Photography is a dangerously gadget friendly environment. Stocked with hundreds of cool camera bodies, lenses and miscellaneous equipment, camera stores happily sell thousands of accessories. Add chemicals, development materials, printing accessories, computers, memory cards, special monitors and you end up with an empty wallet and far more headaches than you deserve. Or as some partners put it, all those headaches you do deserve. Often stated, boating is a hole in the water into which you throw money. Photography is a hole in the sky into which you throw not only money but perhaps your marriage, career, cat and sanity.

The first camera I used was one I liberated from my father. Equipped with a bellowed fixed lens, zero batteries and no focusing assistance, it sure was a curious little machine. Using medium format film in a body smaller than a Leica rangefinder, it took remarkable photos. Not only that, the absence of any modern convenience resulted in complete freedom from gadgets. In fact, available accessories numbered exactly zero. Those were the days.

The basic idea here is that gadgets don’t make photographs – not bad nor good ones. Photography is made possible by light. Light is preserved and eventually becomes viewable as a photograph. No gadget ever changed this basic notion. Light is about photography and photography is about light.

This post is largely an extract from my big essay on photography “On Reality 6: Mysteries of Photography“. Parts of the discussions update and expand the content of other previous posts, notably On Reality – Part 1 – Elements of Light and On Reality – Part 5 – How Perceptions and Illusions destroy Reality. Light Waves

Light is not a simple matter. Here are some of the theories dealing with light: Optics, Particles, Waves, Magnetics, Electrics, Relativity, Quantum, Wave-Particle, Electrodynamics, Radiation, Radiation and Light Pressure, Spectral, Ballistics, Photometry, Spectrometry, Lasers and much more. Yet the basic idea isn’t that complex.

Light is energy. This energy is emitted by sources such as the sun. Light energy consists of magnetic and electric waves traveling through space, atmosphere and some other media. The human eyes are sensitive to light waves. Our brains interpret the light energy as representing the world around us. A photograph captures the light present in a particular moment in time.

That Treacherous Light

Nothing is more important to a photographer than light. No light, no photography. As a photographer, you must love light. You Angus McBean Stage Actors in Profile better love how light bends, creates color, enters a lens, refracts, reflects, bounces, scatters, disappears, enters eyes for processing in the brain and how it is affected by sun spots, black holes, cosmic rays, global warming, atmosphere, clouds, rain, weather, pollution, dust and much else.

All of the factors above are distortions. The original light source, the sun for most practical purposes emits “pure” light. By the time that light reaches some place on Earth and your camera lens or eyes, it is very different compared to that original “pure” light. Light from space is distorted even before it reaches our atmosphere. Then the atmosphere adds its set of oddities. The camera is a virtual snake pit of distortions. Manmade light adds other distortions – its light is differently colored than the “norm”. Our eyes and brains add more layers of distortions.

Historical Light

In the beginning, people assumed one saw by emitting light beams out of one’s eyes. Pythagoras, 500 BC, assumed light traveled from the eyes and a sensationKGLPhoto High Rise At Night of seeing followed as the beam hit some object. Plato, 400BC, supported the same theory. Around 300BC, Euclid questioned that eyes were the only source of light and formulated quite a bit of light related mathematics. Still, the view of the eyes beaming light prevailed. The Bible mentioned “And God said, let there be light, and there was light”, associating light versus darkness as a good versus evil issue.

Around 1000AD, al-Haytham of Egypt finally voiced the idea that light entered the eyes rather than the other way around. He concluded the sun was the source of light. He also invented the Camera Obscura although Leonardo da Vinci received some of that credit 500 years later. Unfortunately, our gentleman resided in jail, so his findings were not immediately available. Most of his ideas were based on the sun light coming into his cell through a tiny opening or crack.

It took over 500 years before al-Haytham’s theories reached Europe, inspiring Kepler to formulate some fairly correct theories late in the 1500s. Galileo, Descartes and Newton added tremendously to the understanding of light over the next 100 years. The wave theory came along through Euler in the mid 1700s. Other contributors include Fresnel, Poisson, Faraway, Planck and Maxwell, leading up to the late 1800s and pretty much the way we understand light today.

A Simple Theory of Light

Light is produced by light emitters, reflected by certain objects and consumed by others. Light is radiation energy affected by combinations of photons, atoms, molecules and KGLPhoto WSindow at Night with a Truckother low lives. It has characteristics such as wave length, frequency and intensity, all of which vary tremendously with quite spectacular results. Most light originates at the sun and manmade processes. Light may be a single beam or scattered in a collision with some obscure molecules.

Radiation is a form of energy with intensity and wave length, vibrating around us constantly. Low frequency waves represent sound. There are TV and radio waves, visible and invisible light, radar waves, cellular phone radiations and X-ray emissions. Light as we see it and as used by a camera is only a small part of the energy waves around us. In some cases, invisible wave lengths affect film or memory cards in undesirable ways. Don’t X-ray your films. A rather extreme example is the HEMP bomb that can fry all electronics within a large radius; including your camera (unless you use a camera similar to that of my father, but even so, the film is probably a goner).

Light is created in many ways – the sun maintains a controlled nuclear explosion emitting lots of radiation energy, some in the form of light, other in the form of quite deadly variations such as gamma rays. Light bulbs, neon lights and many other manmade devices emit light on demand. Such light is usually created by the combination of energy in an enclosure containing suitable gases. Other light sources include computer, radar and TV screens which operate using cathode rays and energy sensitive coatings or by turning KGLPhoto Security on a Walltransistors off and on. Nuclear reactions produce lots of radiation, some of which is visible.

Heat generates light; increasingly hot temperatures transform light from the original color to a glow of red, white and eventually blue – think about your stove, fireplace, kerosene lamp or volcanic lava. Military night sights use slight heat variations as emitted in the infrared spectrum to “see” a battle field. Chemical processes generate light in some organisms: fireflies, glow worms, krill and others. Lightning produces a short burst of light based on heat.

When light falls on an object, some waves with a specific length are reflected and others absorbed. Light emitted by an object also have a specific set of wave lengths. We perceive the light of a specific wave length as a color. We thus “see” the object having a color. The reflected light is not a constant since it depends of the wave lengths of the incoming light. Reddish sunset light makes any object look reddish while the same object is bluish at noon.

Photographers and light meter manufacturers make a big deal out of incident and reflected light. Incident light measures incoming light only and then make assumptions about correct exposure. Reflected readings do the same for reflected light. The problem is that different object reflect light very differently – snow, water and any light object reflects much more light than dark soil, a black cat or any dark object. That means that neither incident nor reflected light measures result in a correct exposure. In the case of snow, an KGLPhoto Street Light Over Bushesincidence measure will overexpose the scene while a reflected metering will underexpose the same scene. The only time you get a good measure is when the scene is a uniform 18% grey – a very rare occurrence.

Auto exposure cameras use only reflected light as does the Zone System. Popularized by Ansel Adams, the Zone System attempts to correct the ambiguity in light measures. In fact, that is the major point of the Zone System.

Meanwhile, the auto exposure camera relies on you to override its automatics to produce a correct reading. Nothing automatic about that, is it?

Most objects are not producing light at all. They are only visible because they reflect light. A chair does not normally emit light. The moon does not produce light – it solely reflects light mostly from the sun. There is a bit of a fallacy here because heat produces light. Heat the chair up and it will produce light. Humans do not produce light but we (and animals) have a body temperature that does cause light emissions in the invisible infrared spectrum. If we actually turned into visible light emitters we are very dead because that implies heat sufficient to make us glow red – blue – white. That would not be healthy. However, it is possible to photograph people in total darkness. All you need is a readily available sensor or film sensitive to infrared light.

Light intensity declines rapidly with distance. Most photographers use a simple formula stating: double the distance from a light source and the KGLPhoto Laughing Lady in the Darkintensity is down to a 1/4 of the original intensity. That is an approximation that serves photography well in most circumstances but is actually wildly inaccurate. If you get close to a light source, then light intensity to distance is almost flat regardless of distance. Nor does the rule hold up when the light is focused with some sort of reflector as you may have noticed using a flashlight, driving at night or watching the beam from a lighthouse.

Light never dies. As time goes by and the light travels great distances, the intensity goes down but it never reaches zero. We are surrounded by light originating billions of years ago. Unfortunately, the intensity is way down making it impossible to see for us humans. The Hubble telescope is extremely light sensitive and can pick up very distant light originating a long time ago.

There is no such thing as “seeing” an object; our eyes only receive light emitted and reflected by the object. The light waves reaching our eyes are quite distorted. The eyes introduce more distortions due to various imperfections. The brain then makes up a “view” of the object, introducing additional distortions. The brain is easily fooled into providing false or biased views. What we “see” is not an accurate representation of the object, it merely is one deemed safe by our brain.

Light Traveling Space

The sun is our major source of light. This light is comes from a massive nuclear reaction that has been going on for billions of years. Sun light affects human health and climates. The current Global Warming crisis is caused by sun energy being trapped by CO2 concentrations rather than reflected back into space, which causes temperatures to rise to dangerous levels. Sun light produces Vitamin D and fuels millions of energy requirements. It also causes skin cancers and ultraviolet KGLPhoto Tending the Shopradiation aging us. The sun will very certainly cause the demise of mankind, possibly through Global Warming but for sure as its energy runs out.

Stars, clusters, galaxies and nebulae provide some light. Polar lights (Aurorae) are clearly visible in high latitude areas and seasons. The moon reflects sun light. Magnetic fields in space bend light, space storms distort light, black holes does who knows what with light and sun flares send out a lot of unpredictable and usually harmful energy.

Cosmic “rays” refer to Earth being bombarded by energy containing particles. These particles originate with the sun but also exploding stars, novae, galaxies, quasars and black holes. These generally low energy (unless you are an astronaut) particles have some limited effect on climate by affecting lightning and cloud formation. Solar cosmic rays can affect electronics on Earth such as communication devices and possibly digital cameras. Then there is the Oh-My-God particle (really) traveling around the Universe at extreme speed and containing enormous KGLPhoto Blues Musician in a Wheelchairenergy, given its tiny size. But that is another story.

Photography in space is quite different than on earth. The radiation levels are harmful to film. NASA tests film extensively to reduce fogging and color shifts – they tend to use film specially made for them by Kodak. Today I’m sure they use digital cameras with similar quality considerations.

Light in space is either on or off with photography taking place when light is on. With the light is on, it is very constant – no clouds, haze, rain storms or shadow. There are only two basic shooting scenarios: close or far. Shooting earth from the space station means using one standard exposure (reflected light is quite constant) and the lens set at infinity. Shooting “close ups” such as space walks require a similar standard exposure and some focusing. Photography inside the space vessel is similar to that on earth.

Space light is much bluer than on earth. There is far more ultraviolet radiation which is not visible with eyes but may impact images. Contrast ranges are extreme – consider an astronaut in a white suit against a pitch black background. The seasoned space photographer must also consider speed. Everything moves way faster than earth speed limits. The shuttle moves at 17,500 miles an hour (5 miles per second or 110 feet a typical exposure of 1/240 seconds) so panning is a necessary skill. The Cartier-Bresson Decisive Moment takes on a different meaning. In space, a photograph doesn’t freeze a moment in time. It records a sequence of movement

Atmosphere and Time

The atmosphere greatly impacts light from space. Distortions include seasonality, clouds, storms, humidity, dust, pollution, inversion layers, refractions and reflections. Other factors Robert Doisneau Baldaccini Portraitinclude time of day effects and temperature distortions.

When light beams reach the atmosphere, they scatter as they collide with atmospheric particles. During the day, this results in a blue sky because the light is coming from a high angle. In the early morning and evening with a low sun, we see a reddish sky because the angle of the incoming beams is low. Without clouds, we experience a mix of sun beams and scattered light. Snow, water and beach sand reflect light more than dark objects. That elevated light level reaches your camera and confuses the light meter. You better reduce the exposure. Ice also reflects light but amplifies the blue wave lengths. Thus, photos of ice bergs usually have a deep bluish tint.

Seasons display unique light effects. Snowy landscapes require special attention to exposure. Fall foil colors can overwhelm a landscape. Some enjoy the Christmas feeling Charles Gatewood Box on Endand warm toned nostalgia. Seasonal sports and graduations are popular events. Some regions suffer extreme weather seasons such as the Arctic winter, the hurricane plagued Southeast US coasts, the mid US Tornado Alley and the Asian Monsoon and Cyclone season.

Clouds reflect the direct sun beams and all we see is the scattered light waves – shadows disappear or dilute. The water content of the clouds scatter light in a way that produces no particular color, hence the grayish feel with a complete cloud cover. The thicker the cloud, the less light passes through. Extreme weather can lead to almost total darkness and a general loss in color. The red rose is suddenly grey.

Bounces and Refractions

Refraction of light is the bending effect that happens when light passes through certain Edward Weston Oceano - Desert Lightmedia at certain angles. The straw in a glass of water is the classic example. Refraction is, for instance, the cause of rainbows. The atmosphere provides refraction of sun beams: the lower the sun, the more the refraction. At sunset the refraction can be as much as half a degree or about one sun diameter. This explains the “oval” sun at sunset or dawn. Another effect of refraction is the “floating mountains” or “elonged islands or ships” seen on hot days (Fata Morgana). Other special effects include mirages and the common illusion of distant pools of water on hot roads. Refraction also makes it possible to see beyond the natural horizon.

Refraction in a vacuum is exactly 1.0, which means there is no refraction. The atmosphere has a refraction of 1.0003 while ordinary Ansel Adams Clearing after the Stormwater refracts 1.33, quite a bit more. Acrylic glass has a refraction index of 1.49 and diamonds are at 2.42. Silicon has an index of over 4 although that probably won’t be much of a photography issue.

Refraction also is important because different wave lengths of light have slightly different refractions in different materials. This causes dispersion of the light into colors. Diamonds, for instance, are very high in dispersions causing their extraordinary “fire”. One moment you see blue light reflected from the stone, then perhaps green or pure white. Rainbows are another example of this phenomenon. Reflection, dispersion and refraction are the mechanisms by which many different kinds of prisms work – very important design aspects of your camera’s lenses.

Pollution and Dust

Atmospheric pollution affects light. Compare light in a smogged Los Angeles, Mexico City or Shanghai to that experienced on top of Mauna Kea in Hawaii. Broadly, there are three Haze over Hong Kongkinds of atmospheric pollution agents. Some reflect solar beams back out into space, resulting in less light and cooler temperatures. The sulphur dioxide crisis of the 1960s and early 1970s is a good example. Other pollutants, such as carbon dioxide, do the opposite – they allow the sun energy to pass to the surface of Earth but disallow the required reflection of excess energy back out into space. The result is Global Warming. Yet another pollutant, typically Freon, destroy the ozone layer allowing ultraviolet light through at levels threatening health.

Here are the smoggiest cities: London, New York, Los Angeles, Mexico City, Houston, Toronto, Athens, Beijing and Hong Kong. Smoggy areas include the Ruhr Area and Silicon Valley and many places in China, Southeast Asia and India. Forest slash and burn practices in Indonesia cause severe smog and smoke in much of surrounding countries. The disastrous 1952 smog in London killed 4,000 people in four days, followed by another 8,000 in the next six months. On a happier note, both LA and Mexico City have made substantial advances in controlling smog.

Apart from the health issues, heavy smog can easily make any normal photography impossible.

Dust in the atmosphere typically reflects sun energy back out and thus has a cooling effect as well as a darker sky. Sunsets tend to be tremendous. Volcanoes cause massive emissions of dSmog on the Rtiverust, particles and ashes into the atmosphere. The eruptions of Mount St. Helen and Mount Pinatubo spewed out ashes that traveled the world for several years. Dust storms due to drought are another major source. The Oklahoma storms of the 1930s, today’s Sahara storms and those of China affect all of Earth. Global Warming will amplify dust storms due to extreme droughts. Yet another source of particles in the air stems from forest fires due to deforestation in Brazil, Malaysia and, above all, Indonesia. The uncontrolled fires in Indonesia cause severe health problems in not only Indonesia but all of Southwest Asia. The particles circle the

Manmade Light

Natural light is terrific to photographers. Manmade light is a pain. Hundreds of different devices, lamps, bulbs, processes, materials, gases and energy sources result in the strangest of light spectra. Add that manmade light is generally there because the natural light is not available. You are stuck with the darn thing. True, you can set up your own light version Diane Arbus Queen and Kingwith all kinds of expensive photographic lighting devices. That’s fine but really what you do is to replace one manmade environment with another manmade environment.

K (Kelvin) values and wave spectra are important to photographers. A K value is an average of a light source’s color spectrum. A spectrum provides much more information about the scene than does the K value. For instance, the spectrum may have a high wave length peak and a low peak – a ‘U’ pattern. The K value will fall between the peaks and not really mean a thing. What you need is, perhaps, double filtration to correct for the two peaks.

The K value of sunlight is about 5,800. Typical daylight is either 5,000K or 6,500K depending on if you go for the US standard calibration or that of Europe. Computer monitors are calibrated to between 5,000K (reddish yellow) and 9,300K (bluish). Digital cameras often display white balance settings in terms of Kelvin values. In the spectrum of colors, red is around 1,800K, the average is 5,000K to 6,500K and blue starts around 12,000K continuing up to 16,000K. Examples of low Kelvin light: Match flares, candles and ordinary (tungsten) light bulbs. Here are some high Kelvin items: Xenon light, analog TVs: “the bluish flicker from you neighbor’s window”. Henri Cartier-Bresson The Duke of Windsor with Divorcee Wife

Unless going for abstraction, photographers compensate for the local K value/spectrum to bring the image back to “normal”. For instance, you try to make skin tones similar to those recorded in regular daylight. That may be accomplished through lens filters, white balance adjustments or post production trickery. When you do that, obviously the original scene is distorted – the ugly manmade light was, after all, the real thing.

Most fluorescent and gas discharge lamps have “interrupted spectra”, meaning the spectra are not smooth curves but a series of narrow peaks over the frequency band. Such irregular peaks, often in the yellow to green range, are very hard to filter away. The only real solution is to use alternative lighting such as flash. Gas discharge lamps include neon light and high intensity lights (mercury vapor, metal halide and sodium vapor) as used in light streets, stadiums and factories.

Then there is another issue. Film or sensors react quite differently to odd light situations than do your eyes. Your eyes and brain compensate for strange light to make it more consistent with your built in database on how a face “should” look. A camera has no such database or ability. It records incoming light according to its fixed sensitivity to different wave lengths.


Are shadows the opposite of light? Of course not, shadows are light just as is present elsewhere. They are a bit darker, that’s all. Zone system proponents know all about shadows being as important as high lights. The old film saying is: “expose for shadows, develop for high lights”. Or, in the case of digital photography, do the reverse, i.e. shoot for high lights and balance shadow detail in Photoshop.

The dynamic range of light in photography is typically measured in f stops. If the ratio of Henri Cartier-Bresson Man and His Shadowlight intensity in high lights compared to minimum light is, say 1024:1, or 2 raised to the power of 10, then the range is 10 stops. There is a huge difference in the ranges different media are capable of recording or displaying. Your eyes are amazing in that not only can they cover the largest dynamic range, they also are self adjusting in real time. Other devices don’t even come close.

On a cloudy day a scene may display a dynamic range of as little as 3 stops. On a sunny day, the same scene may display a range of 12 stops. That is well within the capabilities of most eyes. Eyes can dynamically adjust to a 24 stop range although a more static range of 10-14 stops is more realistic. Most cameras (film and digital) can handle a range of about 8 stops, a considerable reduction. A typical print covers about 6 stops and a monitor slightly less. Newspapers can only display a range of 3-4 stops.

Several techniques and technologies exist to extend either the original or the displayed range. One recent example is High Dynamic Range Photography. In traditional photography, special development techniques coupled with corresponding exposures can do the trick. Consider the Hubble telescope and its ability to record and then enhance the dimmest of light.

In practical, everyday photography, the biggest factor in getting a decent dynamic range is simply to use correct exposures. Over or under exposure quickly destroys the dynamic range. One stop overexposure loses one stop of range on the high light side. Please note that correct exposure is not the same as pointing your camera at something and letting the built-in light meter (or for that matter an external meter) blurb out some numbers. Light meters are very stupid about measuring light. Practice, practice so you truly understand exposure. Otherwise, your shadows or high lights are off, were off and will stay off, blowing you out of the water every time.

Using Light

Now that you know a little bit about light, how do you use that knowledge? In generic terms, the benefit of this knowledge is that you know more about what to expect. Make that an element in your photographic execution. Industrial ShapePhotography in big cities usually means polluted air which produces a different light than that on top of Mount Everest. If you shoot in an ice cave, the light is blue, while if you shoot in a sand cave, the light is reddish. Indoor shooting at, say, Christmas, will probably produce warm, reddish photos. Shooting on a lit street may produce very strange color casts.

We do not know all there is to know about light – much remains a mystery. The current knowledge is recent or no more than a hundred years old. Yet we speak of light with deep convictions, especially in photography. An image “captures” the light, a print contains the “full range” of light, the light reflected from a face “accurately” captures the skin tones. Professional critics have a language, of their own but incomprehensible to many of us, classifying and judging light and how a photographer deals with it in his art.

A photographer can use tools to analyze light. The intensity of light falling on a subject or reflected from a subject into the lens is easily measured. He/she can even determine the color of light falling on the subject. Once the picture is taken the image can be analyzed either with software in the case of digital images or by a densitometer in the case of film. That is all fine, but no meters will ever tell the full story and in fact they may even hide the real magic.

The true story about light is not one of analysis. It is about the creative use of light presented at a particular shooting event. To create that vision, you need to realize light is not just one thing. It is a combination of many different kinds of effects and distortions. Once that is clear, here are a few ideas that you might use to figure out your very own creative toolbox. A tool box is an individual treasure chest. What is a trap to some is an opportunity to others. We are all as different as are our visions. So take the following as nonexclusive ideas, not sinister laws.

  • History and Theory: The history of our understanding of light is long, colorful and by no means finished. The “seeing” interaction of eyes and brain is only partially, and very recently, understood and no doubt inaccurate. Think about the significance of all those tricky images designed to fool the brain – where straight lines suddenly look bent. Or where stationary images impossibly start to move? In your fooled brain, that is.
  • Space: Most natural light comes from space. As light travels through space, it undergoes Edward Weston Kneeling Nudetransformations, most quite subtle. It bends, gets malformed, disappears, reflects, is colored and ends up differently than expected in largely a random, uncontrolled manner. Light in its “cleanest” form is quite variable even if you reside on the International Space Station. The atmosphere is then doing it’s best to make matters even more complex:
  • Atmosphere: The atmosphere shields us from a quite harmful space environment. The ozone layer filters out UV radiation. Space is filled with particles harmful to humans that have come close to killing astronauts. These particles luckily do not penetrate the atmosphere. As the atmospheric filters do their work, light from space becomes even more modified. Then local conditions change light again, either by less filtering or more. A photograph taken in Australia or in Antarctica may be subject to a lot more UV light than elsewhere. A picture shot from an airplane at 37,000 feet is subject to more bombardment of essentially radioactive particles than one taken in Times Square, New York.
  • Refraction: Light bends as it passes through certain media such as water or a lens. This leads to many special situations and opportunities, whether you appreciate oval suns, mirages, Fata Morgana, rainbows, floating mountains or tilting buildings. You figure it out. Make a list of the special situations created by refraction in your shooting environment.
  • Reflections: We all have many so-so shots of tall buildings reflecting wobbly images from their glass walls. And those self portraits using a mirror belong deep in that shoe box in the garage. We realize Edward Weston Veggieshow reflections from snow and water may be controlled by polarizing filters. Portrait photographers use reflectors to create a pleasing light. Film and TV crews do the same. Daylight may be modified by fill flash to create an illusion of reflections. Reflections, in any type of photography, represent huge and under used opportunities for creativity. Think about it. Create you own sun! Make your own shadows!
  • Time of Day: Time of day is an essential tool. Most photographs can only be successfully shot at very specific light conditions, whether it is due to the light intensity or its color balance. Examples: Rarely is noon light the best for nature photography. Long shadows may accentuate the emotional impact of a scene. Some animals are only reachable at certain hours. Downtown traffic is busier at rush hours. Indoors, the uses of ambient light through windows depend not only on time of day but also on the angle to the sun. At noon, light from a south facing window is quite different from a window facing north.
  • Seasonal: Many of us associate seasons with specific events. You shoot fall colors as leaves fall. Or delicate spring colors as leaves return. Cherry trees bloom. Whales, salmon and birds migrate. Grizzlies wake up or retire. Frozen lakes thaw. Change your wardrobe. The barbeque is manned. The car gets its annual wash. The first strawberries show up. Taste the Beaujolais Nouveau or fresh halibut. Eat your heart out at Thanksgiving. Do the Christmas shopping. Snowmobiles, motor cycles or power boats roar. Sailboats tack. Dust off the camera after its winter slumber. Wash the windows, cut the lawn. File April tax returns. Harvest the apples, wheat and oranges. Does you vision include such items and more?
  • Weather: Nature gives us hurricanes, tornados, cyclones, fog, heavy rain, soft rain, clouds, thunder, lightning, sunshine, snow fall, heat waves or cold spells. The impact on your creative situation and challenge is obvious. Weather not only impacts light, it affects the range of possible or desired subjects. Some like shooting close up pictures of tornados. Most of us prefer to run like hell.
  • Pollution and Dust: Imagine grabbing your camera, crawling into your bed and under the covers.Edward Weston More Veggies Try taking a photograph of your left foot. That’s not real easy, is it? The bloody covers filter out the light. So do pollution and dust, both of which consist of airborne particles (and perhaps gases), covering earth like a blanket. Both reduce light coming through and both modify the color of light. Dramatic pictures from hazy Shanghai are perhaps interesting but not real artistic in most cases. The thing is, not all light effects are desirable in the sense they create creative opportunities. Some are simply bad news to most photographers. Here is another example:
  • Manmade Light: Speaking photographically, manmade light is a pest unless specifically created for photographic purposes. Blast that sodium light. Darn that fluorescent office light. Curse those wave length peaks and valleys. Green faces, orange hair. What is fun about lobster red skin? Well, nothing much. Maybe useful in some artistic visions, manmade light is a curse to most photographers.

There you are – you have a shopping list for your magical light tool box and a list of features to think about. This discussion of possible opportunities could go on much longer. It won’t, at this moment. The main idea still is that you are the one to create your own box, preferably by thinking outside the box. Try it on. Now, let’s check out colors which are just one form of light.

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