Modeling of ionospheric scintillation with a full kinetic simulation

dc.contributorAalto-yliopistofi
dc.contributorAalto Universityen
dc.contributor.advisorKallio, Esa
dc.contributor.authorMahmood, Rafay
dc.contributor.schoolInsinööritieteiden korkeakoulufi
dc.contributor.schoolSchool of Engineeringen
dc.contributor.supervisorKallio, Esa
dc.date.accessioned2024-12-16T18:02:53Z
dc.date.available2024-12-16T18:02:53Z
dc.date.issued2024-11-18
dc.description.abstractIonospheric scintillation presents a significant challenge to the reliability of radio-based communication and navigation systems by causing fluctuations in the amplitude and phase of signals. These fluctuations are caused by irregularities in plasma density within the Earth’s ionosphere, which spans altitudes from 50 to 1000 kilometers and plays a crucial role in the propagation of radio waves. The ionosphere, ionized by solar radiation, acts as a dynamic plasma lens, altering the refractive index for electromagnetic (EM) waves. This thesis investigates the impact of plasma density variations on wave propagation, drawing parallels to the behavior of Gaussian lenses. Two simulation models are employed: the full kinetic model and the material EM model. In the full kinetic model, all charged particles are explicitly represented as particles. In contrast, the computationally less expensive material EM model does not simulate individual particles; instead, it incorporates the effects of charged particles through electric conductivity. The simulations were initiated using the full kinetic model. The effects of domain size, wave amplitude, and wave sources, with both point and plane waves, were investigated. Initial simulations used a uniform plasma, followed by ones with a plasma density-enhanced bubble. Later, a plasma bubble with reduced density was introduced to observe its effects, and comparisons were made between these two cases. Finally, the material EM model was applied to the same simulation configurations, and the results were compared with those from the full kinetic model. This showed that both models produced relatively similar results in the analyzed cases. In the final part of the study, the results from the two approaches were qualitatively compared with those obtained from a ray tracing simulation. The work suggests that both of the developed simulations, the full kinetic and material EM, provide useful tools to investigate ionospheric scintillation in detail.en
dc.format.extent60
dc.format.mimetypeapplication/pdfen
dc.identifier.urihttps://aaltodoc.aalto.fi/handle/123456789/132330
dc.identifier.urnURN:NBN:fi:aalto-202412167808
dc.language.isoenen
dc.programmeMaster's programme in Mechanical Engineeringen
dc.subject.keywordionospheric scintillationen
dc.subject.keywordfull kinetic modelen
dc.subject.keywordmaterial electromagnetic modelen
dc.subject.keyworddispersionen
dc.subject.keywordGaussian lensen
dc.subject.keywordplasma bubblesen
dc.titleModeling of ionospheric scintillation with a full kinetic simulationen
dc.typeG2 Pro gradu, diplomityöfi
dc.type.ontasotMaster's thesisen
dc.type.ontasotDiplomityöfi
local.aalto.electroniconlyyes
local.aalto.openaccessyes

Files

Original bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
master_Mahmood_Rafay_2024.pdf
Size:
4.99 MB
Format:
Adobe Portable Document Format