VGOS radio telescopes enable observations in the range of 2–14 GHz and are much more recep- tive for unwanted radio frequency interference. Some spaceborne transmitters may cause detrimental radia- tion to VGOS receivers. The registration of new VGOS sites at ITU is important for obtaining administrative protection. This may help to avoid direct illumination by strong radars. This paper introduces the risk of dam- age and explains the registration procedure.
Biennial Report (2015-2016) of PMD IVS Analysis Center
V. Tornatore;
2016-01-01
Abstract
VGOS radio telescopes enable observations in the range of 2–14 GHz and are much more recep- tive for unwanted radio frequency interference. Some spaceborne transmitters may cause detrimental radia- tion to VGOS receivers. The registration of new VGOS sites at ITU is important for obtaining administrative protection. This may help to avoid direct illumination by strong radars. This paper introduces the risk of dam- age and explains the registration procedure.File in questo prodotto:
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