MAX MILLENNIUM NEWS 11 January 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
What can we learn about solar coronal mass ejections, coronal dimmings, and Extreme-Ultraviolet jets through spectroscopic observations? -- Hui Tian, Scott W. McIntosh, Lidong Xia, Jiansen He, Xin Wang http://solar.physics.montana.edu/cgi-bin/eprint/index.pl?entry=15884
Impulsive Phase Coronal Hard X-ray Sources in an X3.9 Class Solar Flare -- Qingrong Chen, Vahe Petrosian http://solar.physics.montana.edu/cgi-bin/eprint/index.pl?entry=15883
Magnetoacoustic waves in diagnostics of the flare current sheets -- Jelinek, P., Karlicky, M. http://solar.physics.montana.edu/cgi-bin/eprint/index.pl?entry=15881
Small-scale, Dynamic Bright Blobs in Solar Filaments and Active Regions -- Y. Lin, O. Engvold and L.H.M. Rouppe van der Voort http://solar.physics.montana.edu/cgi-bin/eprint/index.pl?entry=15878
Why isn't the solar constant a constant? -- K. J. Li, W. Feng, J. C. Xu, P. X. Gao, L. H. Yang, H. F. Liang, L. S. Zhan http://solar.physics.montana.edu/cgi-bin/eprint/index.pl?entry=15877
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