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
Cite the article: BibTex BibLaTex plain textHTML Link to this page! LinkedIn
Content quality and neutrality are maintained according to our editorial policy.
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.
In WDM systems, AWGs commonly operate on the standard ITU grid with channel spacings of 100 GHz (~0.8 nm) or 50 GHz (~0.4 nm), with typical channel counts of 40, 48, 80 or 96. They also serve in optical add-drop multiplexers (OADMs), where specific wavelength channels are extracted or inserted at network nodes without conversion to the electrical domain.
Optical Sensing Interrogators
AWGs are used as optical sensing interrogators, mapping the wavelength shifts of fiber Bragg gratings (FBG) sensors onto spatial output ports for high-speed parallel readout.
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
Channel Cross-talk
A key performance metric is the channel cross-talk (isolation), i.e. the suppression of unwanted wavelength contributions in a given output channel. One distinguishes adjacent-channel cross-talk, which limits how densely channels can be packed, from non-adjacent (cumulative) cross-talk arising from all other channels combined. High cross-talk degrades the achievable signal-to-noise ratio and bit error rate. Typical specifications are above 25 dB for adjacent channels and above 30 dB for non-adjacent channels.
Insertion Loss and Polarization Dependence
In contrast to cascaded thin-film filters, whose loss scales with channel count, AWGs exhibit a relatively constant insertion loss (typically a few dB) largely independent of the number of channels. Loss uniformity, the spread between the lowest- and highest-loss channels, is important for system link budgeting. Polarization-dependent loss (PDL) is another relevant parameter, since standard single-mode fiber networks do not control the input polarization state.
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.
When selecting an AWG, note that flat-top designs typically incur 2–3 dB higher insertion loss than Gaussian types; the choice depends on source wavelength stability and on whether filters are cascaded. See our Buyer's Guide for arrayed waveguide gratings for more details.
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.
For procurement, the operating temperature range and thermal stabilization type largely determine suitability for indoor versus outdoor deployment, and connector choice (APC preferred to limit back-reflections) matters for system integration. See our Buyer's Guide for arrayed waveguide gratings for more details.
Purchasing
For professional purchasing, our buyer's guide for arrayed waveguide gratings explains additional buyer-oriented technical background and suggests selection criteria: Channel spacing, Number of channels, Passband shape, Insertion loss, Loss uniformity, Channel isolation (crosstalk), Polarization dependent loss (PDL), Thermal stabilization type, Operating temperature range, Fiber connectors. It also lists 11 suppliers of arrayed waveguide gratings. Some of these show their product descriptions as sponsored content:
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).
Questions and Comments from Users
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 |

