Ionospheric Es layer scintillation characteristics studied with Hilbert-Huang transform

S. Y. Su, L. C. Tsai, C. H. Liu, C. Nayak, R. Caton, K. Groves

Research output: Contribution to journalArticlepeer-review

8 Scopus citations

Abstract

A coincident event of daytime ionospheric Es layer scintillation observations is analyzed with the Hilbert-Huang transform (HHT) to study its layer structure. One of the coincident observations is made by a radio beacon passing through the Es layer at a slant angle received by the SCINDA (Scintillation Decision Aide) receivers located at southern Taiwan. The data indicates that the Es layer consists of scattering blocks of ∼ 650 to 970 m in size as revealed in the dominant components of the HHT analysis. The time shift in the two spaced receiving antennas implies that the daytime E region westward drift is about 36 m/s. On the other hand, the same Es layer is observed by the radio occultation (RO) experiment with the L1 signal from the Global Positioning System (GPS) satellites to the FORMOSAT-3/Constellation-Observing-System-for-Meteorology (FS-3/COSMIC) satellites. The GPS L1 signal passes through the Es layer horizontally. The observed signal variations reveal a dense slab structure that blocks the L1 signal to cause a diffraction pattern. The slab thickness in the vertical direction is about 780 m. The HHT analyses of the coincident observations thus conclude that the observed daytime Es layer has a vertical dense slab structure and patches of scattering blocks in the horizontal structure.

Original languageEnglish
Pages (from-to)2137-2144
Number of pages8
JournalAdvances in Space Research
Volume64
Issue number10
DOIs
StatePublished - 15 Nov 2019

Keywords

  • Daytime ionospheric Es layer scintillation
  • FORMASAT-3/COSMIC
  • Hilbert-Huang Transformation (HHT)
  • SCINDA

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