MAX MILLENNIUM NEWS 28 September 2011

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

Origin of the submillimeter radio emission during the time-extended phase of a solar flare -- G. Trottet, J.-P. Raulin, G. Gimenez de Castro, T. Luthi, A. Caspi, C.H. Mandrini, M. L. Luoni, & P. Kaufmann

Radioheliograph observations of microwave bursts with zebra structures -- A.T. Altyntsev, S.V. Lesovoi, N.S. Meshalkina, R.A. Sych, Y. Yan

The Wave Properties of Coronal Bright Fronts Observed Using SDO/AIA -- Long, David M., DeLuca, Edward E., Gallagher, Peter T.

The problematic of large field-of-view spectropolarimetric observations with a large aperture telescope -- Molodij, G., Aulanier, G.

Ubiquitous rotating network magnetic fields and EUV cyclones in the quiet Sun -- Jun Zhang and Yang Liu

On the Force-Freeness of the Photospheric Sunspot Magnetic Fields as Observed from Hinode (SOT/SP) -- Sanjiv Kumar Tiwari

The quiet Sun average Doppler shift of coronal lines up to 2~MK -- N. Dadashi, L. Teriaca, S.K. Solanki

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