An Integrated Millimeter-Wave Satellite Radiometer Working at Room-Temperature with High Photon Conversion Efficiency.

high photon conversion efficiency millimeter-wave radiation optoelectronic upconversion radiometers room-temperature receivers satellite earth observation whispering gallery mode (WGM) resonators

Journal

Sensors (Basel, Switzerland)
ISSN: 1424-8220
Titre abrégé: Sensors (Basel)
Pays: Switzerland
ID NLM: 101204366

Informations de publication

Date de publication:
21 Mar 2022
Historique:
received: 18 02 2022
revised: 10 03 2022
accepted: 17 03 2022
entrez: 26 3 2022
pubmed: 27 3 2022
medline: 27 3 2022
Statut: epublish

Résumé

In this work, the design of an integrated 183GHz radiometer frontend for earth observation applications on satellites is presented. By means of the efficient electro-optic modulation of a laser pump with the observed millimeter-wave signal followed by the detection of the generated optical sideband, a room-temperature low-noise receiver frontend alternative to conventional Low Noise Amplifiers (LNAs) or Schottky mixers is proposed. Efficient millimeter-wave to 1550 nm upconversion is realized via a nonlinear optical process in a triply resonant high-Q Lithium Niobate (LN) Whispering Gallery Mode (WGM) resonator. By engineering a micromachined millimeter-wave cavity that maximizes the overlap with the optical modes while guaranteeing phase matching, the system has a predicted normalized photon-conversion efficiency ≈10-1 per mW pump power, surpassing the state-of-the-art by around three orders of magnitude at millimeter-wave frequencies. A piezo-driven millimeter-wave tuning mechanism is designed to compensate for the fabrication and assembly tolerances and reduces the complexity of the manufacturing process.

Identifiants

pubmed: 35336571
pii: s22062400
doi: 10.3390/s22062400
pmc: PMC8953225
pii:
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Subventions

Organisme : Comunidad de Madrid MARTINLARA - CM
ID : P2018/NMT-4333
Organisme : Agencia Estatal de Investigacion
ID : PID2019-109984RB-C41
Organisme : RTC2017-6394-7
ID : RTC2017-6394-7
Organisme : Fundacion SENER (REFTA)
ID : Fundacion SENER (REFTA)

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Auteurs

Kerlos Atia Abdalmalak (KA)

Signal Theory and Communications Department, Carlos III University of Madrid, 28903 Madrid, Spain.
Electrical Engineering Department, Aswan University, Aswan 81542, Egypt.

Gabriel Santamaria Botello (GS)

Electrical, Computer, and Energy Engineering Department, University of Colorado, Boulder, CO 80309, USA.

Mallika Irene Suresh (MI)

Department of Physics, University of Otago, Dunedin 3016, New Zealand.

Enderson Falcón-Gómez (E)

Signal Theory and Communications Department, Carlos III University of Madrid, 28903 Madrid, Spain.

Alejandro Rivera Lavado (AR)

Yebes Observatory, National Geographic Institute of Spain, 19141 Guadalajara, Spain.

Luis Enrique García-Muñoz (LE)

Signal Theory and Communications Department, Carlos III University of Madrid, 28903 Madrid, Spain.

Classifications MeSH