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GB/T 44434-2024 English PDF

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GB/T 44434-2024: Space environment - Technical requirements for meteor radar
Status: Valid
Standard IDUSDBUY PDFLead-DaysStandard Title (Description)Status
GB/T 44434-2024439 Add to Cart 4 days Space environment - Technical requirements for meteor radar Valid

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Basic data

Standard ID: GB/T 44434-2024 (GB/T44434-2024)
Description (Translated English): Space environment - Technical requirements for meteor radar
Sector / Industry: National Standard (Recommended)
Classification of Chinese Standard: M54
Classification of International Standard: 33.200
Word Count Estimation: 22,283
Date of Issue: 2024-09-29
Date of Implementation: 2024-09-29
Issuing agency(ies): State Administration for Market Regulation, China National Standardization Administration

GB/T 44434-2024: Space environment - Technical requirements for meteor radar

---This is a DRAFT version for illustration, not a final translation. Full copy of true-PDF in English version (including equations, symbols, images, flow-chart, tables, and figures etc.) will be manually/carefully translated upon your order.
Space environment - Technical requirements for meteor radar Technical requirements for space environment meteor radar ICS 33.200 CCS M 54 National Standard of the People's Republic of China Released on 2024-09-29 2024-09-29 implementation State Administration for Market Regulation The National Standardization Administration issued

Table of Contents

Preface ... Ⅲ 1 Scope ... 1 2 Normative references ... 1 3 Terms and Definitions ... 1 4 Meteor Radar ... 1 4.1 Overview ... 1 4.2 Classification ... 2 4.3 Composition 2 5 General requirements ... 2 5.1 Size, color, marking, appearance and completeness ... 2 5.2 Man﹘Machine﹘Environment System Engineering Requirements ... 3 6 Main technical requirements ... 3 6.1 General Requirements 3 6.2 Transmitting Antenna ... 4 6.3 Receiving Antenna ... 4 6.4 Feeder ... 4 6.5 Transmitter ... 5 6.6 Receiver ... 6 6.7 Data Processing and Display and Control Terminal ... 7 6.8 Power Supply ... 8 7 Quality Assurance Requirements ... 8 7.1 Environmental adaptability 8 7.2 Reliability and Maintainability ... 9 7.3 Electromagnetic compatibility 9 7.4 Security Requirements 9 7.5 Interchangeability 10 8 Installation Requirements ... 10 9 Deployment Requirements ... 10 9.1 Single-station meteor radar ... 10 9.2 Distributed Meteor Radar ... 10 Appendix A (Informative) Schematic diagram of meteor radar detection ... 11 Appendix B (Informative) Example of Meteor Radar Horizontal Wind Detection Data ... 13 Appendix C (Informative) Meteor Radar Receiving Antenna Array Configuration ... 15 References ... 16

Foreword

This document is in accordance with the provisions of GB/T 1.1-2020 "Guidelines for standardization work Part 1.Structure and drafting rules for standardization documents" Drafting is required. Please note that some of the contents of this document may involve patents. The issuing organization of this document does not assume the responsibility for identifying patents. This document was proposed by the Chinese Academy of Sciences. This document is under the jurisdiction of the National Technical Committee on Aerospace Technology and Its Applications Standardization (SAC/TC 425). This document was drafted by. National Space Science Center of the Chinese Academy of Sciences, China Institute of Radio Wave Propagation, Wuhan University, Chinese Academy of Sciences Institute of Geophysics, University of Science and Technology of China, Xidian University. The main drafters of this document are. Xu Qingchen, Feng Jian, Gong Yun, He Maosheng, Liang Xianfeng, Yan Zhaoai, Yan Chunxiao, Chen Gang, Hu Lianhuan, Yi Wen, Li Xue, Xu Na, Zhang Pengfei, Li Ping, Li Changhong, Ma Zheng. Technical requirements for space environment meteor radar

1 Scope

This document specifies the general requirements, main technical requirements, quality assurance requirements, installation requirements and layout requirements of Meteor Radar. This document is applicable to meteor distribution surveys that operate in the 25 MHz to 65 MHz frequency band and use meteor trails as the main tracer. and meteor radar for neutral atmospheric wind detection.

2 Normative references

The contents of the following documents constitute the essential clauses of this document through normative references in this text. Among them, the referenced documents with dates are. Only the version corresponding to that date applies to this document; for undated referenced documents, the latest version (including all revised versions) applies to this document. document. GB/T 12506-2017 General specification for wind radar GB/T 12648-1990 General technical requirements for weather radar GB/T 12649-2017 Weather radar parameter test method GB/T 30114.1 Space science and its application terminology Part 1.Basic general

3 Terms and definitions

The following terms and definitions as defined in GB/T 12506-2017, GB/T 12649-2017 and GB/T 30114.1 apply to this document. 3.1 meteor trail When a meteoroid enters the atmosphere at high speed, it rubs against the surrounding atmosphere, causing the material on the surface of the meteoroid to evaporate and ionize. Due to the violent collision with the meteoroid, it is ionized and diffused to form a plasma gas column centered on the meteor track. 3.2 meteor radar A radar device that uses the scattering effect of meteor trails on electromagnetic waves to detect meteor distribution and neutral atmospheric winds. Note. Generally, it can detect the distribution of meteors within the range of 70 km to 110 km above the radar station, as well as the wind speed and direction in the neutral atmosphere. Satellite and debris detection, near-space atmospheric wind field monitoring and early warning, etc. 3.3 Yagi antenna An end-fire type consisting of an active oscillator (usually a folded oscillator), a passive reflector and several passive directors arranged in parallel. antenna.

4 Meteor Radar

4.1 Overview The meteor trails produced by the ablation of meteors entering the atmosphere can scatter radio waves in the medium frequency, high frequency, very high frequency and ultra-high frequency bands. The meteor radar involved in the document operates in the 25 MHz to 65 MHz frequency band, uses meteor trails as the main tracer, and adopts a wide beam
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