Plasma-induced magnetic responses during nonlinear dynamics of magnetic islands due to resonant magnetic perturbations

2014 ◽  
Vol 21 (12) ◽  
pp. 122502 ◽  
Author(s):  
Seiya Nishimura
2015 ◽  
Vol 57 (10) ◽  
pp. 104007 ◽  
Author(s):  
Hai Jin ◽  
Qiming Hu ◽  
Nengchao Wang ◽  
Bo Rao ◽  
Yonghua Ding ◽  
...  

Entropy ◽  
2019 ◽  
Vol 21 (7) ◽  
pp. 648 ◽  
Author(s):  
Pavlos ◽  
Malandraki ◽  
Khabarova ◽  
Karakatsanis ◽  
Pavlos ◽  
...  

In this study we use theoretical concepts and computational-diagnostic tools of Tsallis non-extensive statistical theory (Tsallis q-triplet: qsen, qrel, qstat), complemented by other known tools of nonlinear dynamics such as Correlation Dimension and surrogate data, Hurst exponent, Flatness coefficient, and p-modeling of multifractality, in order to describe and understand Small-scale Magnetic Islands (SMIs) structures observed in Solar Wind (SW) with a typical size of ~0.01–0.001 AU at 1 AU. Specifically, we analyze ~0.5 MeV energetic ion time-intensity and magnetic field profiles observed by the STEREO A spacecraft during a rare, widely discussed event. Our analysis clearly reveals the non-extensive character of SW space plasmas during the periods of SMIs events, as well as significant physical complex phenomena in accordance with nonlinear dynamics and complexity theory. As our analysis also shows, a non-equilibrium phase transition parallel with self-organization processes, including the reduction of dimensionality and development of long-range correlations in connection with anomalous diffusion and fractional acceleration processes can be observed during SMIs events.


2013 ◽  
Vol 20 (10) ◽  
pp. 102510 ◽  
Author(s):  
F. Orain ◽  
M. Bécoulet ◽  
G. Dif-Pradalier ◽  
G. Huijsmans ◽  
S. Pamela ◽  
...  

2012 ◽  
Vol 52 (8) ◽  
pp. 083011 ◽  
Author(s):  
Qiming Hu ◽  
Q. Yu ◽  
Bo Rao ◽  
Yonghua Ding ◽  
Xiwei Hu ◽  
...  

1996 ◽  
Vol 36 (10) ◽  
pp. 1369-1388 ◽  
Author(s):  
R.J Buttery ◽  
T.C Hender ◽  
J.D Ashall ◽  
K.B Axon ◽  
G Blow ◽  
...  

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