Skip to main content
Log in

S 4 index: Does it only measure ionospheric scintillation?

  • Original Article
  • Published:
GPS Solutions Aims and scope Submit manuscript

Abstract

The study of ionospheric scintillation has played a critical role in ionospheric research and also in satellite positioning. This is due to the growing influence of GNSS in navigation and remote sensing activities and also because the scintillation severely degrades the performance of this system. The main parameter that has been used to investigate the ionospheric scintillation impact on quality of GNSS satellite signals is the S 4 index. However, we show that other effects such as multipath may mask the scintillation effects. Furthermore, we propose a method to separate the effect of multipath from scintillation in the S 4 index by a non-decimated wavelet multiscale decomposition, which is shift invariant and more appropriate to use in the analysis of time series. The results show that the multipath effect is evident in the smoother scales of multiscale decomposition by wavelet in the weak scintillation period. Once identified and estimated, this effect can be removed from the S 4 index series during strong scintillation periods and it becomes not significant in the scintillation S 4 index wavelet analysis. Investigations using data from different stations and satellites demonstrate that the effect of ionospheric scintillation varies with station location and elevation angle of the satellite. Therefore, each case must be treated individually.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Fig. 1
Fig. 2
Fig. 3
Fig. 4
Fig. 5
Fig. 6
Fig. 7
Fig. 8
Fig. 9
Fig. 10

Similar content being viewed by others

References

  • Brassarote GON, Souza EM, Monico JFG (2015) Multiscale analysis of GPS time series from non-decimated wavelet to investigate the effects of ionospheric scintillation. TEMA (São Carlos) 16(2):119–130

    Article  Google Scholar 

  • Briggs BH, Parkin IA (1963) On the variation of radio star and satellite scintillations with zenith angle. J Atmos Terr Phys 25(6):339–366

    Article  Google Scholar 

  • Camargo PO, Monico JFG, Ferreira LDD (2000) Application of ionospheric corrections in the equatorial region for L1 GPS users. Earth Planets Space 52(11):1083–1089

    Article  Google Scholar 

  • Davies K (1990) Ionospheric radio. Peter Peregrinus Ltd, London, p 580

    Book  Google Scholar 

  • Kelley MC (1989) The earths ionosphere: plasma physics and electrodynamics. Academic Press, San Diego

    Google Scholar 

  • Kintner PM, Kil H, Beach TL, de Paula ER (2001) Fading timescales associated with GPS signals and potential consequences. Radio Sci 36(4):731–743

    Article  Google Scholar 

  • Kintner PM, Ledvina BM, de Paula ER (2007) GPS and ionospheric scintillations. Space. Weather 5:S09003. https://doi.org/10.1029/2006SW000260

    Google Scholar 

  • Maini AK, Agrawal V (2007) Satellite technology: principles and applications. Wiley, India

    Google Scholar 

  • Mallat SG (1989) A theory for multiresolution signal decomposition: the wavelet representation. IEEE Trans Pattern Anal 11(7):674–693

    Article  Google Scholar 

  • Materassi M, Alfonsi L, De Franceschi G, Romano V, Mitchell CN, Spalla P (2009) Detrend effect on the scalograms of GPS power scintillation. Adv Space Res 43(11):1740–1748

    Article  Google Scholar 

  • McNamara LF (1991) The ionosphere: communications, surveillance, and direction finding. Krieger publishing company, Malabar

    Google Scholar 

  • Mushini SC, Jayachandran PT, Langley RB, Macdougall JW, Pokhotelov D (2012) Improved amplitude-and phase-scintillation indices derived from wavelet detrended high-latitude GPS data. GPS Solut 16(3):363–373

    Article  Google Scholar 

  • Nason GP (2008) Wavelet methods in statistics with R. Springer, New York

    Book  Google Scholar 

  • Percival DB, Walden AT (2000) Wavelets methods for time series analysis. Cambridge University Press, Cambridge

    Book  Google Scholar 

  • Starck JL, Murtagh F, Bertero M (2011) Starlet transform in astronomical data processing. In: Handbook of mathematical methods in imaging, Springer, New York, pp 1489–1531

    Chapter  Google Scholar 

  • Streets RBJ (1969) Variation of radio star and satellite scintillations with sunspot number and geomagnetic latitude. J Can Soc Expl Geophys 5:35–52

    Google Scholar 

  • Tiwari R, Skone S, Tiwari S, Strangeways HJ (2011) 3WBMod Assisted PLL GPS software receiver for mitigating scintillation affect in high latitude region. In: IEEE General assembly and scientific symposium, 2011 XXXth URSI, pp 1–4

  • Tiwari R, Strangeways HJ, Tiwari S, Ahmed A (2013) Investigation of ionospheric irregularities and scintillation using TEC at high latitude. Adv Space Res 52(6):1111–1124

    Article  Google Scholar 

  • Vani BC, Shimabukuro MH, Monico JFG (2016) Visual exploration and analysis of ionospheric scintillation monitoring data: the ISMR query tool. Comput Geosci. https://doi.org/10.1016/j.cageo.2016.08.022

    Google Scholar 

Download references

Acknowledgements

The author would like to thank FAPESP (Foundation for Research Support of the State of São Paulo) for the scholarship to the first author (FAPESP Process No. 2012/13362-5), CNPq for the financial support (Processes 304247/2012-0 and 473973/2012) and Projects CIGALA and CALIBRA (funded by the European Commission in the framework of the FP7-GALILEO-2009-GSA and FP7–GALILEO–2011–GSA–1a, respectively, and FAPESP Project No. 06/04008-2) for database.

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to Gabriela de Oliveira Nascimento Brassarote.

Appendix: NDWT pyramid algorithm

Appendix: NDWT pyramid algorithm

Given a time series {\(X_{t} : t = 0, \ldots ,N - 1\)}, the result of the filtering of \(\{ X_{t} \}\) with the NDWT wavelet \(\{ \tilde{h}_{k} \}\) and scaling \(\{ \tilde{g}_{k} \}\) filters is given, respectively, by (Percival and Walden 2000)

$$\tilde{W}_{j,t} = \mathop \sum \limits_{k = 0}^{K - 1} \tilde{h}_{j,k} X_{t - k\bmod N}$$
(5)
$$\tilde{V}_{j,t} = \mathop \sum \limits_{k = 0}^{K - 1} \tilde{g}_{j,k} X_{t - k\bmod N} ,\quad t = 0,1, \ldots , N - 1$$
(6)

The two sequences given by (5) and (6), called NDWT wavelet and scaling coefficients, represent the NDWT of decomposition level \(j\), and stipulate that the elements of \(\tilde{W}_{j}\), \(\tilde{V}_{j}\) and \(\tilde{V}_{j - 1}\) are obtained by circularly filtering of \(\{ X_{t} \}\) with the filters \(\{ \tilde{g}_{j,k} \} , \{ \tilde{h}_{j,k} \}\) and \(\{ \tilde{h}_{j - 1,k} \}\), respectively. The term “mod” from the equations refers to “maximal overlap discrete,” that treats time series X as if it were circular, making X to be represented with the same number N of coefficients at each scale.

However, it is possible to obtain \(\tilde{W}_{j}\) and \(\tilde{V}_{j}\) by filtering of \(\tilde{V}_{j - 1}\) as in the following equation

$$\tilde{W}_{j,t} = \mathop \sum \limits_{k = 0}^{K - 1} \tilde{h}_{k} \tilde{V}_{{j - 1,t - 2^{j - 1} k\bmod N}}$$
(7)
$$\tilde{V}_{j,t} = \mathop \sum \limits_{k = 0}^{K - 1} \tilde{g}_{k} \tilde{V}_{{j - 1,t - 2^{j - 1} k\bmod N}} ,\quad t = 0,1, \ldots , N - 1$$
(8)

Equations (7) and (8) represent the NDWT pyramid algorithm, and they can be written in matrix form as

$$\tilde{W}_{j,t} = \tilde{B}_{j} \tilde{V}_{j - 1} \;{\text{and}}\;\tilde{V}_{j} = \tilde{A}_{j} \tilde{V}_{j - 1}$$
(9)

where the rows of \(\tilde{B}_{j}\) contain circularly shifted versions of \(\{ \tilde{h}_{k} \}\) after it has been upsampled to width \(2^{j - 1} (K - 1) + 1\), that consists of inserting \(2^{j - 1 }\) zeros between each of the K values of the original filter, and then periodized to length N, and with a similar construction for \(\tilde{A}_{j}\) based upon \(\{ \tilde{g}_{k} \}\)(Percival and Walden 2000).

The NDWT also allows reconstructing \(\tilde{V}_{j - 1}\) from \(\tilde{W}_{j}\) and \(\tilde{V}_{j}\). The inverse NDWT acts to restore the signal in the time domain from its decomposition, and it can be calculated via inverse pyramidal algorithm described by the following equation,

$$\tilde{V}_{j - 1,t} = \mathop \sum \limits_{k = 0}^{K - 1} \tilde{h}_{k} \tilde{W}_{{j,t + 2^{j - 1} k\bmod N}} + \mathop \sum \limits_{k = 0}^{K - 1} \tilde{g}_{k} \tilde{V}_{{j,t + 2^{j - 1} k\bmod N}} , \quad t = 0,1, \ldots , N - 1$$
(10)

which can be expressed in matrix notation as

$$\tilde{V}_{j - 1} = \tilde{B}_{j}^{T} \tilde{W}_{j} + \tilde{A}_{j}^{T} \tilde{V}_{j}$$
(11)

where \(\tilde{B}_{j}^{T}\) and \(\tilde{A}_{j}^{T}\) are transposed matrix of \(\tilde{B}_{j}\) and \(\tilde{A}_{j}\), respectively.

Rights and permissions

Reprints and permissions

About this article

Check for updates. Verify currency and authenticity via CrossMark

Cite this article

de Oliveira Nascimento Brassarote, G., de Souza, E.M. & Monico, J.F.G. S 4 index: Does it only measure ionospheric scintillation?. GPS Solut 22, 8 (2018). https://doi.org/10.1007/s10291-017-0666-x

Download citation

  • Received:

  • Accepted:

  • Published:

  • DOI: https://doi.org/10.1007/s10291-017-0666-x

Keywords

Navigation