scholarly journals Chaos and Strange Attractors in Pulsar Intensity Records

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.

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).


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

2017 ◽  
Vol 27 (10) ◽  
pp. 1750153 ◽  
Author(s):  
Seyede Sanaz Hosseini ◽  
Fahimeh Nazarimehr ◽  
Sajad Jafari

The primary goal in this work is to develop a dynamical model capturing the influence of seasonal and latitudinal variations on the expression of Drosophila clock genes. To this end, we study a specific dynamical system with strange attractors that exhibit changes of Drosophila activity in a range of latitudes and across different seasons. Bifurcations of this system are analyzed to peruse the effect of season and latitude on the behavior of clock genes. Existing experimental data collected from the activity of Drosophila melanogaster corroborate the dynamical model.


1992 ◽  
Vol 128 ◽  
pp. 271-277
Author(s):  
M.V. POPOV ◽  
W. Sieber

Single-pulse radio emission from pulsars has been observed to vary both in intensity and position inside the pulse window. In some cases the variations show a rather regular structure (drifting subpulses). Such a regular structure can clearly be studied by fluctuation spectral analysis. The analysis has identified some particular peculiarities in the fluctuation spectra at different longitudes of the pulse window in many pulsars (Backer 1973, Page 1973, Popov and Smirnova 1982). In pulsars with complex integrated profiles (PSR 1919+21, PSR 1237+25) narrow features in the fluctuation spectra vary strongly with longitude, at some longitudes being quite undistinguishable.


2013 ◽  
Vol 40 (2) ◽  
pp. 307-311 ◽  
Author(s):  
David W. Rees Jones ◽  
M. Grae Worster

1987 ◽  
Vol 42 (6) ◽  
pp. 655-656
Author(s):  
J. Parisi ◽  
J. Peinke ◽  
B. Röhricht ◽  
U. Rau ◽  
M. Klein ◽  
...  

This paper gives a concrete physical interpretation of a simple dynamical model based on the universal Rashevsky- Turing theory of symmetry-breaking morphogenesis in terms of spatio-temporal nonlinear transport phenomena in a synergetic semiconductor system.


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