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Power detector

The beam was then made divergent with a lens. The wafer holder was positioned to ensure a uniform exposure of the resist. In line with the wafer holder was a Scientech 365 Power and Energy Meter equipped with a 2.5 cm diameter thermopile detector. Power/ pulse/cm was obtained while the laser was in a free running mode. The number of pulses needed for a particular dose was calculated. The laser was then triggered and controlled with a Hewlett Packard Model 3314A Pulse Generator. [Pg.295]

A. Detector power supply - wavelength fixed at 254 nm- push in the red button. [Pg.581]

Use the balance knob on the left side of the detector power supply and adjust the pen on the recorder to about 10% full scale. Do not put the recorder pen on the paper,... [Pg.583]

Shut off the detector power supply and clean up the area. Thank you. [Pg.583]

The hardware of an automated solid-phase synthesizer consists of all the electromechanical components of the system (reaction vessel, tubing, valves, pumps, detectors, power supplies, circuit boards, sensors, etc.). It is imperative that all these components are reliable and can operate without failure for many synthesis cycles before repair or replacement. Before using any component in an automated system, it should undergo compatibility and lifetime testing with the reagents that would be in contact during the synthesis. [Pg.717]

The goal of this brief review is to demonstrate the power of the spectropolarimetiy. We enter now a golden age of polarimetry. The combination of new a generation of giant telescopes, high sensitive detectors, powerful computers and fast communication open the possibility to investigate tiny structures of the spectra of cosmic objects from far ultraviolet to the radio domain for extremely faint objects, to discriminate between various physical mechanisms of radiation and to look into the early stages of the Universe. Spectropolarimetiy is now in the point of intersection of microcosm and macrocosm. [Pg.475]

It is possible to find on the market many electronic devices necessary for flow system assemblies, whether constructed, e.g. detectors, power supply, input converter cards and digital output cards, relays, or in kit form. However, frequently it is mandatory to build your own electronics, e.g. to adapt the analog outputs from one device to the other input. [Pg.119]

Explain the rod shadow effect and what this means to reactor operation in terms of effects on rod worths and detector power level indication. [Pg.251]

Filters that output noncoherent detector statistics have, in our recent work [1], shown to be very powerful for grain noise suppression in ultrasonics. However, such filters require the operator to carefully specify a transient prototype as a model of the defect echoes which should be detected. Here a new approach is presented, based on the above ideas about perception, which eliminates the need for the operator to manually specify a defect prototype. [Pg.89]

The war itself also drove the development of improved and miniaturised electronic components for creating oscillators and amplifiers and, ultimately, semiconductors, which made practical the electronic systems needed in portable eddy current test instruments. The refinement of those systems continues to the present day and advances continue to be triggered by performance improvements of components and systems. In the same way that today s pocket calculator outperforms the large, hot room full of intercormected thermionic valves that I first saw in the 50 s, so it is with eddy current instrumentation. Today s handheld eddy current inspection instrument is a powerful tool which has the capability needed in a crack detector, corrosion detector, metal sorter, conductivity meter, coating thickness meter and so on. [Pg.273]

Fig. 1 shows the block diagram of the vibrometer, in which the most sensible to small phase variations interferometric scheme is employed. It consists of the microwave and the display units. The display unit consists of the power supply 1, controller 2 of the phase modulator 3, microprocessor unit 9 and low-frequency amplifier 10. The microwave unit contains the electromechanical phase modulator 3, a solid-state microwave oscillator 4, an attenuator 5, a bidirectional coupler 6, a horn antenna 7 and a microwave detector 11. The horn antenna is used for transmitting the microwave and receiving the reflected signal, which is mixed with the reference signal in the bidirectional coupler. In the reference channel the electromechanical phase modulator is used to provide automatic calibration of the instrument. To adjust the antenna beam to the object under test, the microwave unit is placed on the platform which can be shifted in vertical and horizontal planes. [Pg.655]

The software US-SCAN 3.0 (IBT GmbH, Ober-Ramstadt, Germany) provides all functions of a portable flaw detector and a powerful ultrasonic imaging in A-, B-, C- and D-scans. Not only motor driven scanners can he used, but also manual scanning systems with encoders. Further documentation and test reports can be carried out with Windows software. [Pg.859]

The pulser/receiver HILL-SCAN 30XX boards satisfy DIN 25450. Typical applications are ultrasonie imaging systems for nuclear power stations and for aircraft, material characterization, transducer qualification, replacement of portable flaw detectors (inspections of welded joints), inspection of new materials, measurement systems with air eoupling. ... [Pg.861]

The electronic block, which includes block of the analysis and registration and control system engines, and block of the source-receiver of acoustic oscillations are universal for any installations of this type. As the source-receiver of acoustic oscillations the ultrasonic flow detector is usually use. It s, as a rule, the serial devices for example y/f2-12. The electronic block contains the microprocessor device or PC, device of the power supply and management of engines... [Pg.883]

THz. Therefore, for laboratory absorption experiments, a typical FIR detector provides an estimated detection limit (NEP/source power) of 10 with a source output of 20 nW. In general, high-sensitivity bolometers... [Pg.1235]

Probably the simplest mass spectrometer is the time-of-fiight (TOP) instrument [36]. Aside from magnetic deflection instruments, these were among the first mass spectrometers developed. The mass range is theoretically infinite, though in practice there are upper limits that are governed by electronics and ion source considerations. In chemical physics and physical chemistry, TOP instniments often are operated at lower resolving power than analytical instniments. Because of their simplicity, they have been used in many spectroscopic apparatus as detectors for electrons and ions. Many of these teclmiques are included as chapters unto themselves in this book, and they will only be briefly described here. [Pg.1351]

When the applied magnetic field is swept to bring the sample into resonance, MW power is absorbed by the sample. This changes the matching of the cavity to the waveguide and some power is now reflected and passes via the circulator to the detector. This reflected radiation is thus the EPR signal. [Pg.1561]

The most connnonly used detector in EPR is a semiconducting silicon crystal in contact with a tungsten wire, which acts as an MW rectifier. At microwatt powers, crystal detectors are typically non-linear and render a... [Pg.1561]

The low MW power levels conuuonly employed in TREPR spectroscopy do not require any precautions to avoid detector overload and, therefore, the fiill time development of the transient magnetization is obtained undiminished by any MW detection deadtime. (3) Standard CW EPR equipment can be used for TREPR requiring only moderate efforts to adapt the MW detection part of the spectrometer for the observation of the transient response to a pulsed light excitation with high time resolution. (4) TREPR spectroscopy proved to be a suitable teclmique for observing a variety of spin coherence phenomena, such as transient nutations [16], quantum beats [17] and nuclear modulations [18], that have been usefi.il to interpret EPR data on light-mduced spm-correlated radical pairs. [Pg.1566]

The first detector for optical spectroscopy was the human eye, which, of course, is limited both by its accuracy and its limited sensitivity to electromagnetic radiation. Modern detectors use a sensitive transducer to convert a signal consisting of photons into an easily measured electrical signal. Ideally the detector s signal, S, should be a linear function of the electromagnetic radiation s power, P,... [Pg.379]


See other pages where Power detector is mentioned: [Pg.24]    [Pg.194]    [Pg.190]    [Pg.582]    [Pg.265]    [Pg.125]    [Pg.118]    [Pg.24]    [Pg.194]    [Pg.190]    [Pg.582]    [Pg.265]    [Pg.125]    [Pg.118]    [Pg.216]    [Pg.146]    [Pg.301]    [Pg.540]    [Pg.541]    [Pg.856]    [Pg.969]    [Pg.1062]    [Pg.1165]    [Pg.1168]    [Pg.1235]    [Pg.1235]    [Pg.1475]    [Pg.1561]    [Pg.1561]    [Pg.1566]    [Pg.1574]    [Pg.1670]    [Pg.1829]    [Pg.2955]    [Pg.3001]    [Pg.500]    [Pg.388]   


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