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The LN series of narrow linewidth lasers is renowned for its exceptional characteristics, including high spectral purity, a long coherence length, and minimal phase noise. These lasers are meticulously engineered to deliver a stable and precise light output, making them indispensable for a wide range of sophisticated applications.
In the realm of gravitational wave detection, these lasers play a
crucial role by providing a stable and coherent light source that
is essential for the sensitive instruments used to detect the
minute distortions in spacetime caused by passing gravitational
waves. Their high spectral purity ensures that the measurements are
free from unwanted noise, thereby enhancing the accuracy of the
detection process.
For cold atom physics, the LN series lasers offer an ideal light
source for manipulating and studying atoms at extremely low
temperatures. The long coherence length and low phase noise of
these lasers enable researchers to maintain precise control over
the atomic states, facilitating groundbreaking experiments in
quantum mechanics and precision measurements.
Coherent optical communications also benefit greatly from the use
of these narrow linewidth lasers. The high spectral purity ensures
that the optical signals remain clear and distinct over long
distances, reducing the error rate and increasing the overall
efficiency of data transmission. This is particularly important in
modern telecommunications, where the demand for high-speed and
reliable data transfer is ever-growing.
Optical precision measurements, such as those required in metrology
and materials science, rely heavily on the consistent and accurate
output of narrow linewidth lasers. The minimal phase noise and long
coherence length of the LN series allow for extremely precise
measurements of physical quantities, enabling advancements in
fields such as nanotechnology and semiconductor manufacturing.
Lastly, in the field of microwave photonic signal processing, these
lasers are instrumental in generating stable microwave.
Product code | LN1000 | LN1200 |
Wavelength(nm) | 1064 | 532 (Including iodine stabilizing system) |
Average Power (W) | 2 | 0.01 (Maximum to 0.05, Customization required) |
Power Stability (measured by Standard Deviation) | < 0.1% | < 1% |
Beam Divergence (mrad) | 1.2 @ 3mm Beam Waist | 2.3 @ 3mm Beam Waist |
Beam Quality | M2 < 1.2 | M2 < 1.3 |
Linewidth (kHz) | 1 | 3 |
Polarization | Linear | |
Power supply voltage (V) | 220 | |
Warm-up Time (min) | ~ 5 | ~ 10 |
Storage Temperature (°C) | -10 °C ~ 50°C |
The measurement accuracy of high-speed ultra-precision laser interferometers is constrained by the stability of the probing laser's wavelength and the coherence coefficient of the interferometer itself.
When it comes to high-power output, 1064nm narrow linewidth light sources are employed to deliver a powerful output, which in turn enhances the coherence coefficient of the interferometer. This enhancement plays a crucial role in improving the overall measurement accuracy.
Furthermore, the high wavelength stability of these light sources
significantly contributes to the precision of measurements. By
leveraging ultra-narrow linewidth solid-state lasers, the
measurement accuracy of laser rangefinders can be taken to new
heights. This advancement enables the achievement of measurement
precision that surpasses even the atomic scale, all within a range
of 300mm.
This remarkable capability is made possible by the stability and coherence provided by these cutting-edge laser technologies, ensuring that even the most demanding measurement tasks can be performed with unparalleled accuracy and reliability.
●Scientific Research Field (Scientific Research Institutes and Universities)
*High-precision Laser Rangefinder (Michelson Interferometer)
*Laser Frequency Standard Light Source (532 System) (Lead Time: 6
Months, Currently in Prototype Stage)
*Precision Spectral Measurement
●Core Components for Other Instruments (Manufacturers of Laser
Instruments)
*Ultra-narrow Linewidth Laser Seed Source
●Industrial Manufacturing Fields
*Light Source for High-precision
*Laser Rangefinder in Integrated
*Circuits (532 System)
Q1: This is the first time I use it, is it easy to operate?
A1:We will send you a manual and guide video in English, it can
teach you how to operate the spectrometer. Also, our technicians
will offer professional technical operation meetings.
Q2: Can you offer an operation training?
A2: Your technicians can come to our factory for training. Jinsp engineers can go to your place for local support ( installation, training, debugging, maintenance ).
Q3: How to receive the best price in the shortest time?
A3: When you send us an inquiry, please kindly offer details with wavelength, detector, effective pixels, focal length, and so on. We will send you a quotation with details soon to your email.
Q4:If the spectrometer has a problem in my place, what could I do?
A4: The spectrometer has a one-year warranty. If it breaks down,
our technician will figure out what the problem may be, according
to the client's feedback. We can repair for free within one year
warranty.
Q5: What about quality assurance?
A5:We have a quality inspection team. All goods will go through
quality inspection before shipment. We can send you pictures for
inspection.