scholarly journals Angular dependence of pump-induced bottomside and topside ionospheric plasma turbulence at EISCAT

2011 ◽  
Vol 116 (A3) ◽  
Author(s):  
M. J. Kosch ◽  
E. Mjølhus ◽  
M. Ashrafi ◽  
M. T. Rietveld ◽  
T. Yeoman ◽  
...  
1999 ◽  
Vol 26 (1) ◽  
pp. 37-40 ◽  
Author(s):  
M. C. Lee ◽  
E. M. C. Klien ◽  
W. J. Burke ◽  
A. X. Zhang ◽  
R. J. Riddolls ◽  
...  

2016 ◽  
Vol 186 (11) ◽  
pp. 1189-1228 ◽  
Author(s):  
S.M. Grach ◽  
E.N. Sergeev ◽  
E.V. Mishin ◽  
Alexei V. Shindin

2016 ◽  
Vol 59 (11) ◽  
pp. 1091-1128 ◽  
Author(s):  
S M Grach ◽  
E N Sergeev ◽  
E V Mishin ◽  
A V Shindin

2008 ◽  
Vol 15 (6) ◽  
pp. 847-862 ◽  
Author(s):  
L. Dyrud ◽  
B. Krane ◽  
M. Oppenheim ◽  
H. L. Pécseli ◽  
J. Trulsen ◽  
...  

Abstract. Low frequency electrostatic turbulence in the ionospheric E-region is studied by means of numerical and experimental methods. We use the structure functions of the electrostatic potential as a diagnostics of the fluctuations. We demonstrate the inherently intermittent nature of the low level turbulence in the collisional ionospheric plasma by using results for the space-time varying electrostatic potential from two dimensional numerical simulations. An instrumented rocket can not directly detect the one-point potential variation, and most measurements rely on records of potential differences between two probes. With reference to the space observations we demonstrate that the results obtained by potential difference measurements can differ significantly from the one-point results. It was found, in particular, that the intermittency signatures become much weaker, when the proper rocket-probe configuration is implemented. We analyze also signals from an actual ionospheric rocket experiment, and find a reasonably good agreement with the appropriate simulation results, demonstrating again that rocket data, obtained as those analyzed here, are unlikely to give an adequate representation of intermittent features of the low frequency ionospheric plasma turbulence for the given conditions.


Author(s):  
Jan Błęcki ◽  
Michel Parrot ◽  
Jan Słomiński ◽  
Małgorzata Kościesza ◽  
Roman Wronowski ◽  
...  

2011 ◽  
Vol 29 (12) ◽  
pp. 2277-2286 ◽  
Author(s):  
L. P. Dyrud ◽  
J. Urbina ◽  
J. T. Fentzke ◽  
E. Hibbit ◽  
J. Hinrichs

Abstract. We present the first global simulations on the occurrence of meteor trail plasma irregularities. These results seek to answer the following questions: when a meteoroid disintegrates in the atmosphere, will the resulting trail become plasma turbulent? What are the factors influencing the development of turbulence? and how do these trails vary on a global scale? Understanding meteor trail plasma turbulence is important because turbulent meteor trails are visible as non-specular trails to coherent radars. Turbulence also influences the evolution of specular radar meteor trails; this fact is important for the inference of mesospheric temperatures from the trail diffusion rates, and their usage for meteor burst communication. We provide evidence of the significant effect that neutral atmospheric winds and ionospheric plasma density have on the variability of meteor trail evolution and on the observation of non-specular meteor trails. We demonstrate that trails are far less likely to become and remain turbulent in daylight, explaining several observational trends for non-specular and specular meteor trails.


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