Arrayed Waveguide Gratings
Author: the photonics expert Dr. Rüdiger Paschotta (RP)
Acronym: AWG
Definition: optical filter or multiplexer devices based on arrays of waveguides
- optical elements
- optical filters
- interference filters
- dichroic mirrors
- rugate filters
- arrayed waveguide gratings
- (more topics)
- optical filters
Related: optical filterswavelength division multiplexingastrophotonics
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DOI: 10.61835/1da Cite the article: BibTex BibLaTex plain textHTML Link to this page! LinkedIn
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What are Arrayed Waveguide Gratings?
An arrayed waveguide grating is a (typically fiber-coupled) device which can separate or combine signals with different wavelengths. It is usually built as part of a planar lightwave circuit (photonic integrated circuit), where the light coming from an input fiber first enters a multimode waveguide section, then propagates through several single-mode waveguides to a second multimode section, and finally into the output ports. Wavelength filtering is based on an interference effect and the different optical path lengths in the single-mode waveguides: any frequency component of the input propagates through all single-mode waveguides, and the output in any channel results from the superposition (interference) of all these contributions. The wavelength-dependent phase shifts lead to a wavelength-dependent overall throughput for any combination of an input port and an output port.
Particularly for AWGs with large numbers of channels, a high precision of the fabrication is required for achieving a low channel cross-talk.
AWGs can be realized with different material systems, e.g. based on fused silica (SiO2), indium phosphide (InP), or silicon (Si).
Applications
Communications
Arrayed waveguide gratings are mainly applied in optical fiber communication systems, in particular in those based on multi-channel transmission with wavelength division multiplexing (WDM), where individual wavelength channels must be combined or separated. They can be part of more complex photonic integrated circuits, functioning e.g. as WDM data transmitters. An arrayed waveguide grating may also be used for separating the lines in the optical spectrum of a supercontinuum source, or in a pulse shaper for ultrashort pulses.
Spectrographs in Astrophotonics
Compact and rugged spectrographs can be produced based on arrayed waveguide gratings. These are particularly interesting in astrophotonics, when a substantial number of spectrographs is required, so that compactness matters.
Technical Issues
Spectral Passband Shapes
The spectral transmission profile of an AWG channel is an important design parameter. Two common types are distinguished:
- Gaussian passband: This profile generally offers the lowest peak insertion loss but requires precise alignment of the signal wavelength to the channel center. It is suitable for systems with very stable laser sources.
- Flat-top passband: This profile provides a wider spectral window with nearly constant transmission, making the system more tolerant to laser wavelength drifts and chromatic dispersion effects. However, achieving a flat-top profile typically incurs a slightly higher insertion loss compared to Gaussian designs.
Temperature Dependence and Athermalization
The refractive index of common waveguide materials like silica changes with temperature, causing a shift in the central wavelengths of the filter channels.
- Standard (thermal) AWGs: These rely on active temperature control (using heaters or thermoelectric coolers) to stabilize the device temperature and thus the wavelength grid. This requires electrical power and control electronics.
- Athermal AWGs: These are designed with passive temperature compensation techniques — such as using silicone adhesives with negative thermo-optic coefficients or compliant mechanical packaging that adjusts physical path lengths to counteract refractive index changes. Athermal AWGs operate reliably over wide temperature ranges (e.g. −40 °C to +85 °C) without power consumption, making them ideal for outside plant applications.
Frequently Asked Questions
This FAQ section was generated with AI based on the article content and has been reviewed by the article’s author (RP).
What is an arrayed waveguide grating?
An arrayed waveguide grating (AWG) is a device, typically built as a planar lightwave circuit, that can separate or combine optical signals of different wavelengths. It is mainly used in optical fiber communication systems.
How does an arrayed waveguide grating work?
An AWG works based on interference. Light is split into an array of waveguides, each with a slightly different path length. The resulting wavelength-dependent phase shifts cause different wavelengths to interfere constructively at different output ports, thus separating them.
What are the main applications of arrayed waveguide gratings?
AWGs are primarily used in wavelength division multiplexing (WDM) systems for combining or separating wavelength channels. They also serve as compact spectrographs, for example in astrophotonics, or are used within pulse shapers.
What materials are used for making AWGs?
Arrayed waveguide gratings can be fabricated from different materials, most commonly fused silica (SiO2), indium phosphide (InP), or silicon (Si).
Suppliers
The RP Photonics Buyer's Guide contains 11 suppliers for arrayed waveguide gratings.
Bibliography
| [1] | C. Dragone, “An N × N optical multiplexer using a planar arrangement of two star couplers”, IEEE Photon. Technol. Lett. 3 (9), 812 (1991); doi:10.1109/68.84502 |
| [2] | S. Chandrasekhar et al., “Monolithic eight-wavelength demultiplexed receiver for dense WDM applications”, IEEE Photon. Technol. Lett. 7 (11), 1342 (1995); doi:10.1109/68.473492 |
| [3] | H. Ehlers et al., “Optoelectronic packaging of arrayed-waveguide grating modules and their environmental stability tests”, Optical Fiber Technol. 6, 344 (2000); doi:10.1006/ofte.2000.0341 |
| [4] | P. Gatkine et al., “Arrayed waveguide grating spectrometers for astronomical applications: new results”, Opt. Expr. 25 (15), 17918 (2017); doi:10.1364/oe.25.017918 |
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