Next Article in Journal
Projected Increase in Heatwaves under 1.5 and 2.0 °C Warming Levels Will Increase the Socio-Economic Exposure across China by the Late 21st Century
Previous Article in Journal
Application of Shannon Entropy in Assessing Changes in Precipitation Conditions and Temperature Based on Long-Term Sequences Using the Bootstrap Method
Previous Article in Special Issue
Investigation and Validation of Short-Wave Scattering in the Anisotropic Ionosphere under a Geomagnetic Field
 
 
Font Type:
Arial Georgia Verdana
Font Size:
Aa Aa Aa
Line Spacing:
Column Width:
Background:
This is an early access version, the complete PDF, HTML, and XML versions will be available soon.
Article

Polynomial Fitting-Based Noise Reduction for Correlation Functions in Medium-Frequency Radar

1
National Key Laboratory of Electromagnetic Environment, China Research Institute of Radiowave Propagation, Qingdao 266107, China
2
Kunming Electro-Magnetic Environment Observation and Research Station, Qujing 655500, China
3
Qujing Electro-Magnetic Environment Observation and Research Station, Qujing 655500, China
4
College of Electronics and Information, Guangxi Minzu University, Nanning 530006, China
5
College of Information and Commnunication, National University of Defense Technology, Changsha 410073, China
*
Authors to whom correspondence should be addressed.
These authors contributed equally to this work.
Atmosphere 2024, 15(8), 899; https://doi.org/10.3390/atmos15080899 (registering DOI)
Submission received: 9 June 2024 / Revised: 18 July 2024 / Accepted: 24 July 2024 / Published: 27 July 2024

Abstract

In the theoretical calculation of atmospheric wind fields using the cross-correlation analysis method of Medium-Frequency radar, it is necessary to compute a series of correlation parameters from the received echo signals, such as autocorrelation and cross-correlation functions, within the main lobe range of the antenna array to retrieve atmospheric parameters. However, both theoretical analysis and practical applications have shown that the shape of correlation functions can be affected by atmospheric conditions and receiver noise, leading to significant biases in the estimated correlation parameters within the main lobe range. In this study, we theoretically analyze the influence of noise on the amplitude of autocorrelation and cross-correlation functions. We propose a noise reduction method based on the characteristics of correlation functions at the zero-delay point to calculate the noise factor and process the correlation functions within the main lobe range. Furthermore, we conduct simulation analysis to evaluate the performance of this noise reduction method and summarize the effects of the number of fitting points and fitting methods on the noise reduction performance.
Keywords: noise impact on correlation functions; correlation function denoising; polynomial fitting; cross-correlation analysis method noise impact on correlation functions; correlation function denoising; polynomial fitting; cross-correlation analysis method

Share and Cite

MDPI and ACS Style

Chen, J.; Zhang, Y.; Wang, L.; Kang, G.; Li, N.; Wei, J. Polynomial Fitting-Based Noise Reduction for Correlation Functions in Medium-Frequency Radar. Atmosphere 2024, 15, 899. https://doi.org/10.3390/atmos15080899

AMA Style

Chen J, Zhang Y, Wang L, Kang G, Li N, Wei J. Polynomial Fitting-Based Noise Reduction for Correlation Functions in Medium-Frequency Radar. Atmosphere. 2024; 15(8):899. https://doi.org/10.3390/atmos15080899

Chicago/Turabian Style

Chen, Jinsong, Yang Zhang, Liming Wang, Guoqin Kang, Na Li, and Junfeng Wei. 2024. "Polynomial Fitting-Based Noise Reduction for Correlation Functions in Medium-Frequency Radar" Atmosphere 15, no. 8: 899. https://doi.org/10.3390/atmos15080899

Note that from the first issue of 2016, this journal uses article numbers instead of page numbers. See further details here.

Article Metrics

Back to TopTop