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L09 Instru Spectrofluorometery
L09 Instru Spectrofluorometery

... *detector*(the photocell in UV designed to measure I° and It and take the ratio but here in spectrofluorometer it will measure the intensity of the monochromatic emitted light). Note the design of the spectrofluorometer: The angle between the incident light and the photocell is 90° (but in UV all th ...
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Problem Set 9: SOLUTIONS
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... 3. 15 points. As light from the Sun enters the atmosphere, it refracts due to the small difference between the speeds of light in air and in vacuum. The optical length of the day is defined as the time interval between the instant when the top of the Sun is just visibly observed above the horizon, t ...
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Electricity and Magnetism Experiment

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... index is minimum along CD. A simple consideration of the above shows that the difference between the optical lengths of A'B' and C'D' is less than that between those of AB and CD. As this difference gives twice the amplitude of the corrugation of the emerging wave-front, it follows, in the case show ...
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... are nanophotonic elements designed to achieve this functionality, transducing free-space, far-field radiation to localized electromagnetic energy. The simplest nanoantenna is a single metal nanoparticle whose free electrons can support localized plasmon resonances at visible wavelengths, implying th ...
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Atmospheric optics



Atmospheric optics deals with how the unique optical properties of the Earth's atmosphere cause a wide range of spectacular optical phenomena. The blue color of the sky is a direct result of Rayleigh scattering which redirects higher frequency (blue) sunlight back into the field of view of the observer. Because blue light is scattered more easily than red light, the sun takes on a reddish hue when it is observed through a thick atmosphere, as during a sunrise or sunset. Additional particulate matter in the sky can scatter different colors at different angles creating colorful glowing skies at dusk and dawn. Scattering off of ice crystals and other particles in the atmosphere are responsible for halos, afterglows, coronas, rays of sunlight, and sun dogs. The variation in these kinds of phenomena is due to different particle sizes and geometries.Mirages are optical phenomena in which light rays are bent due to thermal variations in the refraction index of air, producing displaced or heavily distorted images of distant objects. Other optical phenomena associated with this include the Novaya Zemlya effect where the sun appears to rise earlier or set later than predicted with a distorted shape. A spectacular form of refraction occurs with a temperature inversion called the Fata Morgana where objects on the horizon or even beyond the horizon, such as islands, cliffs, ships or icebergs, appear elongated and elevated, like ""fairy tale castles"".Rainbows are the result of a combination of internal reflection and dispersive refraction of light in raindrops. Because rainbows are seen on the opposite side of the sky as the sun, rainbows are more prominent the closer the sun is to the horizon due to their greater distance apart.
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