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Antenna Low Noise Amplifier for GNSS

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21230%2F15%3A00237902" target="_blank" >RIV/68407700:21230/15:00237902 - isvavai.cz</a>

  • Result on the web

  • DOI - Digital Object Identifier

Alternative languages

  • Result language

    angličtina

  • Original language name

    Antenna Low Noise Amplifier for GNSS

  • Original language description

    A wideband low noise amplifier (LNA) was developed to receive signals of all the fundamental satellite navigation systems (GPS, GLONASS, Galileo, and COMPASS). The low noise pHEMT ATF-54143 from Avago Technologies with excellent noise characteristics was used as the basic building block. The amplifier is designed to be placed very close to the receiving antenna, and there are two SMA connectors used for the connection. The input one is used to connect the receiving antenna to be further connected with the amplifier through a coaxial cable which is as short as possible in order to emphasize its excellent noise characteristics. The second one serves as an output of the amplified signal and an input of DC voltage. The intrinsic amplifier is based on the substrate Isola 410, used for high frequency circuits. The entire amplifier is constructed of SMD components which comprise, besides the transistor itself, the matching and power supply circuits. A sophisticated method of the amplifier design was suggested based on multiobjective optimization. A substantial original improvement of the standard optimization method was used to satisfy a uniform coverage of Pareto front. The suggested modified algorithm for the multiobjective optimization as well as extraordinary precise circuit modeling methodology were published in the paper “Precise Characterization and Multiobjective Optimization of Low Noise Amplifiers” in the Radioengineering journal with the WoS IF=0.653. After the complex circuit design, the s21 parameter ranged from of 15 to 25 dB, and the s11 and s22 parameters were lesser than -10 dB in the range of 0.5 GHz to 3.2 GHz. The noise figure was lesser than 1dB in the range from 0.8 to 2.9 GHz, and it was near 0.5 dB at the frequencies where the main satellite navigation systems work. The measured third-order intercept point was 27.5 dBm after the multiobjective optimization. Finally, the stability of the amplifier was carefully checked.

  • Czech name

  • Czech description

Classification

  • Type

    G<sub>funk</sub> - Functional sample

  • CEP classification

    JA - Electronics and optoelectronics

  • OECD FORD branch

Result continuities

  • Project

    <a href="/en/project/TE01020186" target="_blank" >TE01020186: Integrated Satellite and Terrestrial Navigation Technologies Centre</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2015

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Internal product ID

    13137LNA201501

  • Numerical identification

  • Technical parameters

    low noise pHEMT ATF-54143, s21 15-25 dB, range of 0.5 GHz to 3.2 GHz, NF 0.5 dB in L1 band. Výsledek využívá příjemce pro výzkum

  • Economical parameters

    Cena zařízení je přibližně 6000 Kč, cca 60% v porovnání s komerčními LNA.

  • Application category by cost

  • Owner IČO

    68407700

  • Owner name

    ČVUT FEL, Katedra radioelektroniky

  • Owner country

    CZ - CZECH REPUBLIC

  • Usage type

    P - Využití výsledku jiným subjektem je v některých případech možné bez nabytí licence

  • Licence fee requirement

    N - Poskytovatel licence na výsledek nepožaduje licenční poplatek

  • Web page