VGOS radio telescopes enable observations in the range of 2-14 GHz and are much more receptive for unwanted radio frequency interference. Some space-borne transmitters may cause detrimental radiation to VGOS receivers. The registration of new VGOS sites at ITU is important to obtain administrative protection. This may help to avoid direct illumination by strong radars, as well as provide protection in the dedicated RAS bands from lower-level interference that degrades system sensitivity. This article introduces the risk of damage and explains the registration procedure

How to register a VGOS radio telescope at ITU and why it is important

TORNATORE, VINCENZA;
2016-01-01

Abstract

VGOS radio telescopes enable observations in the range of 2-14 GHz and are much more receptive for unwanted radio frequency interference. Some space-borne transmitters may cause detrimental radiation to VGOS receivers. The registration of new VGOS sites at ITU is important to obtain administrative protection. This may help to avoid direct illumination by strong radars, as well as provide protection in the dedicated RAS bands from lower-level interference that degrades system sensitivity. This article introduces the risk of damage and explains the registration procedure
2016
New Horizons with VGOS
VGOS, spectrum management, RFI, SAR radar, ITU registration
File in questo prodotto:
File Dimensione Formato  
2016_GM_SA.pdf

accesso aperto

: Publisher’s version
Dimensione 128.35 kB
Formato Adobe PDF
128.35 kB Adobe PDF Visualizza/Apri

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11311/1017432
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus ND
  • ???jsp.display-item.citation.isi??? ND
social impact