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#Sample zemax file micro lens for downloading archive#
While these auxiliary files will still be stored within a folder hierarchy, the hierarchy can be saved and shared within a single archive file and automatically reproduced when restoring the archive file.
![sample zemax file micro lens for downloading sample zemax file micro lens for downloading](https://www.researchgate.net/profile/Lionel-Chaudet/publication/258812224/figure/fig5/AS:297395154898944@1447915938028/Optimised-relay-optics-and-micro-optics-from-the-MLA-front-to-the-micro-lens-array.png)
The Project Directory allows auxiliary files associated with the OpticStudio design to be stored in the same location as the OpticStudio file. In the 21.3 release, there is support for a new capability called a Project Directory that simplifies sharing and collaborating on the hierarchy of files included in an OpticStudio design. The company has upgraded the way to manage and archive OpticStudio project files. Non-sequential support is also critical in supporting an integrated design workflow between OpticStudio, CAD and finite element analysis (FEA). Non-sequential support for off-axis aspheres, as well as for complex aspheres such as the Q-type asphere added in the 21.2 release, enables the as-built performance of systems using these “modern geometries” to be accurately characterized, allowing engineers to account for the impacts of realistic sources, stray light and opto-mechanics. OpticStudio 21.3 includes native support for off-axis conic aspheric mirrors in non-sequential mode. Zemax has delivered three major product releases in 2021, the first in January (21.1) followed by the May release (21.2) and now the September (21.3) release.
![sample zemax file micro lens for downloading sample zemax file micro lens for downloading](https://www.thorlabs.com/Images/GuideImages/2861_Microlens_Array_3.jpg)
Meanwhile, the Diffraction order of Grid Phase is input with the unit conversion value calculated above:Ĭlick ok to see the following interferogram results, which are consistent with the data on the interferometer.Zemax releases its flagship software, OpticStudio, the OpticStudio STAR Module and OpticsBuilder. The DAT file, as shown in the figure below. In aperture lens editor (STO) phase surface type set to a grid, and properties on the surface - the import TAB in the previously saved data file to import, in this case for the test. Zemax unit (radians) = ZYGO measurement unit (mm) x 2 PI / 0.0006328 = 9924 x (ZYGO measurement unit) In the data file provided by this example, the measured wavelength is 632.8nm, then: Zemax unit (radian) = ZYGO measurement unit (mm) x 2 It should be noted that if the measured data is stored as wavefront data, we need to treat this data file as phase data.The Grid Sag of OpticStudio is in radians.Therefore, the measurement data need to be converted, and the conversion formula is as follows: The screenshot at the beginning of the data file shows that the data format is the same as the Grid Sag data format mentioned in last week's article.The number of data points in XY direction is 732, and since the distance between data points is 0.01344, the diameter of the data file is 9.72mm.Where the first line of the file has a terminal flag (flag) of 0, representing the data unit of mm. DAT file, and to save the file in Zemax root directory "DocumentZemax/ObjectsGrid Files". ZXGRD file, we need in OpticStudio converts the file format. We use ZYGO interferometer provide data as example, ZYGO interferometer generated data file format for company. In this case we use ZYGO interferometer provide data as example, ZYGO interferometer generated data file format for company.