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The Early Days of Laser Spectroscopy
The Early Days of Laser Spectroscopy

Chapter 37 - UBC Physics
Chapter 37 - UBC Physics

... Light Section 20.5, Electromagnetic waves Light is an electromagnetic which travels at 3.00×108m/s in a vacuum. It obeys the relationship: λf = c just like other traveling waves. For visible light, 700nm(red) > λ > 400 nm(indigo) See page 631 for wavelengths of colours Index of refraction = n = ...
TC3PhysSummOutln - Candor Central School
TC3PhysSummOutln - Candor Central School

optical trap
optical trap

... without damaging them. Optical tweezers prove very useful for this because, not only can they manipulate small particles very precisely, but, using infrared light, they can do so without causing damage. The development of the single beam optical trap was an important advance in optical tweezers, bec ...
Contactless visible light probing for nanoscale ICs through 10 μm
Contactless visible light probing for nanoscale ICs through 10 μm

Lecture 6: Continuum Opacity and Stellar Atmospheres
Lecture 6: Continuum Opacity and Stellar Atmospheres

Antonio Rizzo
Antonio Rizzo

transverse waves
transverse waves

... • A transverse wave causes the particles in the medium to oscillate perpendicularly to the direction of wave travel ...
Precession optomechanics - EECS @ UMich
Precession optomechanics - EECS @ UMich

Non-reciprocal Light-harvesting Antennae
Non-reciprocal Light-harvesting Antennae

The Hydrogen Ionization Front-Photosphere
The Hydrogen Ionization Front-Photosphere

Design and Simulation of DPSS Laser with SHG for Material
Design and Simulation of DPSS Laser with SHG for Material

... certain crystal direction at an angle to the optic axis, ne(2 ) at the second harmonic is the same as no( ) at the fundamental frequency: ne(2 )=no( ). This is called index matching and the angle is the phase matching angle. To separate the second harmonic beam from the fundamental beam, something l ...
PHYSICAL SCI E09 11
PHYSICAL SCI E09 11

... properties of light, how it is produced, and the order of waves in the electromagnetic spectrum are described in this unit. The manipulation of light by mirrors and lenses and optical instruments are also presented. Essential Outcomes: (Must be Assessed) 1. The Student Will describe the different ty ...
Correcting chromatic aberrations using a diffraction grating in a
Correcting chromatic aberrations using a diffraction grating in a

... takes for parallel rays entering the lens to meet, and is measured in diopters. Convergent elements have positive powers, and divergent ones have negative power. The combined power of two lens elements in series is the sum of the individual powers. A lenses power will be different for different colo ...
A negative permeability material at red light
A negative permeability material at red light

... thickness δ are chosen to reproduce the complex values of far-field reflectance and transmittance due to a given film. Optical negative index metamaterials (NIMs), also known as left-handed materials, are artificially engineered metal-dielectric composites that exhibit n' < 0 within a certain range ...
Black Coatings to Reduce Stray Light
Black Coatings to Reduce Stray Light

(FT-IR) Microspectroscopic Measurements of Intact Spheres
(FT-IR) Microspectroscopic Measurements of Intact Spheres

... It is simply the consequence of coupling between molecular and morphological properties of the sample. In fact, the spectra become richer in information, since this traditionally molecular measurement now encodes structure as well. While the morphologic information regarding spherical domains inhere ...
Conscious Light, and Signs of the Divine
Conscious Light, and Signs of the Divine

Waves &amp; Oscillations Physics 42200 Spring 2014 Semester
Waves & Oscillations Physics 42200 Spring 2014 Semester

Interaction of light with gravitational waves
Interaction of light with gravitational waves

Lecture 9: Radiation processes Almost all astronomical information
Lecture 9: Radiation processes Almost all astronomical information

... about 3200 Å) to somewhat longer (about 10,000 Å) than the visible as the optical part of the spectrum. Physicists measure optical wavelengths in nanometers (nm). Astronomers tend to use Angstroms. 1 Å = 10-10 m = 0.1 nm. Thus, a physicist would say the optical region extends from 320 to 1000 nm.) A ...
Optical Sources
Optical Sources

... This region is depleted of most carriers A photon generates an electron-hole pair in this region that moves rapidly at the drift velocity by the electric field An electron-hole pair generated outside the depletion region they move by diffusion at a much slower rate Junction is typically reversed bia ...
RAY OPTICS notes
RAY OPTICS notes

... The distances measured in the same direction as the incident light are taken as positive and those measured in the direction opposite to the direction of incident light are taken as negative . ...
Maxwell`s Equations, Photons and the Density of States
Maxwell`s Equations, Photons and the Density of States

... polarization, while the magnetic flux density is given by the sum of magnetic field and magnetization. Some authors prefer not to differentiate between H and B. This leads to difficulties, as can be easily seen from the fact that B is source-free (2.1b) but H is not, as follows from the inspection o ...
Optical forces on small magnetodielectric particles
Optical forces on small magnetodielectric particles

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Magnetic circular dichroism

Magnetic circular dichroism (MCD) is the differential absorption of left and right circularly polarized (LCP and RCP) light, induced in a sample by a strong magnetic field oriented parallel to the direction of light propagation. MCD measurements can detect transitions which are too weak to be seen in conventional optical absorption spectra; they can also probe paramagnetic properties and the symmetry of the electronic levels of the studied systems, such as metal ion sites.
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