MAX MILLENNIUM NEWS 1 May 2013 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
Geometric properties of acoustic waves generated by a point source in the solar-like interior: effects of acoustic cutoff frequency -- S. Zharkov
Study of Failed CME Core Associated with Asymmetric Filament Eruption -- Joshi, N. C.; Srivastava, A. K.; Filippov, B.; Uddin, W.; Kayshap, P.; Chandra, R.
Simulation of the Observed Coronal Kink Instability and Its Implications for the SDO/AIA -- Srivastava, A. K.; Botha, G. J. J.; Arber, T. D.; Kayshap, P.
Investigating Two Successive Flux Rope Eruptions In A Solar Active Region -- X. Cheng, J. Zhang, M. D. Ding, O. Olmedo, X. D. Sun, Y. Guo & Y. Liu
Observations of intensity oscillations in a prominence-like cool loop system as observed by SDO/AIA: evidence of multiple harmonics of fast magnetoacoustic waves -- Srivastava, A. K.; Dwivedi, B. N.; Kumar, Mukul
Observational Evidence of Sausage-pinch Instability in Solar Corona by SDO/AIA -- Srivastava, A. K.; Erd?lyi, R.; Tripathi, Durgesh; Fedun, V.; Joshi, N. C.; Kayshap, P.
The Kinematics and Plasma Properties of a Solar Surge Triggered by Chromospheric Activity in AR11271 -- Kayshap, P.; Srivastava, Abhishek K.; Murawski, K.
Multi-thermal dynamics and energetics of a coronal mass ejection in the low solar atmosphere -- I. G. Hannah and E. P. Kontar
Determination of transverse density structuring from propagating MHD waves in the solar atmosphere -- I. Arregui, A. Asensio Ramos, D. J. Pascoe
Return currents and energy transport in the solar flaring atmosphere -- Anna Codispoti, Gabriele Torre, Michele Piana, Nicola Pinamonti
High rigidity Forbush decreases: due to CMEs or shocks? -- Arun Babu, H. M. Antia, S. R. Dugad, S. K. Gupta, Y. Hayashi, S. Kawakami, P. K. Mohanty, T. Nonaka, A. Oshima, P. Subramanian
Energetic Particle Diffusion In Critically Balanced Turbulence -- Laitinen, T., Dalla, S., Kelly, J., and Marsh, M.
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