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High resolution lineshape spectra and ultra sensitive noise analyzers for narrowband lasers
Linewidth Analyzer
LWA Series
The HighFinesse Linewidth Analyzers are the ultimate high-end instruments for measuring, analyzing and controlling frequency andintensity noise of lasers. The superb sensitivity of these instruments is achieved by combining an interferometric working principle with high-end optical and electronic components.
The main features are:
Frequency noise density, optical lineshape and relative intensity noise (RIN) analysis with evaluation of intrinsic (Lorentzian) and effective (optical) linewidth
Intrinsic (Lorentzian) linewidth measurements down to 350 Hz
Effective (optical) linewidth measurement range down to 1 kHz
Frequency noise density floor down to 5 Hz/√ Hz with a dynamic range of 60 dB between 10 Hz and 10 MHz
RIN measurement down to −150 dB/Hz
Robust against acoustic noise
Error signal generator for further linewidth, frequency noise or RIN reduction
Powerful tool for a detailed analysis of noise sources like servo bumps, frequency drifts, power supply noise and acoustics
Extremely fast analysis: up to real time measurements and evaluation
The laser lightThe laser light is coupled to the input fiber and lead is coupled to the input fiber and lead through an interferometerthrough an interferometer acting as a frequency acting as a frequency discriminator. The transmitted intensity, which is directly discriminator. The transmitted intensity, which is directly proportional to the variations of the input frequency, proportional to the variations of the input frequency, is converted by a photodetectoris converted by a photodetector and our analog elec-and our analog elec-tronicstronics into a voltage signal. This voltage is finally into a voltage signal. This voltage is finally digitized by the Digitizerdigitized by the Digitizer to provide the data for eval- to provide the data for eval- uation on a computeruation on a computer ..
The included software recovers the original frequency The included software recovers the original frequency noise using the precisely known interferometer function.noise using the precisely known interferometer function.
The recovered timeseries of the frequency deviations The recovered timeseries of the frequency deviations is now the basic dataset allowing to calculate easily is now the basic dataset allowing to calculate easily the frequency noise density spectrum and the optical the frequency noise density spectrum and the optical lineshape spectrum.lineshape spectrum.
The user can also export the timeseries data in order The user can also export the timeseries data in order to perform custom evaluation methods such as Allan to perform custom evaluation methods such as Allan deviation or coherence time analysis.deviation or coherence time analysis.
LaserLaser
Frequency Frequency discriminator discriminator (interferometer)(interferometer)
PhotodetectorPhotodetector
Analog electronics Analog electronics
Data acquisition systemData acquisition system
ComputerComputer
00010000 00100011 1111101111110011 10100011 1111001110010001 11100011 1001000110010111 10100011 1111001111010100 00010000 1111101111110011 10100011 1111001110010001 11100011 1001000110010111 10100011 1111001100010000 00100011 1111101111110011 10100011 11110011
Frequencynoise
Δν
Intensitynoise
Δ I
Δν
ΔI
Δν[Hz]
t[s]
S N [H
z/√H
z]
F (Δν(t
)) × F*(Δ
ν(t))
F (ei2π ∫ Δ
ν(t)d
t ) × F*(e
i2π ∫ Δν(t
)dt )
f [Hz]
Frequency noise density Lineshape (optical spectrum)
Frequencydeviations
Δν [Hz]
L [d
B/H
z]
User defined evaluation:User defined evaluation:
Allan deviation Allan deviation Coherence time Coherence time … …
ΔU
Δν
Voltagenoise
Δ U
Typical Data and Linewidth Evaluation
Timeseries Frequency noise density spectrum
Comparison: Discriminator- vs. Delay-line-technique
β-separation line
Area of frequency noise above β-separation line → Integration for effective (optical) linewidth estimation
White noise level → Noise density level directly proportional to intrinsic (Lorentzian) linewidth
Linefit to optical spectrum → Full width at half maximum = effective (optical) linewidth
DBR laser ECDL @ 1550 nm Fiber laser
LWA-1k 1550Typical frequency noise density spectra
LWA-1k 1550 Typical lineshape spectra
Principle
Limits
Basic data
Frequency noise density
Lineshape
Linewidth evaluation
Direct frequency noise to intensity conversion
Steepness of discriminator-function
Frequency deviations in time
By a Fourier analysis of the frequency deviations
By a Fourier analysis of the calculated electric fields
Effective (optical) and intrinsic (Lorentzian) linewidths directly accessible via frequenvy density noise spectrum or lineshape spectrum
Discriminator (e.g. LWA-1k)
Optical delayed superposition by different path lengths
Length of delay path
Spectrum of beat note (convolution of original spectrum)
Not possible without additional techniques
Lorentzian part (intrinsic linewidth) of the lineshape
Only the Lorentzian part of the linewidth is accessible, because the frequency noise is high- passed by the delay line
Delay-line approach
Freq
uenc
y no
ise
dens
ity
[Hz/
√Hz]
Frequency [Hz]
101
10 –1
10 0
101
102
103
104
102 103 104 10 5 10 6 107
Beside the frequency discrimination approach, homo- and heterodyne delay-line techniques are commonly used for linewidth determination. However, using optical delay lines can lead to complex spectra with non-trivial evaluation needs due to the technique inherent loss of information.
Time [s]
Freq
uenc
y de
viat
ions
[Hz]
0.5 6
0
0.5 -6
1.0 -6
1.0 6
0.00 0.02 0.04 0.06 0.08 0.10
Pow
wer
den
sity
[dB/
Hz]
Frequency [Hz]
10 –5
10 –4
10 –3
10 –2
10 –1
10 0
0 1 M–3 M 2 M–2 M 3 M–1 M
Optical lineshape spectrum
Frequency noise density spectrum from LWA-1k
The delay lines are not long enough to resolve the ultra low frequency noise of the fiber laser.
The delay lines filter out significant parts of the frequency noise of the Ti:Sapphire laser.
Calculated spectra from delayed super-position of electric fields
3.5 µs delay; 20 µs delay; LWA-1k lineshape (one side)
Fiber laser @ 1550 nm
The measurement results of a homodyne delay line detector can be simulated using the time-frequency deviation data of the LWA. The graphs below show this comparison for a Ti:Sapphire (813 nm) and a fiber laser (1550 nm) for two
different lengths of the delay line ( 3.5 µs, 20 µs). The evaluated data (one side of optical spectrum) of the LWA-1k is shown as black curve.
Ti:Sapphire @ 813 nm
1 1510 0.5 85
Technical Data
Frequency Noise Specification
Lineshape Specifications
Miscellaneous
Digitizer Module
Product Overview
Unit
Wavelength range
Input power range (@typical wavelength)
Required input power stability
Laser type
Input type
Maximum frequency stroke (@ f > 10Hz)
Noise floor @typ.input power and wavelength
Frequency noise bandwidth
Dynamic range
Dynamic range
Minimum measurable intrinsic linewidth(lorentzian linewidth)
Effective linewidth range (optical linewidth)[β-separation method]
Effective linewidth range (optical linewidth) [curve fitting method]
Interface
Analog Output
Cutoff (highpass filter)
Dimensions
Weight
Relative intensity noise limit(lorentzian linewidth)
nm
mW
%
MHz
Hz/√Hz
Hz
dB
dB
Hz
mm
kg
Hz
Hz
Hz
dB/Hz
Hz
± 5
10 – 10 M10 – 10 M 2) 10 – 10 M 2)
60
60
< 3 k
< 10 k – 20 M
< 10 k – 10 M
USB 2.0 Type B
BNC ± 7.5 (50 Ω) ± 15 (high impedance) V, single ended
10, 1k, 10k, 100k
220 × 334 × 96
8.0
– 150
< 12 k
< 20 k – 30 M
< 20 k – 10 M
Ethernet
10
440 × 340 × 155 mm
12
–
< 2 k
< 5 k – 30 M
< 5 k – 10 M
Ethernet
10
440 × 340 × 155 mm
12
–
< 10 k
< 15 k – 100 M
< 15 k – 10 M
Ethernet
10
440 × 340 × 155 mm
12
–
< 350
< 1 k – 20 M
< 1 k – 10 M
USB 2.0 Type B
10, 1k, 10k, 100k
220 × 334 × 96
8.0
– 150
Laser type CW, single mode
PM-FC/APC
30
FC/APC
40
PM-FC/APC
30
FC/APC
40
FC/APC
100
min maxtyp
LWA-1k 780 1)
10
200
100
75
1k
30
10k
30
100k
25
> 1M
15
min maxtyp
LWA-10k VIS 1)
10
500
100
150
1k
60
10k
60
100k
50
> 1M
30
min maxtyp
1530
0.5
1625
8
1550
5
LWA-1k 1550
10 100 1k 10k 100k > 1M
80 40 15 10 8 5
min maxtyp
1064
0.5
1625
8
1550
5
LWA-10k NIR
10 100 1k 10k 100k > 1M
200 100 30 20 15 10
min maxtyp
1064
0.5
1625
8
1550
5
LWA-100k NIR
10 100 1k 10k 100k > 1M
1k 200 60 50 40 25
760 1064 2)780 450 1064 2)780
Linewidth Analyzer · 1-2022 · This document provides general information only and may be subject to change at any time without prior notice.
Feedback Controller
Due to the design of the LWAs, the outputvoltage can be directly used as an error signal for a feedback controller allowing to reduce the frequency noise of the test laser.
Depending on the used feedback controller and the laser system the optical linewidth can be reduced by more than two orders of magnitude offering a vast amount of new opportunities.
Feedback controller Feedback controller
Laser Laser
Active laser noise reduction
Connect the Analyzer output signal as input signal to a fast feedback controller.
Connect the feedback controller to the laser’s fast DC modulation input (e.g. laser diode current).
Adjust the feedback to minimize the output signal of the Analyzer (e.g. PID parameters, gain)
Typical application
Laser module quality control
Laser design optimization
Metrology and quantum technology
Linewidth control for spectroscopy
Modulation surveillance
Sample rate
Acquisition time (time series)
Dimensions
Resolution
Communication
Evaluation time 3)
Weight
1) Frequency noise and lineshape specifications are derived from measurements at 780 nm.
2) From 900 nm to 1064 nm the frequency noise bandwidth is limited to 10 Hz to 100 kHz.
3) Effective linewidth: Combination of intrinsic linewidth and additional broadening mechanisms (thermal, electronical and acoustic noise). Determination by β-separation method (noise density spectrum) or curve fitting procedure (lineshape spectrum).
Sa/s
s
mm
bits
s
kg
62.5 M (max.)
1 m – 100 m
210 × 200 × 74
16
USB 3.0 Type B
10 m – 1 (typ.)
2.0
HighFinesse GmbHHighFinesse GmbHWöhrdstraße 4Wöhrdstraße 472072 Tübingen, Germany72072 Tübingen, Germany
Linewidth Analyzer 1-2022 · This document provides general information only and may be subject to change at any time without prior notice.
T + 49 (0) 7071 - 53 918 0T + 49 (0) 7071 - 53 918 0F + 49 (0) 7071 - 53 918 99F + 49 (0) 7071 - 53 918 99M [email protected] [email protected]
Additional informationAdditional informationand distributors:and distributors:www.highfinesse.comwww.highfinesse.com
HighFinesse Precision Current HighFinesse Precision Current Sources have been developed Sources have been developed for experiments and quantum for experiments and quantum technologies in the areas of technologies in the areas of Cold atom physics and solid- Cold atom physics and solid- state-physics. The linearly state-physics. The linearly regulated BCS (Bipolar Current regulated BCS (Bipolar Current Source) and UCS (Unipolar Source) and UCS (Unipolar Current Source) series deliver Current Source) series deliver highly stable, low noise source highly stable, low noise source currents for high precision mag-currents for high precision mag-netic field control. The current netic field control. The current output is floating or is on a user output is floating or is on a user defined potential. Ultrafast re-defined potential. Ultrafast re-sponse to control signals and sponse to control signals and trigger functions, clear grounding, trigger functions, clear grounding, connection and signal isolation connection and signal isolation schemes make the integration of schemes make the integration of the current sources into complex the current sources into complex experimental systems easy.experimental systems easy.
PrecisionPrecisionCurrent SourcesCurrent SourcesSpectrometer OSASpectrometer OSA
HighFinesse/Ångstrom offers sen-HighFinesse/Ångstrom offers sen-sitive and compact wavelength sitive and compact wavelength meters with a large spectral range meters with a large spectral range for high speed measurement of for high speed measurement of lasers. The optical unit consistslasers. The optical unit consistsof temperature-controlled Fizeau-of temperature-controlled Fizeau-based interferometers that are based interferometers that are read out by photodiode arrays. read out by photodiode arrays. The high absolute accuracy is The high absolute accuracy is achieved by use of solid state, achieved by use of solid state, non-moving optics. The optical non-moving optics. The optical unit and associated electronics unit and associated electronics are housed in a compact, thermal are housed in a compact, thermal casing. The connection to a com-casing. The connection to a com-puter or notebook is realized via puter or notebook is realized via a highspeed USB 2.0 port, which a highspeed USB 2.0 port, which allows a high data read-out rate. allows a high data read-out rate. The analyzing software displays The analyzing software displays all the interferometer information.all the interferometer information.
Wavelength MeterWavelength Meter
The grating based HighFinesse/The grating based HighFinesse/Ångstrom Laser Spectrum Ångstrom Laser Spectrum Analyzers offer the capability for Analyzers offer the capability for a very accurate simultaneous a very accurate simultaneous measurement of both the center measurement of both the center wavelength and the linewidth wavelength and the linewidth of a laser source with a compact of a laser source with a compact and versatile instrument.and versatile instrument.
The product series covers the The product series covers the ranges from 192 nm to 110000 ranges from 192 nm to 110000 nm. The grating based technol-nm. The grating based technol-ogy allows the analysis of laser ogy allows the analysis of laser sources over a large linewidth sources over a large linewidth range. Utilizing the principle range. Utilizing the principle of non-moving parts just like of non-moving parts just like the well-known HighFinesse the well-known HighFinesse WS-series wavemeters, the LSA WS-series wavemeters, the LSA offers the time-tested robust-offers the time-tested robust-ness and ability to measure both ness and ability to measure both pulsed and cw lasers.pulsed and cw lasers.