Can the Auroral Kilometric Radiation be a Self-Organized Criticality System?

被引:0
|
作者
Marek, M. [1 ]
Schreiber, R. [1 ]
机构
[1] Polish Acad Sci, Space Res Ctr, Warsaw, Poland
关键词
ELECTRON-CYCLOTRON MASER; FINE-STRUCTURE; DISTRIBUTIONS; BURSTS; SOLAR; FIELD; AKR;
D O I
10.1029/2021EA002148
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present statistical results for the analysis of 240 Auroral Kilometric Radiation (AKR) dynamical spectra containing 3,750 short-time AKR bursts each, and recorded on-board Interball-2 mission (POLRAD and MEMO experiments). Data were collected between December 1996 and February 1998. We found that frequency distribution of short AKR bursts as a function of their Power Spectral Density, shows for intense bursts a powerlaw fall. This is the hallmark of the Self-Organized Criticality (SOC) systems. In our case a simple analytical Logistic Growth SOC model can reproduce increments of Electron Cyclotron Maser instability expected for AKR.
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页数:12
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