What are the general requirements for using LayTec‘s in-situ sensors?
For using our standard systems (EpiTT, EpiCurve®TT, EpiR, EpiRAS®TT) a normal incidence viewport is required, together with enough space next to the window. Optical access to the sample must not be blocked within the reactor by additional apertures. Ceilings or inner liner tubes between viewport and sample need to have small holes. In case of a multi-wafer system a "reset" pulse once per revolution is needed for wafer selective measurements.
Which growth systems are compatible with LayTec sensors?
Is sample wobble a problem?
The LayTec in-situ tools are adapted to typical sample wobble of standard MOCVD and MBE systems by LayTec's patented wobble compensation module.
How much wobble can be tolerated?
For customized MOCVD and MBE systems the maximal tolerable wobble is dependent on the geometry. Please contact LayTec for a detailed analysis of possible adoptions. A tool to evaluate the current wobble can be provided on request.
Are window depositions a problem?
Window depositions should be avoided. We therefore strongly recommend purged or heated view-ports. The influence of minor window deposition to reflectance and temperature measurements can be compensated by automated normalization procedure to the substrate reflectance. However, increasing deposition on windows will increase absorption and lead to a lower signal. Hence signal-to-noise-ratio and temperature measurement will be affected.
What is the typical range of rotation frequencies the LayTec systems can cope with?
Most LayTec in-situ sensors can be used on non-rotating samples and for slowly rotating up to the fast speed rotating systems (5rpm-300rpm).
Do vibrations in the Lab have an influence on the in-situ measurements?
Vibrations need to be considered in the design and mounting of the in-situ sensor, Please specify vibration by a simple laser reflectance measurement. Fiber-optical access as realized in LayTec's EpiTT and EpiR DA TT sensors is advantageous in case of strong vibrations!
Can measurements be done in AIXTRON planetary G2 systems using gas-foil rotation for the main susceptor?
It is necessary to install an additional external optical rotation sensor that has to be customized.
Can measurements be done on Aix 200/4 3x2“ satellites?
Yes, EpiRAS and EpiR M are capable to measure in Aix 200/4 3x2” configuration (not wafer selective). Find more in our application note >
Can measurements be done on Aix G3 24x2” and G4 42x2” (multiple wafers per recess)?
Yes, EpiTT and EpiTwin TT are capable to measure at multi wafer pockets (recess) configuration (not wafer selective). In case of 42 or 49x2” with a center wafer on each recess, a wafer selective measurement can be measured for the center wafer.
What are the MOCVD/ MBE requirements for RAS measurements?
One full rotation of the wafer under the view-port is necessary for a RAS measurement with the standard EpiRAS or EpiRAS TT sensors. If wafers are not rotating, customized RAS solutions are required. Please contact LayTec directly.
Why is it necessary to measure a full revolution of the wafer to obtain a RAS signal?
The RAS signal depends on the azimuth of the wafer relative to the fixed polarization of the measurement light. After measuring a full revolution a Fourier analysis can be used to obtain the RAS amplitude from the sinusoidal signal.