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LUNA-ST High-Stability Miniature Fiber Optic Spectrometer

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Brand LuQi Technologies
Origin Anhui, China
Manufacturer Type OEM/ODM Producer
Origin Category Domestic (China)
Model LUNA-ST
Pricing Upon Request
Detector Type Linear CCD Array
Spectral Range 350–1100 nm
Optical Resolution (FWHM) 0.39–6.6 nm
Signal-to-Noise Ratio 300:1 (full signal)
Dynamic Range 1300:1 (single acquisition)
Stray Light <1%
Focal Ratio f/4
Slit Options 10 / 25 / 50 / 75 / 100 µm
Integration Time 1 ms – 10 s
Linearity ≥0.998
A/D Resolution 16-bit
Pixel Count 2048 × 1
Pixel Size 14 µm × 56 µm
Optical Design Crossed Czerny-Turner
Weight 460 g
Interfaces USB 2.0 Type-B, Digital I/O, SMA905 fiber port
OS Compatibility 32/64-bit Windows 7/10/11

Overview

The LUNA-ST High-Stability Miniature Fiber Optic Spectrometer is an engineered solution for embedded and portable spectral measurement applications requiring robust optical performance in a compact form factor. Based on the crossed Czerny-Turner optical architecture with an f/4 focal ratio, the LUNA-ST delivers high wavelength fidelity and minimal optical aberration across its full 350–1100 nm spectral range. Its core measurement principle relies on dispersion of incident light via a ruled or holographic grating, followed by spatially resolved detection using a 2048-pixel linear CCD array with 14 µm pixel pitch. Designed for integration into OEM analytical platforms—including handheld colorimeters, inline process monitors, environmental sensors, and portable photometric systems—the LUNA-ST prioritizes thermal and mechanical stability to ensure repeatability over extended operation cycles. Unlike benchtop spectrometers, the LUNA-ST achieves sub-1% stray light performance through optimized internal baffling and precision-aligned optical path geometry—critical for quantitative reflectance, absorbance, and emission measurements where background suppression directly impacts detection limits.

Key Features

  • Compact footprint (125 × 85 × 40 mm) and lightweight design (460 g), enabling seamless integration into space-constrained instrumentation
  • Thermally stabilized optical bench and low-drift electronics supporting long-term measurement consistency under ambient temperature fluctuations
  • Selectable entrance slits (10–100 µm) allowing user-tuned trade-offs between resolution and throughput without hardware modification
  • USB 2.0 Type-B interface with native support for isochronous data streaming at up to 1 kHz frame rate (dependent on integration time and ROI configuration)
  • Digital I/O lines for hardware-triggered acquisition, external shutter control, and synchronization across multi-spectrometer arrays
  • Full spectral stitching capability: multiple LUNA-ST units can be operated in master-slave mode with synchronized triggering and timestamp-aligned data capture
  • Factory-calibrated wavelength and intensity response with NIST-traceable reference lamp validation documentation available upon request

Sample Compatibility & Compliance

The LUNA-ST interfaces exclusively via SMA905 fiber optic connectors, supporting standard 200–600 µm core diameter fibers with numerical apertures up to 0.22. It is compatible with common illumination sources including tungsten-halogen, deuterium, LED arrays, and pulsed lasers (with appropriate attenuation). The spectrometer meets CE marking requirements for electromagnetic compatibility (EN 61326-1) and safety (EN 61010-1). While not certified for intrinsic safety or hazardous area deployment, its low-power consumption (<2.5 W) and absence of high-voltage components make it suitable for Class I, Division 2 environments when housed in appropriate enclosures. For regulated industries, raw spectral data export supports audit-ready formats (CSV, HDF5) and optional firmware-level timestamping compliant with GLP/GMP documentation workflows. Though not FDA 21 CFR Part 11-certified out-of-the-box, the device’s deterministic trigger behavior and immutable metadata logging enable validation-ready integration into compliant analytical systems.

Software & Data Management

LuQi provides the LUNA Control Suite—a native Windows application supporting real-time spectrum visualization, batch acquisition, dark/baseline correction, and mathematical operations (e.g., derivative, smoothing, peak integration). SDKs are available for C/C++, Python (via ctypes), and LabVIEW, exposing low-level register access, programmable gain control, and hardware synchronization registers. All acquired spectra include embedded metadata: UTC timestamp, integration time, detector temperature (monitored via onboard thermistor), slit ID, and calibration file hash. Data files support optional password-protected encryption and SHA-256 checksum generation for integrity verification. Export options include ASCII (CSV), binary (IEEE 754 float32), and hierarchical HDF5—facilitating direct ingestion into MATLAB, Python (NumPy/Pandas), or LIMS platforms.

Applications

  • Portable colorimetry and spectral reflectance analysis in textile, paint, and plastic quality control
  • In-line monitoring of LED phosphor conversion efficiency and binning during manufacturing
  • Environmental field spectroscopy for water quality assessment (e.g., chlorophyll-a, dissolved organic carbon estimation)
  • UV-Vis absorption kinetics in microfluidic reaction chambers
  • Calibration transfer between reference and field-deployed instruments using spectral matching algorithms
  • Multi-channel fluorescence lifetime excitation profiling via gated acquisition with external TTL triggers

FAQ

What slit width should I select for optimal resolution in the visible range?
For nominal 0.39 nm resolution at 550 nm, a 10 µm slit is recommended; however, this reduces signal throughput by ~50% compared to a 25 µm slit. Trade-off analysis should consider your source brightness and required SNR.
Can the LUNA-ST operate in continuous scanning mode with external clock input?
Yes—digital I/O supports TTL-compatible external trigger frequencies from 1 Hz to 10 kHz, with jitter <100 ns. Frame-to-frame timing is hardware-gated and independent of USB latency.
Is spectral calibration traceable to NIST standards?
Each unit ships with a factory calibration certificate referencing traceable tungsten-halogen and mercury-argon line sources. Full calibration datasets (wavelength, linearity, sensitivity) are provided in machine-readable format.
How does the LUNA-ST maintain stability during temperature cycling?
The optical bench uses low-CTE aluminum alloy, and critical components (grating mount, detector carrier) are secured with athermal kinematic design. Internal temperature is monitored continuously, and optional software-based thermal drift compensation is available.
Does the device support OEM firmware customization?
Yes—LuQi offers contract firmware development for proprietary protocols, custom I/O logic, or accelerated acquisition pipelines, subject to NDA and minimum order volume.

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