{"id":44,"date":"2022-04-27T07:12:54","date_gmt":"2022-04-27T11:12:54","guid":{"rendered":"https:\/\/pressbooks.library.upei.ca\/danceofphotons\/chapter\/photons-radiate\/"},"modified":"2022-05-12T17:40:24","modified_gmt":"2022-05-12T21:40:24","slug":"photons-radiate","status":"publish","type":"chapter","link":"https:\/\/pressbooks.library.upei.ca\/danceofphotons\/chapter\/photons-radiate\/","title":{"raw":"PHOTONS RADIATE","rendered":"PHOTONS RADIATE"},"content":{"raw":"
p. 13<\/div>\r\n
Most light sources (other than lasers) emit photons in all directions - namely they radiate<\/em><\/strong>. They tend to radiate more directly out from their surface and less to any side \"\"<\/div>\r\n

This is true for any point in a candle flame, on a glowing wire in a light bulb, and in a light emitting diode.<\/p>\r\nThe number of photons emitted in various directions from any point on an ideal<\/em><\/strong> source looks like this:\r\n\r\nThe line lengths are proportional to the number of photons in the ray (its<\/em><\/strong> intensity<\/em><\/strong>) in that direction.\r\n

e.g. The 60 degree ray has half the intensity of the direct ray.<\/p>\r\nIn 1760 Lambert found the decrease in photons at any angle could be estimated by multiplying the intensity of the direct ray by the angle\u2019s cosine.\r\n\r\nSurfaces the emit light in this manner are therefore called \u201cLambertian\u201d.\r\n\r\n \r\n

p. 14<\/p>\r\nThis radiation of photons from a source has serious consequences for lighting: The further the source, the weaker the radiation\u2019s strength<\/em> per<\/em> unit<\/em> area<\/em> (or illuminance<\/em><\/strong>, but that comes later, page 80): \"\"\r\n\r\nThe same number of photons reaching a square at 1 meter, spreads out over 4 squares\r\n\r\nat 2 meters, spreads over 9 squares at 3 meters, and so forth.\r\n\r\nBy simple geometry the number of photons per unit area decreases with distance squared.\r\n\r\nAt 3 times the distance, a light meter finds the illumination to be 1\/9 th of what it measured at 1 meter from a source.\r\n\r\nThus we have the Inverse<\/strong> Square<\/strong> Law<\/strong> describing the effectiveness of radiation at a distance.\r\n\r\n \r\n

p. 15<\/p>\r\n\r\n

Then why doesn\u2019t a candle look dimmer as you walk away?<\/em><\/strong><\/h3>\r\nThis question actually applies not only to candles or light bulbs, but also to everything we see.\r\n

The explanation (page 36) comes from physics not perception.<\/p>\r\n

However, that requires understanding some optics.<\/p>\r\nFirst, let\u2019s consider why it applies to (almost) everything we see:\r\n\r\n ","rendered":"

p. 13<\/div>\n
Most light sources (other than lasers) emit photons in all directions – namely they radiate<\/em><\/strong>. They tend to radiate more directly out from their surface and less to any side \"\"<\/div>\n

This is true for any point in a candle flame, on a glowing wire in a light bulb, and in a light emitting diode.<\/p>\n

The number of photons emitted in various directions from any point on an ideal<\/em><\/strong> source looks like this:<\/p>\n

The line lengths are proportional to the number of photons in the ray (its<\/em><\/strong> intensity<\/em><\/strong>) in that direction.<\/p>\n

e.g. The 60 degree ray has half the intensity of the direct ray.<\/p>\n

In 1760 Lambert found the decrease in photons at any angle could be estimated by multiplying the intensity of the direct ray by the angle\u2019s cosine.<\/p>\n

Surfaces the emit light in this manner are therefore called \u201cLambertian\u201d.<\/p>\n

 <\/p>\n

p. 14<\/p>\n

This radiation of photons from a source has serious consequences for lighting: The further the source, the weaker the radiation\u2019s strength<\/em> per<\/em> unit<\/em> area<\/em> (or illuminance<\/em><\/strong>, but that comes later, page 80): \"\"<\/p>\n

The same number of photons reaching a square at 1 meter, spreads out over 4 squares<\/p>\n

at 2 meters, spreads over 9 squares at 3 meters, and so forth.<\/p>\n

By simple geometry the number of photons per unit area decreases with distance squared.<\/p>\n

At 3 times the distance, a light meter finds the illumination to be 1\/9 th of what it measured at 1 meter from a source.<\/p>\n

Thus we have the Inverse<\/strong> Square<\/strong> Law<\/strong> describing the effectiveness of radiation at a distance.<\/p>\n

 <\/p>\n

p. 15<\/p>\n

Then why doesn\u2019t a candle look dimmer as you walk away?<\/em><\/strong><\/h3>\n

This question actually applies not only to candles or light bulbs, but also to everything we see.<\/p>\n

The explanation (page 36) comes from physics not perception.<\/p>\n

However, that requires understanding some optics.<\/p>\n

First, let\u2019s consider why it applies to (almost) everything we see:<\/p>\n

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