MAX MILLENNIUM NEWS 19 December 2012 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
A Note on Computation of Relative Magnetic Helicity Flux Across the Photosphere -- Yang Liu, Peter W. Schuck
Ejections of magnetic structures above a spherical wedge driven by a convective dynamo with differential rotation -- J. Warnecke, P.J. Kapyla, M.J. Mantere, A. Brandenburg
Magnetic Activity Cycles in the Exoplanet Host Star epsilon Eridani -- T.S. Metcalfe, A.P. Buccino, B.P. Brown, S. Mathur, D.R. Soderblom, T.J. Henry, P.J.D. Mauas, R. Petrucci, J.C. Hall, S. Basu
The Relationship Between Plasma Flow Doppler Velocities and Magnetic Field Parameters During the Emergence of Active Regions at the Solar Photospheric Level -- A. Khlystova
The Horizontal Component of Photospheric Plasma Flows During the Emergence of Active Regions on the Sun -- A. Khlystova
The Build-up to Eruptive Solar Events Viewed as the Development of Chiral Systems -- Sara F. Martin, Olga Panasenco, Mitchell A. Berger, Oddbjorn Engvold, Yong Lin, Alexei A. Pevtsov, Nandita Srivastava
Solar filament eruptions and their physical role in triggering Coronal Mass Ejections -- Schmieder B., Demoulin P., Aulanier G.
Can Superflares Occur on Our Sun ? -- Kazunari Shibata, Hiroaki Isobe, Andrew Hillier, Arnab Rai Choudhuri, Hiroyuki Maehara, Takako T. Ishii, Takuya Shibayama, Shota Notsu, Yuta Notsu, Takashi Nagao, Satoshi Honda, Daisaku Nogami
Direct Evidence for a Fast CME Driven by the Prior Formation and Subsequent Destabilization of a Magnetic Flux Rope -- S. Patsourakos, A. Vourlidas, G. Stenborg
Silicon Abundance from RESIK Solar Flare Observations -- B. Sylwester, K. J. H. Phillips, J. Sylwester, A. Kepa
Nonlinear Force-Free Magnetic Field Fitting to Coronal Loops with and without Stereoscopy -- Markus J. Aschwanden
Kappa Distribution Model for Hard X-Ray Coronal Sources of Solar Flares -- M. Oka, S. Ishikawa, P. Saint-Hilaire, S. Krucker and R. P. Lin
2. FROM THE EDITOR ------------------
The Max Millennium program exists to enhance all aspects of solar flare 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