Analisys of noise-injection networks for interferometric-radiometer calibration

The spatial resolution of current space-borne Earth observation radiometers is limited by the physical antenna aperture. This is especially critical at L-band, which exhibits high sensitivity to soil moisture and sea surface salinity. Interferometric radiometers (InR's) are currently being stud...

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Detalhes bibliográficos
Autores: Corbella Sanahuja, Ignasi|||0000-0001-5598-7955, Camps Carmona, Adriano José|||0000-0002-9514-4992, Torres Torres, Francisco|||0000-0003-1160-6350, Bará Temes, Francisco Javier
Formato: artículo
Fecha de publicación:2000
País:España
Recursos:Universitat Politècnica de Catalunya (UPC)
Repositorio:UPCommons. Portal del coneixement obert de la UPC
Idioma:inglés
OAI Identifier:oai:upcommons.upc.edu:2117/1461
Acesso em linha:https://hdl.handle.net/2117/1461
Access Level:acceso abierto
Palavra-chave:Interferometry
Radiation Measurement
Calibration
S-parameters
calibration
oceanographic techniques
radiometers
radiowave interferometry
remote sensing
soil
L-band
distributed noise injection
front-end reradiated noise
interferometric-radiometer calibration
isolated power splitters
network losses
noise-injection networks
optimum circuit topologies
physical antenna aperture
physical temperature
receiving channels
Sea surface salinity
soil moisture
space-borne Earth observation radiometers
spatial resolution
Interferometria
Radiometria
Calibratge
Àrees temàtiques de la UPC::Enginyeria de la telecomunicació::Radiocomunicació i exploració electromagnètica::Teledetecció
Descrição
Resumo:The spatial resolution of current space-borne Earth observation radiometers is limited by the physical antenna aperture. This is especially critical at L-band, which exhibits high sensitivity to soil moisture and sea surface salinity. Interferometric radiometers (InR's) are currently being studied by several space agencies as a feasible alternative to overcome this problem. However, their calibration is a crucial issue since most techniques inherited from radio astronomy cannot be directly applied. Due to the large number of receiving channels, calibration techniques based on centralized noise injection from a single noise source will require a large and stable distribution network, which is technically very complex and unacceptable from the point-of-view of mass and volume. Procedures based on distributed noise injection from a set of noise sources through smaller distribution networks have been recently proposed by the authors as an alternative to alleviate these technological problems. In this paper, the analysis of these networks, the impact of the noise generated by the network losses on the calibration, and the impact of front-end reradiated noise are analyzed. Finally, the optimum circuit topologies and tolerances to which these networks have to be characterized in order to achieve the required calibration are derived. These configurations are formed by cascading basic 1:2 and 1:3 isolated power splitters. Isolators at receiver inputs have to be included in order to minimize offsets originating from the correlation of reradiation of receiver noise. It has been found that, in order to satisfy the calibration requirements of InR's, the S-parameters of the ensemble noise-injection network plus isolators have to be known to within 0.025-0.050 dB in amplitude and 0.5° in phase, and their physical temperature known to within 0.5°C.