Phase Code Integration Using Interpulse Techniques for Enhanced Radar Performance

  • Basmah Ahmad
  • , Faran Awais Butt*
  • , Ijaz Haider Naqvi
  • , Saqib Ejaz
  • , Saqib Ali
  • , Ali Hussein Muqaibel
  • , Saleh A. Alawsh
  • , Muhammad Arif Anwar
  • *Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

Phase coding plays an important role in radar systems, affecting signal modulation, target detection, and interference rejection. This study assesses various phase codes, including Gold, Kasami, Barker, Frank, and Chaotic codes, by analyzing performance metrics like cross-correlation and peak-to-sidelobe ratio (PSLR). The study highlights certain limitations, suggesting the need for new waveform solutions. It integrates component-based and Kronecker product-based interpulse coding to combine different codes and improve overall system performance. By merging phase codes effectively, interpulse coding leverages the strengths of individual codes to produce a composite waveform with enhanced autocorrelation and cross-correlation properties, improving radar performance. An optimization problem is formulated using a weighted performance metric to identify the best waveform, considering factors such as cross-correlation and PSLR. The approach, utilizing simple Kronecker and element-wise multiplication techniques, offers significant benefits with minimal complexity. The Barker-Gold interpulse code stands out as highly effective for spread spectrum-based applications due to its favorable correlation properties.

Original languageEnglish
Pages (from-to)51680-51692
Number of pages13
JournalIEEE Access
Volume13
DOIs
StatePublished - 2025

Bibliographical note

Publisher Copyright:
© 2013 IEEE.

Keywords

  • Barker Code
  • Kasami code
  • Kronecker product
  • cross-correlation
  • gold code
  • interpulse coding
  • peak-to-side-lobe ratio
  • phase codes

ASJC Scopus subject areas

  • General Computer Science
  • General Materials Science
  • General Engineering

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