Max Millennium News

Richard Canfield canfield at mithra.physics.montana.edu
Wed Sep 16 14:02:10 MDT 2015


                           MAX MILLENNIUM NEWS
                            16 September 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

Why does the apparent mass of a coronal mass ejection increase?
-- Feng, Li; Wang, Yuming; Shen, Fang; Shen, Chenglong; Inhester,
   Bernd; Lu, Lei; Gan, Weiqun

Radial Flow Pattern of a Slow Coronal Mass Ejection	
-- Feng, Li; Inhester, Bernd; Gan, Weiqun

Heating and cooling of coronal loops observed by SDO 
-- Li, L. P., Peter, H., Chen, F., and Zhang, J.

APPEARANCES AND STATISTICS OF CORONAL CAVITIES DURING THE ASCENDING
PHASE OF SOLAR CYCLE 24     
-- N. Karna, W. D. Pesnell, and J. Zhang

STUDY OF THE 3D GEOMETRIC STRUCTURE AND TEMPERATURE OF A CORONAL
CAVITY USING THE LIMB SYNOPTIC MAP METHOD      
-- N. Karna, J.  Zhang, W. Dean Pesnell, and S. A. Hess Webber

Application of Kernel Based Machine Learning to Inversion Problem
of Photospheric Magnetic Fields       
-- Fei Teng

Hard X-Ray Imaging of Individual Spectral Components in Solar Flares
-- Amir Caspi, Albert Y. Shih, James M.  McTiernan, Sam Krucker

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
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