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Sunlight bending through ice crystals in cirriform clouds produces bands of color called sundogs, or parhelia, on both sides of the sun on this cold winter day in Minnesota. Photo © 2002 STAR TRIBUNE/Minneapolis-St. Paul. Fig. 15-CO, p. 414
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Figure 15.1: Cloud droplets scatter all wavelengths of visible white light about equally. The different colors represent different wavelengths of visible light. Fig. 15-1, p. 417
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Sunlight Cloud droplet Editable Text Fig. 15-1, p. 417
Figure 15.1: Cloud droplets scatter all wavelengths of visible white light about equally. The different colors represent different wavelengths of visible light. Cloud droplet Editable Text Fig. 15-1, p. 417
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Figure 15.2: Since tiny cloud droplets scatter visible light in all directions, light from many billions of droplets turns a cloud white. Fig. 15-2, p. 417
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Some light penetrates to cloud base
White light is scattered in all directions Figure 15.2: Since tiny cloud droplets scatter visible light in all directions, light from many billions of droplets turns a cloud white. Some light penetrates to cloud base White light is scattered in all directions Editable Text Fig. 15-2, p. 417
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Figure 15.3: Average percent of radiation reflected, absorbed, and transmitted by clouds of various thickness. Fig. 15-3, p. 417
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Figure 15.4: The sky appears blue because billions of air molecules selectively scatter the shorter wavelengths of visible light more effectively than the longer ones. This causes us to see blue light coming from all directions. Fig. 15-4, p. 418
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Figure 15. 5: Blue skies and white clouds
Figure 15.5: Blue skies and white clouds. The selective scattering of blue light by air molecules produces the blue sky, while the scattering of all wavelengths of visible light by liquid cloud droplets produces the white clouds. Fig. 15-5, p. 418
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Figure 15. 6: The Blue Ridge Mountains in Virginia
Figure 15.6: The Blue Ridge Mountains in Virginia. The blue haze is caused by the scattering of blue light by extremely small particles—smaller than the wavelengths of visible light. Notice that the scattered blue light causes the most distant mountains to become almost indistinguishable from the sky. Fig. 15-6, p. 419
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Figure 15.7: The scattering of sunlight by dust and haze produces these white bands of crepuscular rays. Fig. 15-7, p. 419
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Figure 15.8: Because of the selective scattering of radiant energy by a thick section of atmosphere, the sun at sunrise and sunset appears either yellow, orange, or red. The more particles in the atmosphere, the more scattering of sunlight, and the redder the sun appears. Fig. 15-8, p. 420
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Observer Sunset or sunrise Editable Text Fig. 15-8, p. 420
Figure 15.8: Because of the selective scattering of radiant energy by a thick section of atmosphere, the sun at sunrise and sunset appears either yellow, orange, or red. The more particles in the atmosphere, the more scattering of sunlight, and the redder the sun appears. Sunset or sunrise Editable Text Fig. 15-8, p. 420
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Figure 15. 9: Red sunset near the coast of Iceland
Figure 15.9: Red sunset near the coast of Iceland. The reflection of sunlight off the slightly rough water is producing a glitter path. Fig. 15-9, p. 420
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Figure 15.10: Bright red sky over California produced by the sulfur-rich particles from the volcano Mt. Pinatubo during September, The photo was taken about an hour after sunset. Fig , p. 421
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Figure 15.11: The behavior of light as it enters and leaves a more-dense substance, such as water.
Fig , p. 421
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Normal Normal Mirror Editable Text Fig. 15-11, p. 421
Figure 15.11: The behavior of light as it enters and leaves a more-dense substance, such as water. Mirror Editable Text Fig , p. 421
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Figure 15.12: Due to the bending of starlight by the atmosphere, stars not directly overhead appear to be higher than they really are. Fig , p. 422
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Star appears to be here Star Actual position of star Editable Text
Figure 15.12: Due to the bending of starlight by the atmosphere, stars not directly overhead appear to be higher than they really are. Editable Text Fig , p. 422
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Figure 15.13: The bending of sunlight by the atmosphere causes the sun to rise about two minutes earlier, and set about two minutes later, than it would otherwise. Fig , p. 422
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Figure 15.13: The bending of sunlight by the atmosphere causes the sun to rise about two minutes earlier, and set about two minutes later, than it would otherwise. Stepped Art Fig , p. 422
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Figure 15.14: The very light green on the upper rim of the sun is the green flash. Also, observe how the atmosphere makes the sun appear to flatten on the horizon into an elliptical shape. Fig , p. 423
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Figure 15.15: The road in the photo appears wet because blue skylight is bending up into the camera as the light passes through air of different densities. Fig , p. 424
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Figure 15.16: Inferior mirage over hot desert sand.
Fig , p. 424
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Figure 15.16: Inferior mirage over hot desert sand.
Stepped Art Fig , p. 424
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Figure 15. 17: The formation of a superior mirage
Figure 15.17: The formation of a superior mirage. When cold air lies close to the surface with warm air aloft, light from distant mountains is refracted toward the normal as it enters the cold air. This causes an observer on the ground to see mountains higher and closer than they really are. Fig , p. 425
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Figure 15. 17: The formation of a superior mirage
Figure 15.17: The formation of a superior mirage. When cold air lies close to the surface with warm air aloft, light from distant mountains is refracted toward the normal as it enters the cold air. This causes an observer on the ground to see mountains higher and closer than they really are. Stepped Art Fig , p. 425
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Figure 15.18: A 22° halo around the sun, produced by the refraction of sunlight through ice crystals. Fig , p. 425
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Figure 1: The Fata Morgana mirage over water
Figure 1: The Fata Morgana mirage over water. The mirage is the result of refraction—light from small islands and ships is bent in such a way as to make them appear to rise vertically above the water. Figure 1, p. 426
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Figure 15.19: The formation of a 22° and a 46° halo with column-type ice crystals.
Fig , p. 426
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46° 46° Halo Line of sunlight 22° Halo 46° 22° 22° Editable Text
Figure 15.19: The formation of a 22° and a 46° halo with column-type ice crystals. 22° 22° Editable Text Fig , p. 426
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Figure 15.20: Halo with an upper tangent arc.
Fig , p. 427
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Figure 15.21: Refraction and dispersion of light through a glass prism.
Fig , p. 427
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Figure 15.22: Platelike ice crystals falling with their flat surfaces parallel to the earth produce sundogs. Fig , p. 427
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Apparent position of sundog Apparent position of sundog
22° 22° 22° Figure 15.22: Platelike ice crystals falling with their flat surfaces parallel to the earth produce sundogs. 22° Editable Text Fig , p. 427
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Figure 15.23: The bright areas on each side of the sun are sundogs.
Fig , p. 428
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Figure 15.24: A brilliant red sun pillar extending upward above the sun, produced by the reflection of sunlight off ice crystals. Fig , p. 428
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Figure 15.25: Optical phenomena that form when cirriform ice crystal clouds are present.
Fig , p. 429
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Figure 15.25: Optical phenomena that form when cirriform ice crystal clouds are present.
Stepped Art Fig , p. 429
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Figure 15.26: When you observe a rainbow, the sun is always to your back. In middle latitudes, a rainbow in the evening indicates that clearing weather is ahead. Fig , p. 429
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Figure 15.27: Sunlight internally reflected and dispersed by a raindrop. (a) The light ray is internally reflected only when it strikes the backside of the drop at an angle greater than the critical angle for water. (b) Refraction of the light as it enters the drop causes the point of reflection (on the back of the drop) to be different for each color. Hence, the colors are separated from each other when the light emerges from the raindrop. Fig , p. 430
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Sunlight 40° 42° (a) (b) Editable Text Fig. 15-27, p. 430
Figure 15.27: Sunlight internally reflected and dispersed by a raindrop. (a) The light ray is internally reflected only when it strikes the backside of the drop at an angle greater than the critical angle for water. (b) Refraction of the light as it enters the drop causes the point of reflection (on the back of the drop) to be different for each color. Hence, the colors are separated from each other when the light emerges from the raindrop. (a) (b) Editable Text Fig , p. 430
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Figure 15. 28: The formation of a primary rainbow
Figure 15.28: The formation of a primary rainbow. The observer sees red light from the upper drop and violet light from the lower drop. Fig , p. 430
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Raindrops Sunlight Red Violet Observer 40° 42° Editable Text
Figure 15.28: The formation of a primary rainbow. The observer sees red light from the upper drop and violet light from the lower drop. 40° 42° Editable Text Fig , p. 430
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Figure 15.29: A primary and a secondary rainbow.
Fig , p. 431
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Figure 15.30: Two internal reflections are responsible for the weaker, secondary rainbow. Notice that the eye sees violet light from the upper drop and red light from the lower drop. Fig , p. 431
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Falling raindrops Sunlight Violet Red Observer Editable Text
Figure 15.30: Two internal reflections are responsible for the weaker, secondary rainbow. Notice that the eye sees violet light from the upper drop and red light from the lower drop. Observer Editable Text Fig , p. 431
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Figure 15.31: The corona around the moon results from the diffraction of light by tiny liquid cloud droplets of uniform size. Fig , p. 431
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Figure 2: The series of rings surrounding the shadow of the aircraft is called the glory.
Figure 2, p. 432
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Figure 3: Light that produces the glory follows this path in a water droplet.
Figure 3, p. 432
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Sunlight Refracted ray Refracted light Refracted ray Editable Text
Figure 3: Light that produces the glory follows this path in a water droplet. Refracted ray Editable Text Figure 3, p. 432
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Figure 4: The Heiligenschein is the ring of light around the shadow of the observer’s head.
Figure 4, p. 432
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Figure 15. 32: Corona around the sun, photographed in Colorado
Figure 15.32: Corona around the sun, photographed in Colorado. This type of corona, called Bishop’s ring, is the result of diffraction of sunlight by tiny volcanic particles emitted from the volcano El Chichón in 1982. Fig , p. 433
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Figure 15.33: Cloud iridescence.
Fig , p. 433
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Figure 15.13: The bending of sunlight by the atmosphere causes the sun to rise about two minutes earlier, and set about two minutes later, than it would otherwise. Stepped Art
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