MAX MILLENNIUM NEWS 20 April 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
The Coronal Physics Investigator (CPI) Experiment for ISS: A New Vision for Understanding Solar Wind Acceleration -- J. L. Kohl, S. R. Cranmer, J. C. Raymond, T. J. Norton, P. J. Cucchiaro, D. B. Reisenfeld, P. H. Janzen, B. D. G. Chandran, T. G. Forbes, P. A. Isenberg, A. V. Panasyuk, A. A. van Ballegooijen
Coronal Shock Waves, EUV waves, and their Relation to CMEs. II. Modeling MHD Shock Wave Propagation Along the Solar Surface, Using Nonlinear Geometrical Acoustics -- A. N. Afanasyev, A. M. Uralov
Coronal Shock Waves, EUV waves, and Their Relation to CMEs. I. Reconciliation of ''EIT waves'', Type II Radio Bursts, and Leading Edges of CMEs -- V. V. Grechnev, A. M. Uralov, I. M. Chertok, I. V. Kuzmenko, A. N. Afanasyev, N. S. Meshalkina, S. S. Kalashnikov, Y. Kubo
Coronal Shock Waves, EUV Waves, and Their Relation to CMEs. III. Shock-Associated CME/EUV Wave in an Event with a Two-Component EUV Transient -- V. V. Grechnev, A. N. Afanasyev, A. M. Uralov, I. M. Chertok, M. V. Eselevich, V. G. Eselevich, G. V. Rudenko, Y. Kubo
Hard X-ray footpoint sizes and positions as diagnostics of flare accelerated energetic electrons in the low solar atmosphere -- Marina Battaglia, Eduard P. Kontar
Instrumental oscillations in RHESSI count rates during solar flares -- A. R. Inglis, I. V. Zimovets, B. R. Dennis, E. P. Kontar, V. M. Nakariakov, A. B. Struminsky and A. K. Tolbert
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
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