SearcharxivSearch

arXiv · 2510.25090

Commissioning of the TeraNet Optical Ground Station Network

Abstract

TeraNet is a new three-node OGS network that has been established in Western Australia. The network is built to support a broad range of space missions operating between LEO and the Moon, using both conventional and advanced optical technologies developed at UWA. It is designed to be spacecraft and mission agnostic, able to be adapted for compatibility with spacecraft using a variety of communication and timing protocols. The TN network comprises three ground station nodes, each of which are equipped to support direct-detection, bidirectional optical communication with LEO spacecraft. In addition, each node is focused on the development of a unique advanced optics technology. Specifically: -TN-1 is a 70cm aperture OGS located on the campus of UWA. It uses ultra-sensitive optical detectors and specialised modulation formats to maximise the information recovered from spacecraft at lunar distances. -TN-2 is a 70cm aperture OGS at the Yarragadee Geodetic Observatory 300km North of Perth. It is equipped with a commercial-grade adaptive optics system for efficient single-mode fibre coupling. This enables high-speed coherent communications and ultra-precise coherent timing and positioning between ground and space. -TN-3 is a 43cm aperture mobile OGS node built onto the back of a utility vehicle for rapid, tactical deployment anywhere in the world. It is setup for quantum communication and quantum-assured time transfer and can establish satellite communication links within ten minutes of arriving on site, day or night. In this paper, we report on the results and outcomes of the TN commissioning campaign, including optical communication links with on-orbit spacecraft, the performance of the TN-2 adaptive optics system, the rapid deployment capability of TN-3, remote network operations of all three nodes, and interoperability tests with other OGSs across Australia and New Zealand.

Explore related subjects

Keep this discovery

BibTeXRIS

Sascha Schediwy, Aliesha Aden, Benjamin Dix-Matthews, Alex Frost, Amrita Gill, David Gozzard, Mike Kriele, Andrew Lance, Nicolas Maron, Ayden McCann, Shawn McSorley, Lilani Toms-Hardman, Shane Walsh, Larissa Wiese, Graeme Wren, Randall Carman. 2025-10-29. Commissioning of the TeraNet Optical Ground Station Network. https://arxiv.org/abs/2510.25090

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

Two-step high-accuracy microwave frequency measurement and time-frequency analysis based on optical frequency combs

Broadband microwave frequency measurement and time-frequency analysis are crucial for applications such as electronic warfare. However, when it comes to ultra wideband signal analysis, traditional electronic methods have high analysis accuracy, but intrinsic electronic bottlenecks limit their real-time analysis. Here, we propose and experimentally demonstrate a two-step microwave frequency measurement and time-frequency analysis method based on optical frequency combs. The system first performs coarse frequency localization over the 0-40 GHz range using stimulated-Brillouin-scattering-assisted frequency-to-time mapping (FTTM) and dual-comb channelized reception. The dual-comb is then reapplied for downconverting the signal under test, followed by digital signal processing to achieve high-accuracy unambiguous frequency extraction. Experimental results show that the system achieves mean single-tone frequency measurement errors of less than 10 kHz over 0-40 GHz. We further experimentally measure multi-tone, linearly frequency-modulated, and V-shaped frequency-modulated signals, demonstrating the proposed method's capability for analyzing complex signals.

physics.optics

A Two-Mirror Faceted Projection System for EUV Lithography

We propose an all-reflective two-mirror projection system for extreme ultraviolet (EUV) lithography operating at exposure wavelengths of $13.5$~nm (Mo/Si) and $11.2$~nm (Ru/Be), delivering a fourfold ($4\times$) demagnification of the periodic mask pattern at a numerical aperture approaching unity ($\mathrm{NA}_{\max} \approx 0.993$). In contrast to conventional EUV projection objectives that incorporate 6--10 aspheric mirrors with an overall optical throughput of less than $15\%$, the proposed design redirects each accepted discrete spatial diffraction order scattered by the mask onto the wafer via a dedicated pair of planar mirror facets. The number of reflections is strictly fixed at two for all accepted orders, retaining $50$--$60\%$ of the power leaving the mask in each accepted order. We derive a spatial geometry providing rigorous optical path length equalization across all diffraction orders, thereby removing order-dependent propagation phase shifts. Individually optimized 30-bilayer Bragg multilayer coatings are designed for each facet using the transfer matrix method combined with global evolutionary optimization algorithms. The architecture is generalized to a three-dimensional vector formulation with a two-dimensionally periodic mask. Utilizing inverse lithography technology, Fourier parameterization, and a differentiable electromagnetic modal waveguide solver, we solve the synthesis problem for binary absorber masks (La absorber on a Ru/Be/Sr multilayer mirror). We demonstrate simulated aerial images of sub-10-nm features on the wafer (isolated peaks with a full width at half maximum (FWHM) of approximately $5.4$~nm and line pairs with a critical dimension of $6$~nm) and find that the two peaks remain resolved for the tested wafer defocus values from $0$ to $5$~nm along the $z$-axis.

physics.optics

Antimony for broadband nanophotonics across the ultraviolet, visible and infrared

Semimetal elemental antimony (Sb) nanostructures show great potential for applications where nanophotonic properties play a key role, such as phase-change optical memories, non-linear optical elements, photothermal therapy agents, photodetectors and photocatalysts. However, designing advanced Sb-based photonic devices critically requires an accurate and reliable knowledge of the optical response of bulk and nanoscale Sb. Herein, we report for the first time a fully consistent and accurately measured dielectric function for Sb nanoscale films in a wide spectral range from the ultraviolet to the far infrared (4 - 0.04 eV, i.e. ~ 0.3 - 30 $\mu$m), surpassing previous reports that explored a limited spectral range. It is found that the Sb spectral response is driven exclusively by giant interband transitions in the visible up to mid infrared (4 - 0.4 eV, i.e. ~ 0.3 - 3 $\mu$m), and that their contribution dominates over that of free carriers down to 0.12 eV (i.e. ~ 10 $\mu$m). Such spectral response enables Sb nanostructures to display spectrally selective and tunable nanophotonic resonances. First, we showcase interband plasmonic resonances in the visible-to-near infrared for Sb nanogratings. Second, we report giant refractive index dielectric resonances in the mid infrared for nanostructured Sb/dielectric/metal resonant cavities. These findings open a pathway to optimized planar Sb nanoscale designs enabling a tailored light-matter interaction, which will be useful for integrated data, telecom, medical, optoelectronic and energy conversion devices operating in a broad spectral range.

physics.optics