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Denoising of scintillated GNSS signal based on CEEMD-MFDFA method

  • Wasiu Akande Ahmed*
  • , Ganiy Ishola Agbaje
  • , Olakunle Rufus Oladosu
  • , Ngbede Joshua Ada Echoda
  • , Olugbenga Jimoh Hamed
  • *Corresponding author for this work
  • African Regional Centre for Space Science and Technology Education in English (ARCSSTE-E)

Research output: Contribution to journal › Conference article › peer-review

Abstract

The research on signal processing, modeling, imaging and techniques related to ionospheric effects has become a hot topic in recent years. A signal denoising technique that integrates complementary ensemble empirical mode decomposition (CEEMD) with multi-fractal detrended fluctuation analysis (MFDFA), refers to CEEMD-MFDFA is employed in this paper. The CEEMD method is introduced in recent time for adaptive signal decomposition, which is much better than the empirical mode decomposition (EMD) having mode mixing problem. First, the amplitude scintillated (noisy) signal is broken down into a given number of N intrinsic mode functions (IMFs) by CEEMD. However, based on criterion of MFDFA designed to select the number N, which aims to prevent over-binning or under-binning on the CEEMD denoising. Besides, MFDFA is also developed to determine with precision the relevant modes to reconstruct the original signal. The experimental results from real signal indicated the superior performance of CEEMD-MFDFA over CEEMD model based denoising.

Original languageEnglish
JournalProceedings of the International Astronautical Congress, IAC
Volume2020-October
StatePublished - 2020
Externally publishedYes
Event71st International Astronautical Congress, IAC 2020 - Virtual, Online
Duration: 12 Oct 2020 → 14 Oct 2020

Keywords

  • Amplitude scintillation
  • Complementary ensemble empirical mode decomposition (CEEMD)
  • Denoising
  • Multi-fractal detrended fluctuation analysis (MFDFA)
  • Over-binning or under-binning

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