Abstract:
Multichannel array for establishing viscous flow for preventing the flow of particulates causing window clouding. Process chamber for confining process pressure within a process volume with a viewport window along the chamber for viewing portion of process volume. Ingress port disposed in the process chamber for receiving flow of process gas and egress port for extracting flow rate of gas from the process volume. Multichannel array (MCA) disposed between viewport window and process volume of the process chamber. Window chamber separate viewport window from MCA with chamber window port for receiving gas. Viscous flow formed at window side of channels, prevents material from entering window chamber and adhering to window. Viscous flow established by increasing pressure in window chamber via chamber window port. Viscous flow rate substantially lower than rate of process gas flow into process volume.
Abstract:
The present invention is directed to an apparatus, method and software producer for enhancing the dynamic range of a CCD sensor without substantially increasing the noise. Initially, the area of a N x M pixel CCD sensor array is subdivided into two regions, a large region having (M-a) pixels in each column for outputting large-amplitude signals with low noise and a smaller region having a pixels in each column for outputting small-amplitude signals with improved dynamic range. At integration time, the CCD is read out one region's vows at a time into the horizontal shift registers by shifting the pixel charges in either a or M-a vertical shifts. The charges in the horizontal shift registers are then shifted out of the horizontal shift registers in N horizontal shifts.
Abstract:
The present invention is directed to a system and method for radiometric calibration of spectroscopy equipment utilized in fault detection and process monitoring. Initially, a reference spectrograph is calibrated to a local primary standard (a calibrated light source with known spectral intensities and traceable to a reference standard). Other spectrographs are then calibrated from the reference spectrograph rather than the local primary calibration standard. This is accomplished by viewing a light source with both the reference spectrograph and the spectrograph to be calibrated. The output from the spectrograph to be calibrated is compared to the output of the reference spectrograph and then adjusted to match that output. The present calibration process can be performed in two stages, the first with the spectrographs calibrated to the reference spectrograph and then are fine tuned to a narrow band light source at the plasma chamber. Alternatively, the reference spectrograph can be calibrated to the local primary standard while optically coupled to the plasma chamber. There, the local primary standard calibration light source is temporarily positioned within the plasma chamber, or in a light chamber disposed along the interior of the chamber for calibrating the reference spectrograph. Other spectrographs can be calibrated to the reference spectrograph while coupled to the plasma chamber with the local primary standard calibration light source, thereby calibrating every component in the entire optical path to the reference spectrograph.
Abstract:
A linearly polarized light comprised of two linearly polarized components that are orthogonal to each other, with split optical frequencies, is directed toward a film causing one of the optical polarization components to lag behind the other due to an increase in the optical path in the film for that component. A pair of detectors receives the beam reflected from the film layer and produces a measurement signal, and the beam prior to incidence on the film layer and generates a reference signal, respectively. The measurement signal and reference signal are analyzed by a phase detector for phase shift. The detected phase shift is then fed into a thickness calculator for film thickness results. A grating interferometer may be included with the heterodyne reflectometer system with a grating, which diffracts the reflected beam into zeroth- and first-order bands, which are then detected by separate detectors. A detector receives the zeroth-order beam and generates another measurement signal. Another detector receives the first-order beam and generates a grating signal. The measurement signal from the grating and reference signal may be analyzed by a phase detector for phase shift, which is related to the thickness of the film. Additionally, the zeroth-order beam measurement signal is analyzed with the grating signal by a phase detector for detecting a grating phase shift induced by the grating. The refractive index for the film can then be calculated directly from grating phase shift and the heterodyne phase shift for the grating pitch, and the beam's wavelength and incidence angle on the film of the measurement apparatus. Using the refractive index and heterodyne phase shift, the film's thickness is determined. Conversely, a film thickness calculation may be derived independent of the film's refractive index using from the actual corrected grating phase shift and corrected heterodyne phase shift.
Abstract:
Afterglow spectroscopy allows observing light emission of gaseous species in absence of direct plasma light. This absence avoids the creation of a background sprectrum obscuring weak emission from trace species. The geometry of the invention prevents direct plasma light (3) from reaching the observation window (10) while a lens (10) focues afterglow emission light on the entrance of a photo multiplier (11). The invention describes a flowing afterglow version monitoring in-situ the cleanup of vacuum tools during pump/purge cycles. The invention also describes an intermittent afterflow version siutable for trace gas analysis at atmospheric pressure.
Abstract:
A spectral ellipsometer that enables complete simultaneous measurement of ellipsometric parameters of a surface (18) with thin films and coatings for the full wavelength range of interest by using an imaging spectrograph (24) together with a novel optical arrangement that disperses the polarization information of a time-invariant train of optical signals in a linear spatial array of points along or parallel to an input aperture or slit of the imaging spectrograph (24) and disperses the polarization information in wavelength perpendicular to the aperture or slit to provide a two-dimentional spectrograph image that is collected and stored by an imaging array with one axis relating to wavelength and the other axis relating to the light polarization. Multiple simultaneous measurements of the spectral ellipsometric parameters psi (psi) and DELTA (delta) are taken at all wavelengths without the need of any time-varying or mechanically-moving optical elements.
Abstract:
A spectral ellipsometer that enables complete simultaneous measurement of ellipsometric parameters of a surface with thin films and coatings for the full wavelength range of interest by using an imaging spectrograph together with a novel optical arrangement that disperses the polarization information of a time-invariant train of optical signals in a linear spatial array of points along or parallel to an input aperture or slit of the imaging spectrograph and disperses the polarization information in wavelength perpendicular to the aperture or slit to provide a two-dimensional spectrograph image that is collected and stored by an imaging array with one axis relating to wavelength and the other axis relating to the light polarization. Multiple simultaneous measurements of the spectral ellipsometric parameters psi (psi) and DELTA (delta) are taken at all wavelengths without the need of any time-varying or mechanically-moving optical elements. The ellipsometer can be used for real-time measurements of ellipsometric parameters of a moving or static surface with the thin films and coatings.