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 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