2015
DOI: 10.1134/s1063780x15030010
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Influence of inhomogeneities of the plasma density and electric field on the generation of electrostatic noise in the auroral zone

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Cited by 16 publications
(12 citation statements)
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“…The high-latitude ionosphere is characterized by intense small-scale irregularities and inhomogeneities in the plasma density [18][19][20] , which can be related to electric fields and increased precipitation of energetic particles. For example, the largest number of jumps in determining TEC during periods of geomagnetic storms is located close to the auroral oval 14 .…”
Section: The Influence Of An Auroral Substorm On the Total Electron Cmentioning
confidence: 99%
“…The high-latitude ionosphere is characterized by intense small-scale irregularities and inhomogeneities in the plasma density [18][19][20] , which can be related to electric fields and increased precipitation of energetic particles. For example, the largest number of jumps in determining TEC during periods of geomagnetic storms is located close to the auroral oval 14 .…”
Section: The Influence Of An Auroral Substorm On the Total Electron Cmentioning
confidence: 99%
“…26 and 27, and references herein). Numerical stability analysis using FAST or FREJA satellite data was carried out in recent papers, 20,21,[28][29][30] and it was confirmed that the IEDD instability could play an important role in the creation of electrostatic broadband turbulence (or noise) in the auroral zone and explain the experimental observations.…”
Section: Introductionmentioning
confidence: 74%
“…Later, these results were expanded using other sources of free energy such as field-aligned velocity of particles 19 and plasma density. 20,21 Fluctuations of the electric field and of the plasma density were successfully identified in laboratory experiments with plasma (e.g., Refs. [22][23][24][25].…”
Section: Introductionmentioning
confidence: 99%
“…The IEDDI can play a fundamental role in the generation of broadband electrostatic turbulence (or noise) in the auroral region high‐latitude ionosphere [ Hamrin et al , ; Chernyshov et al , ; Ilyasov et al , ] and for the outflow of ions from the ionosphere into the magnetosphere [ André et al , ]. Similar processes can be observed in regions of the high‐latitude ionosphere such as the cusp and the cleft.…”
Section: Introductionmentioning
confidence: 99%