Jose Saiz

Mr. Jose Saiz

Electronics, Universidad de Las Palmas de Gran Canaria, Las Palmas de Gran Canaria, Spain
orcid

Research Focus & Metrics

Academic Career Length

5Years (2022-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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2 December 2022 in Sensors
Verified
Journal Article
Open access
PDF file
IMIrene Merino-Fernandez
Irene Merino-Fernandez
SKSunil Lalchand Khemchandani
Sunil Lalchand Khemchandani
FSFrancisco Javier del Pino Suárez
Francisco Javier del Pino Suárez
JSJose Saiz
Jose Saiz
Nowadays, mega-constellations of Low Earth Orbit (LEO) satellites have become increasingly important to provide high-performance Internet access with global coverage. This paper provides an updated comparison of four of the largest LEO mega-constellations: Telesat, SpaceX, OneWeb and Amazon. It describes the gateway design workflow from the patch antenna to phased array analysis. Patch antennas are developed for both transmission and reception after a thorough examination of the four systems. The results of electromagnetic simulation using Advanced Design Software (ADS) Momentum are shown, including their radiation pattern. Finally, a model of the gateway phased array using SystemVue is obtained using hexagonal, circular, and square arrays. According to the required effective isotropic radiated power (EIRP) and gain, the antenna sizes for the four constellations are estimated. As an example, for SpaceX constellation, a reception antenna with 8910 radiating elements using a hexagonal distribution with a gain of 46.9 dB and a sensitivity of −113.1 dBm was obtained.

31 May 2023 in Micromachines
Verified
Journal Article
Open access
PDF file
FSFrancisco Javier del Pino Suárez
Francisco Javier del Pino Suárez
SKSunil Lalchand Khemchandani
Sunil Lalchand Khemchandani
MMMario San Miguel Montesdeoca
Mario San Miguel Montesdeoca
SMSergio Mateos-Angulo
Sergio Mateos-Angulo
DMDaniel Mayor-Duarte
Daniel Mayor-Duarte
DGDavid Galante-Sempere
David Galante-Sempere
This paper presents a novel and compact vector modulator (VM) architecture implemented in 130 nm SiGe BiCMOS technology. The design is suitable for use in receive phased arrays for the gateways of major low Earth orbit (LEO) constellations that operate in the 17.8 to 20.2 GHz frequency range. The proposed architecture uses four variable gain amplifiers (VGA) that are active at any given time and are switched to generate the four quadrants. Compared to conventional architectures, this structure is more compact and produces double the output amplitude. The design offers 6-bit phase control for 360°, and the total root mean square (RMS) phase and gain errors are 2.36° and 1.46 dB, respectively. The design occupies an area of 1309.4 μm × 1783.8 μm (including pads).