, F., Zemanova, A.

SWAP Observations of Post-flare Giant Arches in the Long-Duration 14 October 2014 Solar Eruption -- Matthew J. West and Daniel B. Seaton

Inverse diffraction for the Atmospheric Imaging Assembly in the Solar Dynamics Observatory -- Gabriele Torre, Richard A Schwartz, Federico Benvenuto, Anna Maria Massone, Michele Piana

An explanation for the difference between physical conditions in two ribbons in the July 23, 2002 flare -- N.M. Firstova

Are Halo-like Solar Coronal Mass Ejections Merely a Matter of Geometric Projection Effects? -- Ryun-Young Kwon, Jie Zhang, and Angelos Vourlidas

Forecasting F10.7 with solar magnetic flux transport modeling -- C. J. Henney, W. A. Toussaint, S. M. White, and C. N. Arge

FIP Bias Evolution in a Decaying Active Region -- D. Baker, D. H. Brooks, P. Demoulin, S. L. Yardley, L. van Driel-Gesztelyi, D. M. Long, L. M. Green

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 canfield at physics.montana.edu