LightSmyth 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’s 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.
Calibration/Alignment Features 校准对齐功能
The six small gratings at the top and bottom of the array (reference 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:
Monolithic Silicon Grating Array单片硅阵列光栅
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).
More technical details regarding the monolithic grating array can be found in Application Note: Monolithic Silicon Grating Arrays.
|
Part |
Primary |
Calibration |
Line/mm |
Size |
Price first 99 units 2,3 |
Unit price 100+ |
|
SAG-1212A-Al |
1 |
381, 522 nm |
1788 |
12.5mm |
$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. |
||||||