# Regional ionospheric modeling using wavelet network model

- Mohammed El-Diasty
^{1, 2}Email author

**15**:2

**DOI: **10.1186/s41445-017-0007-y

© The Author(s) 2017

**Received: **16 November 2016

**Accepted: **11 May 2017

**Published: **22 May 2017

## Abstract

A major error component of Global Positioning System (GPS) is the ionospheric delay. Ionopspheric error can be reduced by a dual frequency receiver using a linear combination technique that can not be applied with a single frequecy receiver. However, an accurate ionospheric error modeling for single-frequency receiver is required. Due to the nonlinearity of the ionospheric error, a highly nonlinear wavelet network (WN) method is proposed in this paper. The main objective of the paper is to develop a short-term prediction model based on a short dataset. Therefore, five GPS stations with five days of ionospheric datasets along with time and location were employed to develop the proposed WN-based ionospheric model. Four days of datasets were employed to develop the model and one day of dataset was employed to test the prediction accuracy. To validate the WN-based ionospheric model, a comparison was made between the developed WN-based ionospheric model and the CODE, JPL and IGS Global Ionospheric Map (GIM) models. It is shown that the Root-Mean-Squared (RMS) errors of the developed WN-based ionospheric model are 2.51 TECU, 2.75 TECU and 2.50 TECU (Total Electronic Content Unit) with percentage errors of about 3.4%, 3.8% and 3.4% when compared with the CODE, JPL and IGS GIM models.

### Keywords

GPS Ionospheric delay Wavelet network Total electron content (TEC) GIM model## Introduction

*L*frequency band and are subject to important distortions while crossing the ionosphere. The ionospheric delay is due to the electron concentration in the ionosphere layers. It varies during the day with the ionisation of the particles hit by sun rays. It is a consequence of the dispersive nature of the medium, which causes sinusoidal waves with different frequencies to travel at slightly different velocities. As a result, the satellite signal is submitted to a group delay and a phase advance of identical amplitudes. The ionospheric delay

*I*is computed as a function of the electron content along the signal trajectory through the ionosphere as follows (Misra and Enge 2006):

where *d* is the distance delay (m) in comparison to the propagation in vacuum, TEC is the electron concentration determined along the oblique trajectory (total electron content for the concerned path in el/m2), *f is* signal frequency (Hz), S is the path from the transmitter to the receiver (m) and *n* is the electron density (el/m3).

The equation here above only considers the first order effect of ionosphere on signals propagation. The ionospheric delay mathematical representation is actually a limited development. According to the need of precision in the expression of the ionospheric delay the second order effect and the third order effect may be taken into account. The second (1/f^{3}) and third order effect (1/f^{4}) are functions of the plasma frequency, the electrons gyrofrequency and the direction of the wave with relation to the magnetic field. In most of the cases only the first order effect is considered to assess the ionospheric delay. In the case of GPS signals, the second order effect is typically of a magnitude of a few centimeters, while the third order effect has a typical magnitude of some millimeters.

All of the GPS errors can be corrected to some extent by implementing model algorithms depending on the applications. A major error component of GPS positioning is the ionospheric delay. However, unlike other GPS errors, ionospheric delay correction is hard and complex to model because the ionosphere shows both spatial and temporal behavior. Ionopspheric error can be reduced by a dual frequency receiver using a linear combination technique that can not be applied for a single frequecy receiver. Operationally for single-frequency receiver, the Klobuchar model is employed to correct for ionospheric error, however, the Klobuchar model permits to correct about 50% of the ionospheric error for mid-latitudes location and average ionospheric environment (Klobuchar, 1975). Therefore, the ionospheric modeling has been investigated for last few decades to develop an accurate ionospheric correction for single-frequency receiver. Currently, GPS analysis centers provide GIMs (Global Ionosphere Maps) on a daily basis. The widely used GPS-derived GIMs are provided by the Center for Orbit Determination in Europe (CODE), the Jet Propulsion Laboratory (JPL) and the International GNSS Service (IGS) with a spatial resolution of 2.5° and 5.0° in latitude and longitude, respectively, and a 2-h temporal resolution (Komjathy 1997; Feltens and Jakowski 2002). However, the Global Ionospheric Map (GIM) models (GIM) models such as CODE, JPL and IGS GIM models cannot reproduce local, short-lasting processes in the ionosphere. In addition, the resolution of these products might not be sufficient to support high quality GPS positioning, especially in the presence of local ionospheric disturbances. The need to produce regional ionosphere models for accurate positioning was investigated by many researchers (Komjathy and Langley, 1996; Hernández-Pajares et al., 1997; Hernandez- Pajares et al. 1999; Liu and Gao, 2003; Wielgosz et al., 2003; Moon, 2004; Leandro and Santos 2007; Sayin et al., 2008; Maruyama, 2007; Liu et al., 2011; Liu et al., 2014; Ohashi et al., 2015 and Razin et al., 2015), where different algorithms were employed for regional ionosphere modeling such as Spherical harmonics, Spline interpolation, Gaussian process, kriging and artificial neural networks. However, due to the nonlinearity of ionosphere physical properties a highly nonlinear model a highly nonlinear wavelet network method is proposed in this paper to model and predict the temporal and spatial variations of ionosphere modeling. The main objective of the paper is to develop a short-term prediction model based on a short dataset. Therefore, five GPS stations with five days of ionospheric datasets along with time and location with 15 min sampling rate are employed to develop the proposed WN-based ionospheric model. Four days of datasets are employed to develop the model and one day of dataset is employed to test the prediction accuracy. Also, a comparison is made between the proposed wavelet network based ionospheric model and the well-established CODE, JPL and the IGS Global Ionospheric Map (GIM) models.

## Ionospheric delay estimation

The major range error for GPS measurements is mainly due the deviation of the speed of the signal from its actual light speed because of the presence of free electrons in the ionosphere medium. This medium is extended from 50 km to about 1000 km above the earth surface. The variations of the ionospheric effects are mainly governed by the ionization processes, which is caused by the solar radiation. Hence there is a direct relationship and the state of the ionosphere can be realized by observing the intensity of the solar activity. The physical characteristics of the ionosphere have noticeable diurnal (day and night) variations. During the sun rise, the electron density starts to build up due to the ultraviolet radiations which help to break up gas molecules into ions and free electrons (Leick, 2004; Hofmann-Wellenhof et al., 2008).

Single-frequency receivers can access eight ionospheric coefficients, located in the GPS navigation message to estimate the ionospheric delay based on the Klobuchar model. These coefficients are generated at least once per 6 days but no more than once a day and they are updated by the 5 GPS Ground Control Segment stations. The Klobuchar algorithm is a physical model that considers the changes in latitude, season, solar flux and magnetic activity representing the amplitude change along with the associated diurnal period change of the ionospheric delay. The Klobuchar model permits to correct about 50% of the ionospheric error for mid-latitudes location and average ionospheric environment. Therefore, the ionospheric modeling has been investigated for last few decades to develop an accurate ionospheric correction for single-frequency receiver applications. To develop a regional ionospheric model, the ionospheric error is estimated using dual frequency receivers distributed in the area under consideration as discussed below.

*L*frequency bands (

*L1*and

*L2*) and a dual frequency receiver can be used to provide code measurements (

*P*

_{ f1}and

*P*

_{ f2}) and carrier-phase measurements (

*ϕ*

_{ f1}and

*ϕ*

_{ f1}). The receiver is able to assess the ionospheric delay on

*f1*using code measurements combination

*I*

_{ P − f1}or using carrier-phase measurements combination

*I*

_{ ϕ − f1}of identical amplitudes as follows (Hofmann-Wellenhof et al., 2008):

*ϕ*

_{ f2}−

*ϕ*

_{ f1})

_{0}and (

*P*

_{1}−

*P*

_{2})

_{0}are the initial values of the carrier-phase measurements combination and code measurements combination, respectively, and

*el*is the number of electrons. Fig. 1 shows an example of a noisy and smoothed TEC for one satellite.

*α*) is estimated, the Zenith angle at receiver (

*z*') and the Zenith angle at IPP (

*z*) can be estimated as follows:

It is worth noting that an appropriate cut-off angel is used to ignore those satellites with bad geometry and under horizon level (Hofmann-Wellenhof et al., 2008).

where *z* is the zenith angle at pierce point.

In this paper, the wavelet network model is proposed to model the estimated VTEC form a number of GPS receivers in a regional area and the model was validated by the Global Ionospheric Model (GIM) developed by the CODE analysis center.

## Wavelet network model

*ŷ*

_{ k }computed as:

*c*

_{ i }are coefficient variables,

*a*

_{ m }are dilation variables,

*b*

_{ m }are translation variables, and

*Ψ*is a wavelet function. Fig. 3 shows the wavelet network structure. The wavelet network consists of an input vector of

*N*

_{ m }values, a layer of

*N*

_{ i }weighted wavelets and an output vector of

*N*

_{ k }output neurons. The wavelet network parameters (

*c*

_{ i },

*a*

_{ m }, and

*b*

_{ m }) can be estimated by a backpropagation-learning method (Haykin 1999; Lekutai, 1997; Zhang and Benveniste, 1992).

*N*

_{ k }is the number of outputs, \( {y}_k^d \) is the desired output values and

*ŷ*

_{ k }is the network output estimated from Eqn. (9), then, the wavelet network training objective is to minimize the error function,

*E*(Haykin 1999; Lekutai 1997; Zhang and Benveniste, 1992):

*x*is:

where, ‖*x*‖^{2} = *x*
^{T}
*x*, and *p* is the order of the model (12)

The structure of the wavelet network is determined by empirical methods. The number of neurons can be determined by training different architectures with different number of neurons to select the optimal number, based on the lowest RMS error (El-Diasty et al. 2007). It should be noted that the dilation and transition properties of the wavelet function make the wavelet network much more dynamic, flexible, robust, and promising methodology for regional ionospheric modeling and prediction than traditional artificial neural network method.

## Methods

The structure of the wavelet network was built using the Matlab software version 2010. Many wavelet network models were carried out to optimize the structure of the wavelet network using four days of dataset to build the model and one day of dataset to test (prediction mode) the proposed WN-based model. It was found that the wavelet network with the structure [5–90–1] provides the best solution with the lowest root-mean-square (RMS) error. The input layer of five values that represent first input of the day number (one to five), second input of the time of the day (from 0 to 24 in 15 min interval), third input of the latitude of the IPP point (in radians), fourth input of the longitude of the IPP (in radians) and fifth input of the estimated Klobuchar model at same IPP point. The hidden layer of 90 wavelet neurons (wavelons) was employed to model the desired VTEC value.

## Results and discussion

The summary statistical results when the absolute VTEC mean estimated from wavelet network model is compared with the ones estimated from CODE, JPL and IGS GIM models for training dataset (4 days)

Statistical parameter | WN-based model versus CODE GIM model | WN-based model versus JPL GIM model | WN-based model versus IGS GIM model |
---|---|---|---|

Correlation between the WNbased model and GIM model | 87.9% | 86.7% | 87.7% |

RMS error between the WNbased model and GIM model | 2.51 TECU | 2.75 TECU | 2.50 TECU |

ercentage of error | 3.4% | 3.8% | 3.4% |

Absolute VTEC error bias | 1.95 TECU | 1.90 TECU | 1.78 TECU |

Absolute VTEC maximum error | 7.9 TECU | 8.54 TECU | 7.3 TECU |

The summary statistical results when the absolute VTEC mean estimated from wavelet network model is compared with the ones estimated from CODE, JPL and IGS GIM models for testing (prediction) dataset (1 day)

Statistical parameter | WN-based model versus CODE GIM model | WN-based model versus JPL GIM model | WN-based model versus IGS GIM model |
---|---|---|---|

Correlation between the WNbased model and GIM model | 88.12% | 86.5% | 88.5% |

RMS error between the WNbased model and GIM model | 2.50 TECU | 2.83 TECU | 2.40 TECU |

Percentage of error | 3.60% | 4.2% | 3.4% |

Absolute VTEC error bias | 1.78 TECU | 2.03 TECU | 1.89 TECU |

Absolute VTEC maximum error | 7.17 TECU | 8.54 TECU | 5.78TECU |

## Conclusion

The main objective of the paper is to develop a short-term prediction model based on a short dataset. An ionospheric model using a wavelet network method was proposed and developed in this paper. GPS data from five stations for five days long were used to implement and validate the proposed model. The wavelet network structure of 5–90–1 gave the best performance solutions (i.e., the minimum RMS), and therefore was used in modeling the VTEC values. It is shown that the Root-Mean-Squared (RMS) errors of the developed WN-based ionospheric model are 2.51 TECU, 2.75 TECU and 2.50 TECU (Total Electronic Content Unit) with percentage errors of about 3.4%, 3.8% and 3.4% when compared with the CODE, JPL and IGS GIM models and with a maximum absolute error of about 7.17 TECU, 8.17 TECU and 5.74 TECU, respectively. Therefore, in practice the developed WN model can be used for real-time regional ionospheric modeling for accurate GPS positioning with a single frequency GPS receiver and can reduce the ionospheric error with about 96% in average.

## Declarations

### Competing interest

The author declare that they have no competing interests

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## Authors’ Affiliations

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