MODEL 260
ULTRA-STABLE LASER
General Performance:
The Model 260 will provide the user with a reliable and stable single
frequency source of substantially greater power output than heretofore
available commercially. The plasma tubes are preselected to provide
an initial single frequency power output of 3 mW or more and mid-life
values often exceed 3.5 mW. When used as a frequency stabilized
source without a polarizer for single mode selection, the power
output is typically between 6 and 7 mW. In the absence of
retroreflection, the Model 260 will provide a source of excellent
frequency stability, both short and long term. However, the stability
of this type of laser is quite sensitive to retroreflection,
especially when used in the polarized single frequency output mode.
It should be noted that this latter mode will exhibit an amplitude
modulation of some 2.5% peak-to-peak at a frequency of several hundred
kiloHertz. (The exact frequency is fixed and determined by the
particular laser tube employed.) Further, in polarized single
frequency operation there is also a small amount of power, typically
less than 2% of the total, located in axial modes ±860 MHz from line
center. Programming the laser to operate other than at line center
will significantly increase the sum total power in these satellite
modes.
Theory of Operation:
In a laser with three TEM00 modes, there will be two primary beat
frequencies corresponding to the difference frequencies between the
central mode and each of the modes on either side of center. These
two beat frequencies, typically in the range of 400 to 500 MHz, will
in general not be exactly the same because the frequency pulling
effects on each mode will vary with the differing slopes at the
respective operating points on the Doppler gain curve. The difference
between these two beat frequencies will yield a third or
intercombinational beat frequency typically in the range of 100 kHz.
In an integral end mirror tube, where the alternate modes are
orthogonally polarized, the intercombinational beat frequency will not
be zero even when the central mode is at line center because of the
birefringence of the mirrors. In the Model 260, the laser tube is
preselected not only for power but also for an appropriate range in
the intercombinational beat frequency. The median frequency is then
tightly phase locked to the frequency of a crystal controlled
frequency synthesizer. This tight phase lock accounts for the high
degree of short and long term stability achieved with the Model 260.
In addition the use of this digital control system makes it possible
to slave the Model 260 to a reference laser, such as the Model 220, to
improve its frequency stability in the presence of retroreflection.
We have found that the orientation and degree of birefringence in the
chosen laser tubes remain remarkably constant throughout the life of
the laser tube, and readjustment of the plane of polarization or the
lock-frequency setting is rarely necessary to maintain a quality
single frequency output.
Other Features:
The Model 260 employs virtually the same phase locking architecture
that is used in the Model 220. The frequency synthesizer provides a
three decade modulus set by digital switches on the side of the Power
Control Unit, and very readily permits the central output mode to be
locked on line center. Additional preset binary stages to allow for
variability in different plasma tubes The Mode Options Plug, located
on the underside of the Power control Unit, facilitates non-standard
modes of operation.
As with other members of the Model 200 Series, headphones are supplied
as a standard accessory to help the user minimize the problem of
retroreflections. where some loss in long term frequency stability is
acceptable, the convenience of the beam shutter equipped with a high
efficiency cube polarizer and Brester angle absorber is available as
an optional accessory.
Application Hints:
If the full frequency stability of the Model 260 is to be realized,
the associated optical system should be configured to reduce the
problem of retroreflection and/or back scattering to an absolute
minimum. Whenever possible, one should work at a distance to minimize
back scattering and to allow space for the complete absorption of any
specular reflections (by means for example with the Model 211 Black
Etalon). Since back scattering from an internally mounted cube
polarizer may degrade frequency stability by as much as a factor of
ten from the indicated specifications, we also offer a 'reduced drift'
version of this laser. With this option (and an external polarizer
set to operate at a distance), we include additional components to
reduce drift down to 50 kHz/day. For the purpose of defining the
correct axis orientation, a simple HN-32 polarizer is supplied.
In the case of interferometers, designs of the Mach-Zender type, or
any of the corner cube variations of the Michelson type, are much to be
preferred because the interfering beams cannot retrace their paths
back to the laser except by reflection or back scattering from the
detector. Problems of this latter type can be solved by tilting the
PIN diode detector by at least half the convergence angle of the
photodiode focusing lens, having it slightly inside the focal point
of the lens, and using a circular polarizer in front of the lens.
Where direct retroreflection is unavoidable, proper isolation will
require a high-quality calcite polarizer that will provide an
extinction ratio of at least 10-5, and a V-coated* quarter
waveplate very accurately oriented both as to tilt and azimuthal
angle. where intervening optical components alter the state of
polarization of the returning beam so that it is no longer perfectly
circular, it may be necessary to introduce appropriate compensating
plates.
Another technique to reduce the problem of retroreflection that can
often be used to good advantage, especially when a component scatters
the polarization, is to use the unpolarized beam and position
potentially troublesome components at a "servo system nodal point",
i.e., at an integral number of plasma tube cavity lengths from the
output mirror. The high intensity vertically polarized central mode
is then selected out before the detector to provide single frequency
performance.
In each case the headphones and touch test can be used as a diagnostic
corrective technique to arrive at in situ adjustments that will
assure the optimum system performance.
----------------------------------------------------------
- For that fraction of the light undergoing a zig-zag double
internal reflection, there is an additional half wave retardation
that permits retroreflection of this fraction to pass directly back
through the polarizer. The low reflectivity provided by a 6328 V-coat
on the waveplate surfaces is therefore highly desirable.
ULTRA-STABLE LASER
MODEL 260
Specifications: |
Frequency of emitted light (THz) |
473.612200* |
Frequency control range (MHz) |
±15 |
Spatial mode structure |
TEM_00 |
Beam diameter <1/e2> (mm) |
0.8 |
Beam divergence angle (mrad) |
1.0 |
Method of stabilization |
Intercombinational beat phase-locked to xtal
|
Unpolarized axial mode structure |
triple frequency |
Axial mode spacing (kHz) |
435 |
Total power output (mW) |
6.0 |
Amplitude noise (% rms): |
10 Hz - 100 kHz |
< 0.02 |
1 - 2 MHZ |
< 0.02 |
Polarized axial mode structure |
single frequency |
Power output (mW, w/cube polarizer) |
3.0 |
Amplitude noise (% rms): |
< 0.005 |
10 Hz - 100 kHz: |
< 0.02 |
1 - 2 MHz: |
< 0.1 |
Amplitude modulation (% rms): |
<1 |
Frequency of ampl. mod. (kHz): |
200 - 1000 |
Frequency stability (kHz): |
1 sec |
10 |
1 min |
10 |
1 hour |
50 |
1
day |
200 |
|
Warm-up time (min): |
for stable operation |
35 |
for rated specifications |
90 |
Laser head operating temperature (°C) |
40 |
Environmental temperature range (°C): |
for normal operation |
22 ± 5 |
for limited stability (± 1 °C) |
5 - 17, 27 - 33 |
for storage |
5 - 45 |
Cube Polarizer |
Yes |
Reduced drift option (HN-32 Pol. <T=0.7) |
Yes |
Accessories available |
Yes |
Laser head dimensions (in/cm) |
3x3x16.9/7.5x7.5x43 |
Laser head weight (Ib/kg) |
7.5/3.4 |
Power control unit dimensions (in/cm) |
6x3x7.5/15x7.5x19 |
Power control weight (Ib/kg) |
5.5/2.5 |
Operating voltage (V) |
115 or 230 (spec.) |
Power consumption (W) |
70 |
B.R.H. Class IIIa compliance |
Yes |
Accessories included |
Headphones |
----------------------------- |
* Final zero not significant. |
Copyright. 1987
LABORATORY FOR SCIENCE
2821 9th Street
Berkeley, CA 94710
(415) 653-7591
|