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Electro-Optic Modulation
by Robert F. Enscoe and Richard J. Kocka
The laser, when coupled with a wideband modulation system,
has many applications in data recording. As data recording has progressed,
demands for wider recording bandwidths have marked the design of modulators.
In this article, we'll consider the design and application of transverse-field
electro-optic modulators using the Pockels effect. This effect produces
a refractive index change when an electric field is applied to specific
classes of crystals.
The electroded crystal may be considered to be a voltage-variable waveplate (Figure 1.) When a voltage is applied, the polarization of the light exiting the crystal changes. This variation in polarization results in intensity modulation downstream from the output polarizer. The ideal
electro-optic material possesses all of the following properties:
Modulator
Design
Drive
Amplifier Considerations Bandwidth considerations will now determine the configuration of both the driver and modulator. If system bandwidth is the range of DC to 10 megahertz, the modulator may be driven as a lumped capacitor. A push-pull common-emitter stage with a balanced output impedance of 100 ohms will perform quite nicely throughout this range. Some shunt peaking in the amplifier output will deliver detected rise times of 35 ns with less than 5% overshoot. Figure 3 depicts the modulator as a single 180-pF capacitor. Detected response is close to 10 MHz with short interconnecting cables between modulator and driver.
For a modulator with the same total capacitance and a driver with equal output impedance, the bandwidth is improved by a factor of 2.5 over the simpler, lumped, single 180-pF case. This improvement comes at no increase in output power of the drive electronics. To extend the bandwidth past 25 MHz, the intrinsic propagation delay of the balanced line must be reduced. This may be accomplished either by reducing the total capacitance of the modulator (i.e., using a smaller optical aperture) or by lowering the characteristic impedance of the balanced line. One 50-Mhz system uses an optical modulator with a 50-ohm characteristic impedance, thus reducing the delay to 9 ns and doubling the useable bandwidth of the modulator. At this point, the drive electronics' power-handling capability must be doubled. Operating from DC through 50 MHz requires a much-broader-bandwidth output stage in the driver. A cascade-connected, ground-base output stage is an excellent choice for broadband operation, because it removes any Miller capacitance at its input, thus reducing the reactive component of the input impedance to the stage. The large-geometry output transistors required for high-current operation have intrinsically high output capacitance (C0b) which cannot be tuned out as the stage response extends down to DC. The common-base design increases the output break frequency of the amplifier, as the typical Rbb and associated external base impedance are negligible. Common-base operation is potentially the most unstable amplifier connection, since the device exhibits gain out to ft. This makes small parasitic strays dominant at frequencies where the device still has forward gain. For this reason, the designer must pay close attention to the electrical performance of the transmission line within the modulator. Doubling the bandwidth again, to 100 MHz, presents a far more complex problem than going from 25 to 50 MHz. Extending useable response from DC to 100 MHz requires that the propagation delay of the modulator again be cut in half. To cut the impedance to 25 ohms would mean that the peak current in the output stage would be greater than 3.6 amps. Devices with this current-handling capability have very large output capacitance and would, in effect, limit the response of the driver to less than the required system bandwidth. Paralleling smaller-geometry devices in the output would also parallel output capacitance, yielding the same results as the larger output transistor. Reducing the total modulator capacitance would cause a dramatic reduction in the useable optical aperture, thus precluding large-frame ion lasers without beam-forming optics. One viable alternative is to section the modulator in two pieces, cutting the electrical delay of the modulator in half, and then driving the modulator section electrically in parallel, optically in series. Each modulator section would then rotate the plane of polarization 45°; when combined, they would deliver a full 90° rotation. This approach (Figure 5) would maintain a 50-ohm characteristic impedance for each section.
Maintaining a 50-ohm characteristic impedance keeps the interconnecting balance cable at a commercially available value and also removes the difficult power-handling requirements that a 25-ohm structure would have required. The amplifier is capable of putting out more than 40 watts of RF power from DC to 100 MHz. All of the transmitted RF, after propagating down the electro-optic modulator, is absorbed by high-power thick-film resistors, which terminate the line in the proper characteristic impedance. No electrical power is absorbed in the modulator head, as all the elements are reactive. Large-signal, DC-coupled linear amplifiers have to deal with very large dynamic power changes within the active devices. This device dissipation change versus operating point shows up in the output as a signature or "thermal tail", which will effect the overall repeatability of the input/output transfer function. Good repeatability is essential in analog imaging recorders for tight correlation between the video input signal and resultant exposure level. Thermal time constants of small-geometry devices can be in the 2 to 3-microsecond range, well within the more dominant, low frequency imaging detail. The only practical way to minimize this effect is to make the quiescent amplifier current large with respect to the current signal, thus making the particular stage dissipation remain fairly constant. Closed-loop feedback is not practical because the inherent propagation delay through the amplifier is typically of the order of tens of nanoseconds, thus limiting the loop bandwidth to a few megahertz. Modulator
Bias Control Typically, two different types of automatic servo systems can be used, depending on the application. For scanning systems, where a "dead time" (retrace) is available, a sampled loop is often used (Figure 6). During the dead time, a signal is applied to the system at J2 that instructs the loop to start operation. A signal is generated by the clock, amplified by the RF power amplifier, and sent to the modulator. A photodetector examines the resultant modulation, while a sample-and-hold extracts amplitude phase information. The resultant error signal (if any) is amplified and applied to the modulator through the bias amplifier to reduce the operating point error. The sampled system can set the operating point at either minimum or maximum transmission, as required by system format.
In the second type of system, generally used in continuouswave systems such as videodisk mastering (Figure 7), the average optical power exiting the modulator in both the throughput and rejected ports is measured, compared differentially, and amplified. The differential error is then reduced by the high-gain negative-feedback loop. This format sets the modulator's operating point at the 50% transmission level.
Applications Imaging
and Data Recorders. Disk Recorders Digital
Recording Modulator Alignment Procedure I. All products described here are "transverse field type"
Pockels cells. II. The modulator
materials are: III. Alignment
Figure
1.
2. A DC power supply is required, if you have a Conoptics driver one
is included with it.
Figure
2.
Please note that if you've used an auxiliary polarizer at the input for power attenuation, it will have to be removed for this step. If your laser polarization is vertical, then the rejected component will be directed to the ceiling or table top. DO NOT BLOCK THE REJECTED COMPONENT AT THE MODULATOR. If you want the plane of polarization horizontal (vertical in) then the rejected component will be in a plane parallel to the table top. (See Figure 3)
Figure
3.
5. Fine polarization alignment. Align the power meter or photo-diode to accept the beam exiting the modulator. For parallel operation (vertical in-vertical out), adjust the bias voltage and the rotation of the cell for a minimum; for crossed operation, adjust the bias voltage and rotation for a maximum. 6. Fine
pitch and yaw adjustments. Adjust the voltage for a maximum and note
the extinction ratio (max/min). Adjust the voltage for a minimum; adjust
the cell in pitch and yaw, slightly, while observing the minimum (you
will have to re-adjust the voltage), to improve the minimum. Re-check
the maximum to be sure that you have not reduced it. |
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