Slide 1
... Parameters as lithium temperature (250 C), wave pattern or lithium velocity (15 m/s) must be measured not only for the adequate operation but also for safety. Some of the required diagnostic system will be exposed to intense radiation fields (up to 100 Gy/s) and also to lithium ions bombardment. Rad ...
... Parameters as lithium temperature (250 C), wave pattern or lithium velocity (15 m/s) must be measured not only for the adequate operation but also for safety. Some of the required diagnostic system will be exposed to intense radiation fields (up to 100 Gy/s) and also to lithium ions bombardment. Rad ...
exam solutions
... (c) If you reflect an unpolarized beam from a glass plate at the polarization angle, the reflected light is linearly polarized. (d) In an optically dense material, interference between an incoming beam and the secondary wave it creates is constructive in the forward direction. (e) In specular reflec ...
... (c) If you reflect an unpolarized beam from a glass plate at the polarization angle, the reflected light is linearly polarized. (d) In an optically dense material, interference between an incoming beam and the secondary wave it creates is constructive in the forward direction. (e) In specular reflec ...
Wollaston and Nomarski Prisms
... axis oriented at a 45-degree angle (northwest to southeast) to the polarizer and analyzer. The prisms are composed of two precisely ground and polished wedge-shaped slabs produced from high-grade optical quartz, a uniaxial birefringent crystal. Two quartz wedges having perpendicular orientations of ...
... axis oriented at a 45-degree angle (northwest to southeast) to the polarizer and analyzer. The prisms are composed of two precisely ground and polished wedge-shaped slabs produced from high-grade optical quartz, a uniaxial birefringent crystal. Two quartz wedges having perpendicular orientations of ...
Team Number: ______ OPTICS Team Members
... emitting out of the laser aperture. What type of EM wave is emitted? (2 pts) A) Near Infrared B) Green light C) Near Ultraviolet D) Gamma rays 32. Reflective mirrors used in modern astronomy telescopes are typically _________ in shape. A) flat B) spherical C) hyperbolic D) parabolic 33. In telescope ...
... emitting out of the laser aperture. What type of EM wave is emitted? (2 pts) A) Near Infrared B) Green light C) Near Ultraviolet D) Gamma rays 32. Reflective mirrors used in modern astronomy telescopes are typically _________ in shape. A) flat B) spherical C) hyperbolic D) parabolic 33. In telescope ...
Velocity of sound in liquids
... To determine the wavelength of sound in liquids, and from this calucate the sound velocity, from the structure of the centrally projected image. Set-up and procedure Fig. 1 shows the experiment set-up. The glass cell is 2/3 full of liquid, and the sound head is immersed in it to a depth of a few mil ...
... To determine the wavelength of sound in liquids, and from this calucate the sound velocity, from the structure of the centrally projected image. Set-up and procedure Fig. 1 shows the experiment set-up. The glass cell is 2/3 full of liquid, and the sound head is immersed in it to a depth of a few mil ...
Test Review 3
... The key principle underlying interference is _______________________________________. ...
... The key principle underlying interference is _______________________________________. ...
Interferometry
Interferometry is a family of techniques in which waves, usually electromagnetic, are superimposed in order to extract information about the waves. Interferometry is an important investigative technique in the fields of astronomy, fiber optics, engineering metrology, optical metrology, oceanography, seismology, spectroscopy (and its applications to chemistry), quantum mechanics, nuclear and particle physics, plasma physics, remote sensing, biomolecular interactions, surface profiling, microfluidics, mechanical stress/strain measurement, and velocimetry.Interferometers are widely used in science and industry for the measurement of small displacements, refractive index changes and surface irregularities. In analytical science, interferometers are used in continuous wave Fourier transform spectroscopy to analyze light containing features of absorption or emission associated with a substance or mixture. An astronomical interferometer consists of two or more separate telescopes that combine their signals, offering a resolution equivalent to that of a telescope of diameter equal to the largest separation between its individual elements.