Electromagnetic energy within a magnetic infinite cylinder and
... cylinder is a plane and monochromatic complex wave, with time-harmonic dependence given by exp共−it兲 [19,21]. The quantity is the angular frequency and it is considered to be the same for the incident and scattered waves (elastic scattering). In addition, we assume that these media are electromagn ...
... cylinder is a plane and monochromatic complex wave, with time-harmonic dependence given by exp共−it兲 [19,21]. The quantity is the angular frequency and it is considered to be the same for the incident and scattered waves (elastic scattering). In addition, we assume that these media are electromagn ...
Self-Organization of Atomic Samples in Resonators and Collective Light Forces.
... detuning, the experimentally critical parameter is not the force magnitude, that can be very large due to the stimulated nature of the emission process, but the necessary intensity to reach threshold at the given particle polarizability, sample density and temperature, and light detuning. To identif ...
... detuning, the experimentally critical parameter is not the force magnitude, that can be very large due to the stimulated nature of the emission process, but the necessary intensity to reach threshold at the given particle polarizability, sample density and temperature, and light detuning. To identif ...
lecture plan
... L7: Detailed Theory of Plane Transmission Grating, Formation of Spectra, Concept of Absent Spectra, Dispersive Power of Diffraction Grating. L8: Resolving Power of an Optical Instrument, Rayleigh Criteria for Resolution, Resolving Power of Plane Transmission Grating and Resolving Power of a Glass Pr ...
... L7: Detailed Theory of Plane Transmission Grating, Formation of Spectra, Concept of Absent Spectra, Dispersive Power of Diffraction Grating. L8: Resolving Power of an Optical Instrument, Rayleigh Criteria for Resolution, Resolving Power of Plane Transmission Grating and Resolving Power of a Glass Pr ...
The Magnetic Universe
... magnetic field, and that this field is beautifully ordered into a spiral pattern, just like in our own galaxy. This simply should not be the case – any magnetism that the LMC might have been able to build up over billions of years should have been destroyed as our galaxy gradFigure 3. A simulation o ...
... magnetic field, and that this field is beautifully ordered into a spiral pattern, just like in our own galaxy. This simply should not be the case – any magnetism that the LMC might have been able to build up over billions of years should have been destroyed as our galaxy gradFigure 3. A simulation o ...
Laser Refraction and Diffraction
... A. Measurement of the refractive index of a glass plate 1. Use Fig. 1 to calculate the refractive index of a glass plate. 2. Illuminate the glass plate with a laser beam at a predetermined incident angle. 3. Mark the following spots: ☉ The “spot of output” at the output of the laser. ☉ The “spot of ...
... A. Measurement of the refractive index of a glass plate 1. Use Fig. 1 to calculate the refractive index of a glass plate. 2. Illuminate the glass plate with a laser beam at a predetermined incident angle. 3. Mark the following spots: ☉ The “spot of output” at the output of the laser. ☉ The “spot of ...
Nanocrystalline silicon prepared at high growth rate using helium
... sity rapidly increased in general, with its significant contribution around 520 cm–1, identifying very good crystallinity of the film prepared at P = 120 W. The crystalline volume fraction (Fc) in the network has been estimated using deconvoluted Raman spectra (Das and Bhattacharya 2006) and that ha ...
... sity rapidly increased in general, with its significant contribution around 520 cm–1, identifying very good crystallinity of the film prepared at P = 120 W. The crystalline volume fraction (Fc) in the network has been estimated using deconvoluted Raman spectra (Das and Bhattacharya 2006) and that ha ...
introduction - Stanford Synchrotron Radiation Lightsource
... experiments. It is written based on the User and FEL physics requirements for the x-ray optics and x-ray diagnostics, and the facility requirements (i.e. the facility protocols and guidelines). Some of the User and FEL physics requirements are found in the document “LCLS First Experiments (September ...
... experiments. It is written based on the User and FEL physics requirements for the x-ray optics and x-ray diagnostics, and the facility requirements (i.e. the facility protocols and guidelines). Some of the User and FEL physics requirements are found in the document “LCLS First Experiments (September ...
Evanescent-field optical microscopy: effects of polarization, tip
... with a higher refractive index, grazing-incidence illumination or a coated fibre could also be of ...
... with a higher refractive index, grazing-incidence illumination or a coated fibre could also be of ...
Color center production by femtosecond-pulse laser
... temperature and intensity rate. The difference in using a focused laser beam is that the density of primary defects formed is much higher than the usual methods, and therefore the probability of aggregation is very much increased. This can be seen by the ratio of the F to the M bands in YLF (Fig. 3) ...
... temperature and intensity rate. The difference in using a focused laser beam is that the density of primary defects formed is much higher than the usual methods, and therefore the probability of aggregation is very much increased. This can be seen by the ratio of the F to the M bands in YLF (Fig. 3) ...
physics 415/416 supplemental problems
... shows the relative efficiency of the grating (relative amount of reflected light) versus wavelength. Note that the efficiency is polarization dependent. Light polarized perpendicular to the grooves is called “s-polarization” while light polarized parallel to the grooves is “p-polarization”. Below th ...
... shows the relative efficiency of the grating (relative amount of reflected light) versus wavelength. Note that the efficiency is polarization dependent. Light polarized perpendicular to the grooves is called “s-polarization” while light polarized parallel to the grooves is “p-polarization”. Below th ...
STELLAR ATMOSPHERES
... P pressure and n density that leads to spectra consistent with observations ...
... P pressure and n density that leads to spectra consistent with observations ...
Photonic bandgap
... • effective index of “cladding” is close to that of air (n=1) • anomalous dispersion over wide range (enables soliton transmission) • can tailor flat dispersion for phase-matching ...
... • effective index of “cladding” is close to that of air (n=1) • anomalous dispersion over wide range (enables soliton transmission) • can tailor flat dispersion for phase-matching ...
- CSE PSTU
... optical power budget and system risetime budget, receiver noise power, Q factor, bit error rate and maximum usable bit rate of a digital optical fiber system d. To explain/compare the factors affecting the performance of different optical fiber communication systems e. To communicate laboratory find ...
... optical power budget and system risetime budget, receiver noise power, Q factor, bit error rate and maximum usable bit rate of a digital optical fiber system d. To explain/compare the factors affecting the performance of different optical fiber communication systems e. To communicate laboratory find ...
