Classification of VLF/LF Lightning Signals Using Sensors and Deep Learning Methods
Abstract
:1. Introduction
Novelty and Contributions
- Using the lightning waveforms and lightning location data from different regions collected by the three-dimensional lightning positioning network of the Institute of Electrical Engineering of the Chinese Academy of Sciences, a lightning waveform database was constructed for deep learning testing, training, and verification. The collected lightning signal is an electric field signal in the VLF/LF band.
- Based on the expert classification method, we classified the waveforms in the lightning waveform database. Currently, the database contains 10 types of lightning. It needs to be emphasized that we considered lightning signals transmitted from different distances, including but not limited to the basic types of lightning described earlier. This paper mainly analyzed the feasibility and effectiveness of deep learning methods in lightning signal classification.
- A lightning classification algorithm based on deep learning was proposed to replace the statistical method. The input of the algorithm is a fixed-length lightning signal, and the output is a lightning type number.
- Apply the classification algorithm to a thunderstorm process to detect the actual application of the algorithm. Test results showed that the model could accurately recognize lightning during this thunderstorm as high as 97.55%.
2. Dataset and Preprocessing
2.1. Lightning Dataset
2.2. Pre-Processing
- (1)
- Digital filter to reduce noise. The zero-phase digital filtering [27] method is used to remove the high-frequency noise contained in the signal. Zero-phase filtering reduces noise in the signal and preserves the lightning complex at the same time it occurs in the original. Conventional filtering reduces noise in the signal but delays the lightning complex. Figure 4 shows an example of suppressing signal noise by zero-phase digital filtering.
- (2)
- Data standardization (normalization) [28]. Data standardization is to scale the data to a specific interval according to a certain algorithm, remove the unit limit of the data, and convert it into a dimensionless pure value. Normally, standardization allows the features between different dimensions to be numerically comparable, which can greatly improve the accuracy of the classifier and prompt the convergence speed. The most typical one is the normalization of the data; that is, the data is uniformly mapped to [0,1]. Data normalization methods include min-max normalization (min-max normalization), log conversion, arctangent conversion, z-score normalization, and fuzzy quantization.
3. Methods
3.1. Independent Feature Branch
3.1.1. 1-D Convolution Layer
3.1.2. 1-D Pooling Layer
3.1.3. Fully-Connected Layer
3.2. Parameter Optimization
4. Result
4.1. Model Structure and Parameters
4.2. Train and Evaluate
4.3. Model Test
- (1)
- The +CG occurrence probability was significantly less than other classes, which resulted in fewer samples in this class.
- (2)
- We found that there were a few data that were significantly different from the waveforms in the data set when manually verifying the classification accuracy of the model. This was also the reason that the accuracy of +CG type recognition was significantly reduced.
5. Discussion
5.1. Methods Comparison
- (1)
- Pulse rise time. The time elapsed from the 10% peak of the waveform to the peak of the waveform. .
- (2)
- Pulse fall time. The time elapsed from the peak of the waveform to the 10% peak of the waveform. .
- (3)
- Pulse width. The time elapsed from the 10% peak of the rising edge to the 10% peak of the falling edge. .
- (4)
- Forward peak-to-peak ratio. The ratio of initial negative peak to maximum peak. .
- (5)
- Backward peak-to-peak ratio. The ratio of following negative peak to maximum peak. .
- (6)
- Sub-peak ratio. The ratio of the maximum peak to the secondary peak. .
- (7)
- Signal to noise ratio (SNR). The ratio of the average power of the signal within 20 before and after the peak point to the average power of the signal at other times.
- (8)
- Pre-SNR. The ratio of the average power of the signal within 20 before and after the peak point to the average power of the signal before the peak point.
- (9)
- Post-SNR. The ratio of the average power of the signal within 20 before and after the peak point to the average power of the signal after the peak point.
5.2. Model Structure Analysis
5.3. Real-Time Analysis
6. Conclusions
Supplementary Materials
Author Contributions
Funding
Acknowledgments
Conflicts of Interest
References
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No. | Layer | Filter Number | Kernel Size | Pooling Window Size | Padding | Stride | Activation Function | Output Shape |
---|---|---|---|---|---|---|---|---|
1 | Input | / | / | / | / | / | / | (1000,1) |
2 | 1D-Conv | 16 | 32 | / | √ | / | ReLU | (1000,16) |
3 | 1D- Conv | 16 | 32 | / | √ | / | ReLU | (1000,16) |
4 | Max-Pooling | / | / | 2 | × | 2 | / | (500,16) |
5 | 1D- Conv | 32 | 32 | / | √ | / | ReLU | (500,32) |
6 | 1D- Conv | 32 | 32 | / | √ | / | ReLU | (500,32) |
7 | Max-Pooling | / | / | 2 | × | 2 | / | (250,32) |
8 | 1D- Conv | 64 | 16 | / | √ | / | ReLU | (250,64) |
9 | 1D- Conv | 64 | 16 | / | √ | / | ReLU | (250,64) |
10 | Max-Pooling | / | / | 2 | × | 2 | / | (125,64) |
11 | 1D- Conv | 128 | 8 | / | √ | / | ReLU | (125,128) |
12 | 1D- Conv | 128 | 8 | / | √ | / | ReLU | (125,128) |
13 | Max-Pooling | / | / | 5 | × | 5 | / | (25,128) |
14 | 1D- Conv | 256 | 3 | / | √ | / | ReLU | (25,256) |
15 | 1D- Conv | 256 | 3 | / | √ | / | ReLU | (25,256) |
16 | Mean-Pooling | / | / | 5 | × | 5 | / | 256 |
17 | Dense | / | / | / | / | / | Softmax | 10 |
K | −CG (%) | CG-IR (%) | NBR (%) | +CG (%) | MP (%) | +PBP (%) | −PBP (%) | −NBE (%) | +NBE (%) | SW (%) | Ave (%) |
---|---|---|---|---|---|---|---|---|---|---|---|
1 | 98.84 | 99.40 | 98.88 | 99.64 | 99.58 | 100.00 | 96.50 | 99.80 | 98.16 | 99.82 | 99.06 |
2 | 96.16 | 99.10 | 94.98 | 99.86 | 99.86 | 99.94 | 98.20 | 99.80 | 99.30 | 99.00 | 98.62 |
3 | 99.04 | 99.34 | 99.36 | 99.96 | 99.82 | 99.94 | 98.36 | 99.92 | 99.18 | 99.84 | 99.47 |
4 | 97.74 | 99.32 | 98.64 | 99.58 | 99.84 | 99.96 | 98.42 | 99.92 | 99.36 | 99.80 | 99.26 |
5 | 98.52 | 98.82 | 98.48 | 99.16 | 99.74 | 99.92 | 97.68 | 99.88 | 99.04 | 99.88 | 99.11 |
Ave | 98.06 | 99.20 | 98.07 | 99.64 | 99.77 | 99.95 | 97.83 | 99.86 | 99.01 | 99.67 | 99.11 |
−CG | CG-IR | NBE | +CG | MP | +PBP | −PBP | −NBE | +NBE | SW | Total | |
---|---|---|---|---|---|---|---|---|---|---|---|
TP | 1321 | 1852 | 1180 | 179 | 260 | 417 | 830 | 729 | 298 | 2345 | 9411 |
NP | 23 | 28 | 84 | 32 | 8 | 4 | 32 | 3 | 0 | 22 | 236 |
Acc(%) | 98.29 | 98.51 | 93.35 | 84.83 | 97.01 | 99.05 | 96.29 | 99.59 | 100.00 | 99.07 | 97.55 |
Type | CC | CG | +NBE/−NBE | Other | Acc (%) |
---|---|---|---|---|---|
−CG | 2232 | 2752 | 0 | 16 | 55.04 |
CG-IR | 4196 | 582 | 0 | 222 | 11.64 |
NBE | 4049 | 1 | 0 | 950 | 80.98 |
+CG | 0 | 3436 | 0 | 1564 | 68.72 |
MP | 522 | 3 | 0 | 4475 | 10.44 |
+PBP | 1202 | 0 | 2 | 3796 | 24.04 |
−PBP | 3507 | 1 | 1 | 1491 | 70.14 |
−NBE | 0 | 4 | 3206 | 1790 | 64.12 |
+NBE | 0 | 904 | 3953 | 143 | 79.06 |
SW | 4620 | 66 | 0 | 314 | 92.40 |
Average | 55.66 |
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Wang, J.; Huang, Q.; Ma, Q.; Chang, S.; He, J.; Wang, H.; Zhou, X.; Xiao, F.; Gao, C. Classification of VLF/LF Lightning Signals Using Sensors and Deep Learning Methods. Sensors 2020, 20, 1030. https://doi.org/10.3390/s20041030
Wang J, Huang Q, Ma Q, Chang S, He J, Wang H, Zhou X, Xiao F, Gao C. Classification of VLF/LF Lightning Signals Using Sensors and Deep Learning Methods. Sensors. 2020; 20(4):1030. https://doi.org/10.3390/s20041030
Chicago/Turabian StyleWang, Jiaquan, Qijun Huang, Qiming Ma, Sheng Chang, Jin He, Hao Wang, Xiao Zhou, Fang Xiao, and Chao Gao. 2020. "Classification of VLF/LF Lightning Signals Using Sensors and Deep Learning Methods" Sensors 20, no. 4: 1030. https://doi.org/10.3390/s20041030
APA StyleWang, J., Huang, Q., Ma, Q., Chang, S., He, J., Wang, H., Zhou, X., Xiao, F., & Gao, C. (2020). Classification of VLF/LF Lightning Signals Using Sensors and Deep Learning Methods. Sensors, 20(4), 1030. https://doi.org/10.3390/s20041030