• DocumentCode
    2580047
  • Title

    Time-frequency analysis of ionosphere scintillations observed by a GNSS receiver array

  • Author

    Wang, Jun ; Morton, Yu ; Zhou, Qihou ; Van Graas, Frank ; Pelgrum, Wouter

  • Author_Institution
    Electr. & Comput. Eng., Miami Univ., Oxford, OH, USA
  • fYear
    2012
  • fDate
    23-26 April 2012
  • Firstpage
    274
  • Lastpage
    281
  • Abstract
    The objective of this paper is to present and compare performances of several time-frequency analysis algorithms that characterize and associate ionosphere scintillation events focusing on carrier phase measurements obtained from three relatively close spaced antennas in Alaska. The results will be used to derive plasma drift velocity and estimate the 2-dimension size of the scintillation patches. There are two challenges in detecting and associating scintillations among closely spaced receivers. First, we have to precisely estimate the start time and end time of the scintillation event captured by each receiver. Second, we have to distinguish the fluctuation caused by multipath and receiver clock from the effects of scintillation. Our approach is to analyze the time-frequency relations of GPS L1 signal observables among the receivers. Based on past experience, scintillation causes high frequency fluctuations in the range of 0.1 to 10 Hz, while multipath only introduce an extra frequency less than 1 Hz and are typically occurring at low elevations. Receiver clock errors are eliminated using differenced measurements from L1 and L2, or from a reference satellite without scintillation. Several algorithms have been studied to perform the time-frequency spectrum analysis of carrier phases: windowed Fourier transform (WFT), Morlet Wavelet transform (MWT), Hilbert-Huang transform (HHT), and an adaptive periodogram technique (APT). All four algorithms are evaluated using both simulated and real scintillation signals. Among them, APT provides the most optimal performance in terms of precision in detecting the occurrences of scintillation events in both time-domain and frequency-domain. However, APT also has a high computational cost. Morlet Wavelet transform offers complimentary performance with significantly lower computational cost. Thus, it is implemented as the level one scintillation filter before the events are finally analyzed by APT.
  • Keywords
    Fourier transforms; Hilbert transforms; antenna arrays; ionospheric electromagnetic wave propagation; radiowave propagation; satellite navigation; time-frequency analysis; wavelet transforms; APT; GNSS receiver array; GPS L1 signal; HHT; Hilbert-Huang transform; MWT; Morlet wavelet transform; WFT; adaptive periodogram technique; carrier phase measurement; close spaced antenna; closely spaced receiver; frequency 0.1 Hz to 10 Hz; frequency-domain analysis; ionosphere scintillation; plasma drift velocity; receiver clock error; scintillation patches; time-domain analysis; time-frequency spectrum analysis; windowed Fourier transform; Global Positioning System; Noise; Noise measurement; Receivers; Time frequency analysis;
  • fLanguage
    English
  • Publisher
    ieee
  • Conference_Titel
    Position Location and Navigation Symposium (PLANS), 2012 IEEE/ION
  • Conference_Location
    Myrtle Beach, SC
  • ISSN
    2153-358X
  • Print_ISBN
    978-1-4673-0385-9
  • Type

    conf

  • DOI
    10.1109/PLANS.2012.6236892
  • Filename
    6236892