LightSmyth Technologies is proud to introduce monolithic, single-substrate, silicon grating arrays (Figure 1) that uniquely provide continuous high-resolution access to optical bandwidths beyond that achievable with a single grating. No moving parts are required. LightSmyth monolithic grating arrays are consistent with single-shot data acquisition for many broadband applications, e.g. laser-induced breakdown spectroscopy and can help reduce system component numbers dramatically. Each array consists of multiple primary gratings – all formed coherently on a single substrate. The primary gratings have contiguous, slightly overlapping active spectral ranges. Additionally, auxiliary gratings at the top and bottom of the substrate produce optical outputs used for the straightforward calibration of the output field using a single reference wavelength such as a HeNe laser.
In Figure 2, a grating array is shown in a simple spectrometer arrangement. A two-dimensional detector array is used to record output of the grating array. Figure 3 shows a schematic of the grating array output as seen on the 2D detector array when illuminated by white light and a co-propagating HeNe laser. Each near horizontal line comprises output of one of the four primary gratings and corresponds to the spectral range indicated. Also shown as red dots are the calibration reference marks produced by the 6 auxiliary gratings when exposed to HeNe light. Details of the device operation and design are described further in an application note.
The six small gratings at the top and bottom of the array (see Figure 1) provide markers for calibrating the spectral output as well as assisting in system alignment. The calibration marks, here for HeNe illumination, are shown schematically in Figure 4. The calibration marks provide two principal functions: First, they indicate the beginning and end points of the calibrated portion of the primary grating output. They thus allow the user to calibrate the wavelength as a function of position along each of the primary gratings’ dispersion lines - note that the wavelength range denoted by the calibration spots is independent of the grating input angle, making the LightSmyth grating array extraordinarily versatile with respect to possible device layouts. Second, the auxiliary gratings aid in system alignment. When the detector surface is properly positioned in the focal plane of the post-array focusing mirror, the two pairs of alignment marks are designed to coincide, indicating proper far-field operation. The two center marks enable correct horizontal alignment of array and detector surface.
More technical details of the LightSmyth Monolithic grating array can be found in the following application note.
Silicon substrate has a thickness of 0.73mm. Substrate height and width tolerances are ± 0.3 mm. Grating substrate: single crystal silicon. Grating coating: aluminum (other coating types are available at additional charge).
|Primary Grating||Calibration Markers 1||Line/mm||Size||Part Number||Price first 99 units 2,3||Unit price 100+|
|1||381, 522 nm||1788||12.5mm x 12.5mm||SAG-1212A-Al||$96.00 ea.||$25.00 ea.|
|2||509, 696 nm||1341|
|3||683, 935 nm||998|
|4||929, 1271 nm||734|
|1The calibration markers listed are produced by a HeNe laser incident on the small calibration gratings. Use of a different calibration light source having a different wavelength will produce markers (see Fig. 4) coinciding with different values of the dispersed spectra of the four primary gratings. Using a common input angle for calibration light and signal, the calibration marks delineate spectral output ranges of the primary gratings that are independent of grating input angle.|
|2 For orders with the total product value below $250.00, a handling charge of $75.00 will be added.|
|3 Academic discounts are available for eligible institutions. To determine eligibility complete an account application procedure.|