A simple dynamical model for the description of binary glass-forming systems

1996 ◽  
Vol 226 (4) ◽  
pp. 268-282 ◽  
Author(s):  
Matthieu Micoulaut
1993 ◽  
Vol 141 ◽  
pp. 542-544
Author(s):  
P. Mein ◽  
N. Mein

AbstractWe use imaging spectroscopy from the MSDP of the VTT telescope in Tenerife (collaboration Paris-Meudon Observatory and Kiepenheuer Institut) to analyse Doppler velocities of arch filaments in Hα and NαD1. The geometry of the magnetic loops is deduced from perspective effects with a simple dynamical model. Velocities are correlated in both lines.Further results are expected from simultaneous observations with other instruments (SVST of La Palma and Huairou magnetograph).


1992 ◽  
Vol 128 ◽  
pp. 326-328 ◽  
Author(s):  
Roger W. Romani ◽  
J. M. Rankin ◽  
D. C. Backer

AbstractWe have examined high quality Arecibo data of three pulsars for evidence of strange attractors in pulse-to-pulse intensity fluctuations. Significant structure was found for PSR 0823+26, and seems related to pulse drifting and nulling activity. The low dimensionality of the possible attractor suggest that a simple dynamical model can explain this component of the flux variability.


2013 ◽  
Vol 27 (S1) ◽  
Author(s):  
Min‐Yeong KANG ◽  
Aurelie FOUCQUIER ◽  
Marcel FILOCHE ◽  
Bernard SAPOVAL

2018 ◽  
Vol 3 (3) ◽  
pp. 236-245 ◽  
Author(s):  
Christopher J. Duffy ◽  
Hilary A. Dugan ◽  
Paul C. Hanson

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