Cloud native EDA tools & pre-optimized hardware platforms
The SmartStart Library, an extensive collection of optical data for commercially available diffusers, reflectors, mold textures, plastics, and glasses, can be licensed for use in LucidShape, LucidShape CAA V5 Based, or LightTools. By leveraging the SmartStart Library, you can significantly enhance your optical design process and achieve more accurate results. Discover the full potential of the SmartStart Library in our blog article.
The latest updates include a new catalog for Nihon Etching micro textures as well as additional optical properties and materials from well-known manufacturers including Mold Tech.
To achieve the most accurate simulation results, we recommend downloading the new quarterly release, and replacing those datasets in your downloaded SmartStart Library with these newly published ones.
To access the SmartStart library updates and installation instructions:
1. Log into SolvNetPlus.
2. Click one of the following links:
If you are not currently licensing the SmartStart Library and would like to learn more, read our datasheet. You can also contact the SmartStart Library team at smartstart_support@synopsys.com.
CODE V example models provide opportunities to explore CODE V’s extensive design and analysis capabilities as you work on practical examples. Get a head start designing your next imaging application with example models in CODE V. We have recently added the following example models to :
This example demonstrates how to use the BSP option for modeling the beam propagation from a nanolaser source. We discuss the beam input parameters and the propagation settings.
This example demonstrates how to use optimization with SN2 and SNS constraints, in order to reduce the tolerance sensitivity.
This example model demonstrates the workflow of how to use Reduce Tolerance Sensitivity merit function (SAB) in Automatic Design.
In this example, we will use TOR to analyze the sensitivity of a singlet lens and determine the tolerance and compensator values.
This example discusses a workflow on how to remove an element from a starting point spherical design by introducing aspheres. The workflow is demonstrated with a mid-wave infrared (MWIR) system, although the technique is not limited to MWIR.
This example introduces an aberration-based design approach. We apply this approach to reduce field-dependent aberrations in an off-axis three-mirror anastigmat system.
This example demonstrates how to prevent aspheric inflection point with optimization. This is achieved with a user-defined function by pushing the inflection point outside of the aperture.
A logo lamp system is used to project a personalized/brand-specific logo. This example demonstrates how to design a collimator lens for an automotive logo lamp.
For a logo lamp system, the projection lens projects the pattern on the mask to a logo on the ground. This example demonstrates how to design a three-element projection lens.
This example demonstrates the workflow of using CODE V to design a pixel headlamp. We will start with the final design from Part I, design with aspheric surfaces, reduce system F/Number, substitute with real glasses, analyze the system for display to roadway performance, and export the design.
To download the new CODE V example models:
Looking for optical design services? Partner with a world-class engineering team that has worked on significant space telescope projects, from the Hubble servicing mission to Webb. We offer services in precision imaging, illumination, photonic design, and complete optical systems. Whether you need full project management or specific expert advice, you'll benefit from our top-tier design expertise, advanced software tools, and practical, cost-effective solutions. Our mission is to deliver high-quality results focused on your success.
Note: Please log into first to view these videos.
13 February 2025
5:00–5:45 p.m. CET (Europe)
8:00–8:45 a.m. PST (North America)
19 February 2025
5:00–5:45 p.m. CET (Europe)
8:00–8:45 a.m. PST (North America)
25 February 2025
4:00–5:00 p.m. CET (Europe)
7:00–8:00 a.m. PST (North America)
11 March 2025
8:00–9:00 a.m. PDT (North America)
4:00–5:00 p.m. CET (Europe)
18 March 2025
10:00-11:00 a.m. PST (North America)
6:00-7:00 p.m. CET (Europe)
26 March 2025
9:00-9:45 a.m. PDT (North America)
5:00-5:45 p.m. CET (Europe)
Note: Please log into first to view these videos.
Note: Please log into first to view these articles.
View knowledge articles, training courses, user group presentations and more on SolvNetPlus. Bookmark these links:
Please note that you must be logged into first before you click on a SolvNetPlus link.
We are always looking for papers that utilize our tools. Have your students published any research in the areas of AR/VR, machine learning, optical design, or photonics? If so, please send us references! Our team of lifelong learners is passionate about following advances in these fields, especially those most relevant to our users.
Thank you for your contributions and for inspiring the community with your work.
Meet us at these upcoming events:
草榴社区 staff at SPIE Photonics West in San Francisco, CA on 28-30 January 2025. We celebrated LightTools' 30th and CODE V's 50th anniversaries with a Happy Hour at the booth.
Missed an enews? View the directory of past enews.