Polarization of Light Reflected from Rough Surfaces with by Wright F. E. PDF
By Wright F. E.
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Extra resources for Polarization of Light Reflected from Rough Surfaces with Special Reference to Light Reflected by the Moon
Example text
In measurement, a tunable laser source with a tuning range 1525–1575 nm was used as an input light source. Three wavelengths of λ1 = 1540 nm, λ2 = 1550 nm, and λ3 = 1560 nm were coupled to the input waveguides 1, 2, and 3, respectively. 35 Fabricated optical switch array on a 4-inch Si wafer. extinction ratio of the device were calculated. The insertion loss of the device is defined as 210 log10(Pout/Pin), where Pin is the input power, Pout is the output power. 98 dB, which includes total on-chip propagation and structure loss.
14 Output optical power versus the applied forward bias. 55 µm operation14. It is a 2 × 2 SiGe waveguide structure with an input Y branch and an output Y branch connected to an intersection region. 15 Near-field output intensity patterns observed by a vidicon at the end facets of the switch. © Woodhead Publishing Limited, 2010 Electro-optical switches 21 forward-bias into a region, which is called the carrier injection region. The injected carriers in this region diffuse and drift toward a collector which is located on the surface of the guiding layer and apart from the p-n+ junction for a distance of d.
55-µm optical signals with same original phase, amplitude, and polarization are coupled into the input ports A and B, respectively and without applying a forward-bias voltage to both the p-n junctions of regions I and II, the input signal coupled from the input port A will be switched to the output port 3 and the input light coupled from the input port B will be switched to the output port 1. In this case, the switch is at cross-state and functions as an optical crossconnection, as shown in Plate Va.
Polarization of Light Reflected from Rough Surfaces with Special Reference to Light Reflected by the Moon by Wright F. E.
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