Technical specification for radio telescope electromagnetic environment protection (English Version)
With the rapid development of radio technology, radio telescopes are facing increasing threats of electromagnetic interference. The formulation of GB/T 42557-2023 aims to provide a scientific and technical basis for radio astronomical observations and ensure the accuracy and reliability of observation data.
| Standard chapters | Main content | Differences from other electromagnetic environment standards |
|---|---|---|
| Radio telescope | Applicable to site selection, construction, operation and maintenance stages | Designed for interference protection requirements for high-sensitivity astronomical observations |
| 4.1 Protection threshold | Harmful interference threshold values are specified separately for continuous spectrum and spectral line observation modes | Differentiated protection standards are set for different business types |
class='instrument'>The technical requirements for electromagnetic environment protection of radio telescopes mainly involve:
During the site selection stage, a radio observatory conducted electromagnetic environment measurements in strict accordance with standard requirements to ensure that the measurement equipment complies with the provisions of GB/T6113.101, and optimized the antenna polarization mode and gain. By implementing geographical isolation measures, interference was successfully reduced to the lowest level.
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