Posted on May 12, 2019
I returned Friday from my annual Grand Canyon Raft Trip for Photographers and am playing catch-up on all aspects of my photography life. I’ve barely looked at the my raft trip images, but chose this one for a couple of reasons: first, because I think it perfectly conveys the intimate serenity that always catches me by surprise in this landscape known mostly for it’s broad vistas; and second, because it’s the only image I’ve processed so far.
This is Blacktail Canyon, one of hundreds (thousands?) of narrow slot canyons cutting into the Grand Canyon’s towering walls. Most of them we just float past, sometimes because of the physical challenges required to explore their depths, but usually because there just isn’t time to stop at every slot canyon. On my trips we pick our slots for their photo opportunities, and this year Blacktail Canyon was a particular highlight.
With tall, tightly spaced walls, Blacktail Canyon spends most of its daylight hours in full shade, ideal for photography on sunny days. It doesn’t always have water, but this year’s wet winter meant water in lots of places that don’t always get it. We found the little creek that splits the canyon carrying just enough water to create a series of reflective pools before disappearing into the stream bed, only to reappear farther downstream.
What first drew my eye to this scene was a tiny sapling sprouting from an overhanging ledge, but I soon realized that the tree would best serve me as a visuall element to hold the top of my frame rather than the primary subject. The most interesting thing, I decided, was the blue sky reflection like a jewel embedded in the creek bed.
To create this composition, I dropped my tripod to about a foot above the canyon floor and positioned myself so the lines connecting my primary focal points (the sky reflection, the pair of boulders, and the green tree) created a triangle. Fitting all this into the frame required a vertical orientation of my Sony a7RIII, using virtually the entire width of my Sony 16-35 f/2.8 G lens. Even at this wide focal length, the smooth pebbles at my feet were only about a foot away; getting both the nearby pebbles and glowing (from bounced sunlight) sandstone above the tree sharp, meant choosing my exposure settings and focus point very carefully. My hyperfocal app told me that at f/16, by focusing two feet away, I could achieve my sharpness goal. Watching the rapidly changing sky, I timed my click for the best blend of clouds and sky filling the reflection.
What’s the point?
It seems like one of photography’s great mysteries is achieving proper focus: the camera settings, where to place the focus point, even the definition of sharpness are all sources of confusion. If you’re a tourist just grabbing snapshots, everything in your frame is likely at infinity and you can just put your camera in full auto mode and click away. But if you’re a photographic artist trying to capture something unique with your mirrorless or DSLR camera and doing your best to have important visual elements objects at different distances throughout your frame, you need to stop letting your camera decide your focus point and exposure settings.
Of course the first creative focus decision is whether you even want the entire frame sharp. While some of my favorite images use selective focus to emphasize one element and blur the rest of the scene, most (but not all) of what I’ll say here is about using hyperfocal techniques to maximize depth of field (DOF). I cover creative selective focus in much greater detail in another Photo Tip article: Creative Selective Focus.
Beware the “expert”
I’m afraid that there’s some bad, albeit well-intended, advice out there that yields just enough success to deceive people into thinking they’ve got focus nailed, a misperception that often doesn’t manifest until an important shot is lost. I’m referring to the myth that you should focus 1/3 of the way into the scene, or 1/3 of the way into the frame (two very different things, each with its own set of problems).
For beginners, or photographers whose scene doesn’t include subjects from near to far, the 1/3 technique may be a useful rule of thumb. But taking the 1/3 approach to focus requires that you understand DOF and the art of focusing well enough to know when 1/3 won’t work, and how to adjust your focus point and settings. And once you achieve that level of understanding, you may as well do it the right way from the start. Focus control becomes especially important in those scenes where missing the focus point by just a few feet or even inches can make or break and image.
Back to the basics
Understanding a few basic focus truths will help you make focus decisions:
Depth of field discussions are complicated by the fact that “sharp” is a moving target that varies with display size and viewing distance. But it’s safe to say that all things equal, the larger your ultimate output and closer the intended viewing distance, the more detail your original capture should contain.
To capture detail a lens focuses light on the sensor’s photosites. Remember using a magnifying glass to focus sunlight and ignite a leaf when you were a kid? The smaller (more concentrated) the point of sunlight, the sooner the smoke appeared. In a camera, the finer (smaller) a lens focuses light on each photosite, the more detail the image will contain at that location. So when we focus we’re trying to make the light striking each photosite as concentrated as possible.
In photography we call that small circle of light your lens makes for each photosite its “circle of confusion.” The larger the CoC, the less concentrated the light and the more blurred the image will appear. Of course if the CoC is too small to be seen as soft, either because the print is too small or the viewer is too far away, it really doesn’t matter. In other words, areas of an image with a large CoC (relatively soft) can still appear sharp if small enough or viewed from far enough away. That’s why sharpness can never be an absolute term, and we talk instead about acceptable sharpness that’s based on print size and viewing distance. It’s actually possible for the same image to be sharp for one use, but too soft for another.
So how much detail do you need? The threshold for acceptable sharpness is pretty low for an image that just ends up on an iPhone or an 8×10 calendar on the kitchen wall, but if you want that image to fill the wall above the sofa, acceptable sharpness requires much more detail. And as your print size increases (and/or viewing distance decreases), the CoC that delivers acceptable sharpness shrinks correspondingly.
Many factors determine the a camera’s ability to record detail. Sensor resolution of course—the more resolution your sensor has, the more important it becomes that to have a lens that can take advantage of that extra resolution. And the more detail you want to capture with that high resolution sensor and tack-sharp lens, the more important your depth of field and focus point decisions become.
The foundation of a sound approach to maximizing sharpness for a given viewing distance and image size is hyperfocal focusing, an approach that uses viewing distance, f-stop, focal length, and focus point to ensure acceptable sharpness.
The hyperfocal point is the focus point that provides the maximum depth of field for a given combination of sensor size, f/stop, and focal length. Another way to express it is that the hyperfocal point is the closest you can focus and still be acceptably sharp to infinity. When focused at the hyperfocal point, your scene will be acceptably sharp from halfway between your lens and focus point all the way to infinity. For example, if the hyperfocal point for your sensor (full frame, APS-C, 4/3, or whatever), focal length, and f-stop combinition is twelve feet away, focusing there will give you acceptable sharpness from six feet (half of twelve) to infinity—focusing closer will soften the distant scene; focusing farther will keep you sharp to infinity but extend the area of foreground softness.
Because the hyperfocal variable (sensor size, focal length, f-stop) combinations are too numerous to memorize, we usually refer to an external aid. That used to be awkward printed tables with long columns and rows displayed in microscopic print, the more precise the data, the smaller the print. Fortunately, those have been replaced by smartphone apps with more precise information in a much more accessible and readable form. We plug in all the variables and out pops the hyperfocal point distance and other useful information
It usually goes something like this:
You’re not as sharp as you think
Since people’s eyes start to glaze over when CoC comes up, they tend to use the default returned by the smartphone app. But just because the app tells you you’ve nailed focus, don’t assume that your work is done. An often overlooked aspect of hyperfocal focusing is that app makes assumptions that aren’t necessarily right, and in fact are probably wrong.
The CoC your app uses to determine acceptable sharpness is a function of sensor size, display size, and viewing distance. But most app’s hyperfocal tables assume that you’re creating an 8×10 print that will be viewed from a foot away—maybe valid 40 years ago, but not in this day of mega-prints. The result is a CoC three times larger than the eye’s ability to resolve.
That doesn’t invalidate hyperfocal focusing, but if you use published hyperfocal data from an app or table, your images’ DOF might not be as ideal as you think it is for your use. If you can’t specify a smaller CoC in your app, I suggest that you stop-down a stop or so more than the app/table indicates. On the other hand, stopping down to increase sharpness is an effort of diminishing returns, because diffraction increases as the aperture shrinks and eventually will soften the entire image—I try not to go more than a stop smaller than my data suggests.
Keeping it simple
As helpful as a hyperfocal app can be, whipping out a smartphone for instant in-the-field access to data is not really conducive to the creative process. I’m a big advocate of keeping photography as simple as possible, so while I’m a hyperfocal focus advocate in spirit, I don’t usually use hyperfocal data in the field. Instead I apply hyperfocal principles in the field whenever I think the margin of error gives me sufficient wiggle room.
Though I don’t often use the specific hyperfocal data in the field, I find it helps a lot to refer to hyperfocal tables when I’m sitting around with nothing to do. So if I find myself standing in line at the DMV, or sitting in a theater waiting for a movie (I’m a great date), I open my iPhone hyperfocal app and plug in random values just to get a sense of the DOF for a given f-stop and focal length combination. I may not remember the exact numbers later, but enough of the information sinks in that I accumulate a general sense of the hyperfocal DOF/camera-setting relationships.
Finally, something to do
Unless I think I have very little DOF margin for error in my composition, I rarely open my hyperfocal app in the field. Instead, once my composition is worked out and have determined the closest object I want sharp—the closest object with visual interest (shape, color, texture), regardless of whether it’s a primary subject.
Of course these distances are very subjective and will vary with your focal length and composition (not to mention the strength of your pitching arm), but you get the idea. If you find yourself in a small margin for error focus situation without a hyperfocal app (or you just don’t want to take the time to use one), the single most important thing to remember is to focus behind your closest subject. Because you always have sharpness in front of your focus point, focusing on the closest subject gives you unnecessary near sharpness at the expense of distant sharpness. By focusing a little behind your closest subject, you’re increasing the depth of your distant sharpness while (if you’re careful) keeping your foreground subject within the zone of sharpness in front of the focus point.
And finally, foreground softness, no matter how slight, is almost always a greater distraction than slight background softness. So, if it’s impossible to get all of your frame sharp, it’s usually best to ensure that the foreground is sharp.
Why not just automatically set the aperture to f/22 and be done with it? I thought you’d never ask. Without delving too far into the physics of light and optics, let’s just say that there’s a not so little light-bending problem called “diffraction” that robs your images of sharpness as your aperture shrinks—the smaller the aperture, the greater the diffraction. Then why not choose f/2.8 when everything’s at infinity? Because lenses tend to lose sharpness at their aperture extremes, and are generally sharper in their mid-range f-stops. So while diffraction and lens softness don’t sway me from choosing the f-stop that gives the DOF I want, I try to never choose an aperture bigger or smaller than I need.
Now that we’ve let the composition determine our f-stop, it’s (finally) time to actually choose the focus point. Believe it or not, with this foundation of understanding we just established, focus becomes pretty simple. Whenever possible, I try to have elements throughout my frame, often starting near my feet and extending far into the distance. When that’s the case I stop down focus on an object slightly behind my closest subject (the more distant my closest subject, the farther behind it I can focus).
When I’m not sure, or if I don’t think I can get the entire scene sharp, I err on the side of closer focus to ensure that the foreground is sharp. Sometimes before shooting I check my DOF with the DOF preview button, allowing time for my eye to adjust to the limited light. And when maximum DOF is essential and I know my margin for error is small, I don’t hesitate to refer to the DOF app on my iPhone.
A great thing about digital capture is the instant validation of the LCD—when I’m not sure, or when getting it perfect is absolutely essential, after capture I pop my image up on the LCD, magnify it to maximum, check the point or points that must be sharp, and adjust if necessary. Using this immediate feedback to make instant corrections really speeds the learning process.
Sometimes less is more
The depth of field you choose is your creative choice, and no law says you must maximize it. Use your camera’s limited depth of field to minimize or eliminate distractions, create a blur of background color, or simply to guide your viewer’s eye. Focusing on a near subject while letting the background go soft clearly communicates the primary subject while retaining enough background detail to establish context. And an extremely narrow depth of field can turn distant flowers or sky into a colorful canvas for your subject.
There’s no substitute for experience
No two photographers do everything exactly alike. Determining the DOF a composition requires, the f-stop and focal length that achieves the desired DOF, and where to place the point of maximum focus, are all part of the creative process that should never be left up to the camera. The sooner you grasp the underlying principles of DOF and focus, the sooner you’ll feel comfortable taking control and conveying your own unique vision.
About this image
Yosemite may not be New England, but it can still put on a pretty good fall color display. A few years ago I arrived at Valley View on the west side of Yosemite Valley just about the time the fall color was peaking. I found the Merced River filled with reflections of El Capitan and Cathedral Rocks, framed by an accumulation of recently fallen leaves still rich with vivid fall color.
To emphasize the colorful foreground, I dropped my tripod low and framed up a vertical composition. I knew my hyperfocal distance at 24mm and f/11 would be 5 or 6 feet, but with the scene ranging from the closest leaves at about 3 feet away out to El Capitan at infinity, I also knew I’d need to be careful with my focus choices. For a little more margin for error I stopped down to f/16, then focused on the nearest rocks which were a little less than 6 feet away. As I usually do when I don’t have a lot of focus wiggle room, I magnified the resulting image on my LCD and moved the view from the foreground to the background to verify front-to-back sharpness.
Click an image for a closer look and slide show. Refresh the screen to reorder the display.
Posted on April 17, 2019
The annual Grand Canyon monsoon is known for its spectacular electrical storms, but let’s not forget the rainbows that often punctuate these storms. A rainbow requires rain, sunlight, and the right viewing angle—given the ephemeral nature of a monsoon thunderstorm, it’s usually safe to assume that the sun probably isn’t far behind. To experience a rainbow after a Grand Canyon monsoon storm, all it takes is some basic knowledge, a little faith, and some good fortune.
To help with the knowledge part, I’m sharing the how-and-why of rainbows, excerpted from my just updated Rainbow article in my Photo Tips section. For the faith and good fortune part, read “The story of this image” at the bottom of this post.
Most people understand that a rainbow is light spread into various colors by airborne water drops. Though a rainbow can seem like a random, unpredictable phenomenon, the natural laws governing rainbow are actually quite specific and predictable, and understanding these laws can help photographers anticipate a rainbow and enhance its capture.
Energy generated by the sun bathes Earth in continuous electromagnetic radiation, its wavelengths ranging from extremely short to extremely long (and every wavelength in between). Among the broad spectrum of electromagnetic solar energy we receive are ultra-violet rays that burn our skin, infrared waves that warm our atmosphere, and a very narrow range of wavelengths the human eye sees.
These visible wavelengths are captured by our eyes and interpreted by our brain. When our eyes take in light comprised of the full range of visible wavelengths, we perceive it as white (colorless) light. Color registers when some wavelengths are more prevalent than others. For example, when light strikes an opaque (solid) object such as a tree or rock, some of its wavelengths are absorbed; the wavelengths not absorbed are scattered (reflected). Our eyes capture this scattered light, send the information to our brains, which interprets it as a color. When light strikes water, some is absorbed, some passes through to reveal the submerged world, and some light is reflected by the surface as a reflection.
To understand the interaction of water and light that creates a rainbow, it’s simplest to visualize what happens when sunlight strikes a single drop. Light entering a water drop refracts (bends), with different wavelengths refracting different amounts, which separates the originally homogeneous white light into the myriad colors of the spectrum.
But simply separating the light into its component colors isn’t enough to create a rainbow—if it were, we’d see a rainbow whenever light strikes water. Seeing the rainbow spectrum caused by refracted light requires that the refracted light be returned to our eyes somehow.
A raindrop isn’t flat like a sheet of paper, it’s spherical, like a ball. Light that was refracted (and separated into multiple colors) as it entered the front of the raindrop, continues through to the back of the raindrop, where some is reflected. Red light reflects back at about 42 degrees, violet light reflects back at about 40 degrees, and the other spectral colors reflect back between 42 and 40 degrees. What we perceive as a rainbow is this reflection of the refracted light—notice how the top color of the primary rainbow is always red, the longest visible wavelength; the bottom color is always violet, the shortest visible wavelength.
Every raindrop struck by sunlight creates a rainbow. But just as the reflection of a mountain peak on the surface of a lake is visible only when viewed from the angle the reflection bounces off the lake’s surface, a rainbow is visible only when you’re aligned with the 40-42 degree angle at which the raindrop reflects the spectrum of rainbow colors.
Fortunately, viewing a rainbow requires no knowledge of advanced geometry. To locate or anticipate a rainbow, picture an imaginary straight line originating at the sun, entering the back of your head, exiting between your eyes, and continuing down into the landscape in front of you—this line points to the “anti-solar point,” an imaginary point exactly opposite the sun. With no interference, a rainbow would form a complete circle, skewed 42 degrees from the line connecting the sun and the anti-solar point—with you at the center. (We don’t see the entire circle because the horizon usually gets in the way.)
Because the anti-solar point is always at the center of the rainbow’s arc, a rainbow will always appear exactly opposite the sun (the sun will always be at your back). It helps to remember that your shadow always points toward the anti-solar point. So when you find yourself in direct sunlight and rain, locating a rainbow is as simple as following your shadow and looking skyward—if there’s no rainbow, the sun’s probably too high.
Sometimes a rainbow appears as a majestic half-circle, arcing high above the distant terrain; other times it’s merely a small circle segment hugging the horizon. As with the direction of the rainbow, there’s nothing mysterious about its varying height. Remember, every rainbow would form a full circle if the horizon didn’t get in the way, so the amount of the rainbow’s circle you see (and therefore its height) depends on where the rainbow’s arc intersects the horizon.
While the center of the rainbow is always in the direction of the anti-solar point, the height of the rainbow is determined by the height of the anti-solar point, which will always be exactly the same number of degrees below the horizon as the sun is above the horizon. It helps to imagine the line connecting the sun and the anti-solar point as a fulcrum, with you as the pivot—picture yourself in the center of a teeter-totter: as one seat rises above you, the other drops below you. That means the lower the sun, the more of its circle you see and the higher it appears above the horizon; conversely, the higher the sun, the less of its circle is above the horizon and the flatter (and lower) the rainbow will appear.
Assuming a flat, unobstructed scene (such as the ocean), when the sun is on the horizon, so is the anti-solar point (in the opposite direction), and half of the rainbow’s 360 degree circumference will be visible. But as the sun rises, the anti-solar point drops—when the sun is more than 42 degrees above the horizon, the anti-solar point is more than 42 degrees below the horizon, and the only way you’ll see a rainbow is from a perspective above the surrounding landscape (such as on a mountaintop or on a canyon rim).
Of course landscapes are rarely flat. Viewing a scene from above, such as from atop Mauna Kea or from the rim of the Grand Canyon, can reveal more than half of the rainbow’s circle. From an airplane, with the sun directly overhead, all of the rainbow’s circle can be seen, with the plane’s shadow in the middle.
Not all of the light careening about a raindrop goes into forming the primary rainbow. Some of the light slips out the back of the raindrop to illuminate the sky, and some is reflected inside the raindrop a second time. The refracted light that reflects a second time before exiting creates a secondary, fainter rainbow skewed 50 degrees from the anti-solar point. Since this is a reflection, the colors of the secondary rainbow are reversed from the primary rainbow.
And if the sky between the primary and secondary rainbows appears darker than the surrounding sky, you’ve found “Alexander’s band.” It’s caused by all the light machinations I just described—instead of all the sunlight simply passing through the raindrops to illuminate the sky, some of the light was intercepted, refracted, and reflected by the raindrops to form our two rainbows, leaving less light for the sky between the rainbows.
Understanding the optics of a rainbow has practical applications for photographers. Not only does it help you anticipate a rainbow before it happens, it also enables you to find rainbows in waterfalls.
Unlike a rainbow caused by rain, which requires you to be in exactly the right position to capture the incongruous convergence of rainfall and sunshine, a waterfall rainbow can be predicted with clock-like precision—just add sunshine.
Yosemite is my location of choice, but there’s probably a waterfall or two near you that will deliver. Just figure out when the waterfall gets direct sunlight early or late in the day, then put yourself somewhere on the line connecting the sun and the waterfall. And if you have an elevated vantage point, you’ll find that the sun doesn’t even need to be that low in the sky.
Understanding rainbow optics can even help you locate rainbows that aren’t even visible to the naked eye. A “moonbow” (lunar rainbow) is a rarely witnessed and wonderful phenomenon that follows all the natural rules of a daylight rainbow. But instead of resulting from direct sunlight, a moonbow is caused by sunlight reflected by the moon.
Moonlight isn’t bright enough to fully engage the cones in your eyes that reveal color, though in bright moonlight you can see the moonbow as an arcing monochrome band. But a camera on a sturdy tripod can use its virtually unlimited shutter duration to accumulate enough light to bring out a moonbow in full living color. Armed with this knowledge, all you need to do is put yourself in the right location at the right time.
Following a nice sunrise at the always beautiful Point Imperial, the Grand Canyon Monsoon photo workshop group spent two hours near Bright Angel Point photographing a spectacular electrical storm that delivered multiple lightning captures to everyone in the group. When the storm moved too close and drove us to safety (we’re resilient and adventuresome, not stupid), it would have been easy call it a day and tally our bounty. I mean, who likes getting rained on? Photographers, that’s who.
Don Smith and I herded our group into the cars and headed to Cape Royal Road, where we could follow the Grand Canyon’s East Rim above Marble Canyon all the way to Cape Royal. Knowing that monsoon showers are fairly localized, the plan was to drive out of the cell that was dumping on us at the lodge and either shoot back at it, or (more likely) find another cell firing out over the canyon. In the back of my mind though was the hope for a rainbow above the canyon—dropping in the west, the sun was perfectly positioned for rainbows in the east.
The rainbow appeared just after we passed the Point Imperial Road junction, arcing high above the forest. Climbing through the trees toward the rim (and its views of Marble Canyon), my urgency intensified with the rainbow’s vivid color, but we were stuck behind a meandering tourist who clearly had different priorities. As tempted as I was to pass him, I knew that would be a mistake with three more cars following me. So we poked along at a glacial pace. After what felt like hours, screeched to a halt at the Vista Encantada parking area with the rainbow hanging in there—I swear everyone was out of the car and scrambling for their gear before I came to a complete stop.
With a full rainbow above an expansive view, I opted for my Sony 12-24 lens on my a7RII, but immediately began to question that choice. While Vista Encantada offers a very pretty view, it’s not my favorite scene to photograph because of the less-than-photogenic shrubbery in the foreground—a telephoto lens definitely would have worked better to eliminate the foreground, but I wanted more rainbow. So after a few failed attempts to find a composition at the conventional vista, I sprinted into the woods to find something better. This turned out to be a wise choice, as the shrubs here were replaced with (much more photogenic) mature evergreens.
In a perfect world I’d have found an unobstructed view into the Grand Canyon, but as photographers know, the world is rarely perfect. Committed to my wide lens, I decided to use the nearby evergreens as my foreground, moving back just far enough for the rainbow to clear their crowns. Composing wide enough to include the trees top-to-bottom also allowed me to include all of the rainbow—suddenly my 12-24 lens choice was genius!
After finishing at Vista Encantada we continued down the road and photographed another rainbow from Roosevelt Point, then wrapped up the day with a sunset for the ages at Cape Royal. A great day indeed, all thanks to monsoon weather that would have kept most tourists indoors.
Click an image for a closer look and to view slide show.
Posted on April 7, 2019
Every year for the last 10 (or so) years I’ve traveled to the Grand Canyon during the Southwest summer monsoon to photograph lightning. Not only have I captured hundreds of lightning strikes and lived to tell about it (yay), I’ve learned a lot. A couple of years ago I added an article sharing my insights on photographing lightning to my photo tips section. With lightning season upon (or almost upon) us here in the United States, I’ve updated my article with new images and additional info. You can still find the article (with updates) in my Photo Tips section, but I’m re-posting it here in my regular blog feed as well.
Read the story of this image at the bottom of this post, just above the gallery of lightning images.
Let’s start with the given that lightning is dangerous, and if “safety first” is a criterion for intelligence, photographers are stupid. So combining photographers and lightning is a recipe for disaster.
Okay, seriously, because lightning is both dangerous and unpredictable, before attempting anything that requires you to be outside during an electrical storm, it behooves you to do your homework. And the more you understand lightning, how to avoid it and stay safe in its presence, the greater your odds of living to take more pictures. Not only will understanding lightning improve your safety, a healthy respect for lightning’s fickle power will also help you anticipate and photograph lightning.
Lightning is an electrostatic discharge that equalizes the negative/positive polarization between two objects. In fact, when you get shocked touching a doorknob, you’ve been struck by lightning. The cause of polarization during electrical storms isn’t completely understood, but it’s generally accepted that the extreme vertical convective air motion (convection is up/down circular flow caused when less-dense warm air rises, becomes more dense as it cools with elevation, and ultimately becomes cool/dense enough to fall. Convection is also what causes bubbling in boiling water. Convection in a thunderstorm carries positively charged molecules upward and negatively charged molecules downward. Because opposite charges attract each other, the extreme polarization (positive charge at the top of the cloud, negative charge near the ground) is quickly (and violently) equalized: lightning.
With lightning comes thunder, the sound of air expanding explosively when heated by a 50,000 degree jolt of electricy. The visual component of the lightning bolt that caused the thunder travels to you at the speed of light, over 186,000 miles per second (virtually instantaneous regardless of your distance on Earth). But lightning’s aural component, thunder, only travels at the speed of sound, a little more than 750 miles per hour—a million times slower than light. Knowing that the thunder occurred at the same time as the lightning flash, and how fast both travel, we can compute the approximate distance of the lightning strike. At 750 miles per hour, thunder will travel about a mile in about five seconds: Dividing the time between the lightning’s flash and the thunder’s crash by five gives you the lightning’s distance in miles; divide the interval by three for the distance in kilometers. If five seconds pass between the lightning and the thunder, the lightning struck about one mile away; fifteen seconds elapsed means it’s about three miles away.
The 30 (or so) people killed by lightning in the United States each year had one thing in common with the rest of us: they didn’t believe they’d be struck by lightning when they started whatever it was they were doing when they were struck. The only sure way to be safe in an electrical storm is to be in a fully enclosed structure or metal-framed vehicle, away from open windows, plumbing, wiring, and electronics.
While there’s no completely safe way to photograph lightning, it doesn’t hurt to improve your odds of surviving to enjoy the fruits of your labor. (Unfortunately, photographing lightning usually requires being outside.) Most lightning strikes within a six mile radius of the previous strike. So, if less than thirty seconds elapses between the flash and bang, you’re too close. And since “most” doesn’t mean “all,” it’s even better to allow a little margin for error. Thunder isn’t usually audible beyond ten miles—if you can hear the thunder, it’s safe to assume that you’re in lightning range.
But if you absolutely, positively must be outside with the lightning crashing about you, or you simply find yourself caught outside with no available shelter, there are few things you can do to reduce the chance you’ll be struck:
Photographing lightning at night is mostly a matter of pointing your camera in the right direction with a multi-second shutter speed and hoping the lightning fires while your shutter’s open—pretty straightforward. Photographing daylight lightning is a little more problematic. It’s usually over before you can react, so without a lightning sensor to recognize lightning and click your shutter, success is largely dumb luck (few people are quick enough see it and click). And using a neutral density filter to stretch the exposure time out to 20 or 30 seconds sounds great in theory, but a lightning bolt with a life measured in milliseconds, captured in an exposure measured in multiple seconds, will almost certainly lack the contrast necessary to be be even slightly visible.
Lightning Trigger: The best tool for the job
Most lightning sensors (all?) attach to your camera’s hot shoe and connect via a special cable to the camera’s remote-release port. When engaged, the sensor fires the shutter (virtually) immediately upon detecting lightning, whether or not the lightning is visible to the eye or camera. With many lightning sensors from which to choose, before I bought my first one I did lots of research. I ended up choosing the sensor that was the consensus choice among photographers I know and trust: Lightning Trigger from Stepping Stone Products in Dolores, CO. At around $350 (including the cable), the Lightning Trigger is not the cheapest option, but after many leading lightning-oriented photo workshops, I can say with lots of confidence that lightning sensors are not generic products, and the internal technology matters a lot. Base on my own results and observations, the Lightning Trigger is the only one I’d use and recommend (I get no kickback for this). On the other hand, if you already have a lightning sensor you’re happy with, there’s no reason to switch.
I won’t get into lots of specifics about how to set up the Lightning Trigger because it’s simple and covered fairly well in the included documentation. But you should know that of the things that sets the Lightning Trigger apart from many others is its ability to put your camera in the “shutter half pressed” mode, which greatly reduces shutter lag (see below). But that also means that connecting the Trigger will probably disable your LCD replay, so you won’t be able to review your captures without disconnecting—a simple but sometimes inconvenient task. You also probably won’t be able to adjust your exposure with the Lightning Trigger connected.
The Lightning Trigger documentation promises at least a 20 mile range, and after many years using mine at the Grand Canyon, I’ve seen nothing that causes me to question that. It also says you can expect the sensor to fire at lightning that’s not necessarily in front of you, or lightning you can’t see at all, which I will definitely confirm. For every click with lightning in my camera’s field of view, I get many clicks caused by lightning I didn’t see, or that were outside my camera’s field of view. But when visible lightning does fire somewhere in my composition, I estimate that the Lightning Trigger clicked the shutter at least 95 percent of the time (that is, even though I got lots of false positives, the Lightning Trigger missed very few bolts it should have detected). Of these successful clicks, I actually captured lightning in at least 2/3 of the frames.
The misses are a function of the timing between lightning and camera—sometimes the lightning is just too fast for the camera’s shutter lag. In general, the more violent the storm, the greater the likelihood of bolts of longer duration, and multiple strokes that are easier to capture. And my success rate has increased significantly beyond 2/3 since switching from a Canon 5DIII to Sony mirrorless (more on this in the Shutter Lag section).
The Lightning Trigger documentation recommends shutter speeds between 1/4 and 1/20 second—shutter speeds faster than 1/20 second risk completing the exposure before all of the secondary strokes fire; slower shutter speeds tend to wash out the lightning. To achieve daylight shutter speeds between 1/4 and 1/20 second, I use a polarizer, with my camera at ISO 50 and aperture at f/16 (and sometimes smaller). Of course exposure values will vary with the amount of light available, and you may not need such extreme settings when shooting into an extremely dark sky. The two stops of light lost to a polarizer helps a lot, and 4- or 6-stop neutral density filter is even better with fairly bright skies (but if you’re using a neutral density filter, try to avoid shutter speeds longer than 1/4 second).
Lightning is fast, really, really fast, so the faster your camera’s shutter responds after getting the command from the trigger device, the more success you’ll have. The delay between the click instruction (whether from your finger pressing the shutter button, a remote release, or a lightning sensor) and the shutter firing is called “shutter lag.”
The less shutter lag you have, the better your results will be. The two most important shutter lag factors are:
In addition to a lightning sensor and fast camera, you’ll need:
Getting the shot
Lightning is most likely to strike in or near the gray curtains (clearly recognizable as distant rain) that hang beneath dark clouds. In addition to visible rain curtains, the darkest and tallest clouds are usually the most likely to fire lightning. Here are a few more points to consider:
Do as I say (not as I do)
Be aware that electrical storms can move quite quickly, so you need to monitor them closely. Sometimes this simply means adjusting your composition to account for shifting lightning; other times it means retreating to the car if the cell threatens your location. No shot is worth your life.
About this image
On the first evening of last year’s second Grand Canyon Monsoon photo workshop, Don Smith and I took the group to Point Imperial for a sunset shoot. Based on the forecast we had little hope for lightning, but one thing I’ve learned over the many years of photographing the monsoon here is that the forecast isn’t the final word. We got another reminder of this that evening.
The view from Point Imperial is both expansive and different from other Grand Canyon vistas, stretching east across the Painted Desert and north to the Vermillion Cliffs. As the group made their way down to the vista platform, in the corner of my I thought I a lighting strike far to the north. A second bolt confirmed my discovery and soon we had the entire group lined up with cameras pointed and triggers ready.
With everyone in business, I set up my tripod and attached my Lightning Trigger to my Sony a7RIII. Since this lightning was close to 30 miles away, maybe farther than any lightning I’ve tried to photograph, so I hauled out my Sony 100-400 GM lens and zoomed in as tight as I could. I didn’t have to wait long to confirm that my Lightning Trigger would catch strikes this distant—it didn’t hurt that these were massive bolts, many with multiple pulses and forks.
Everyone was thrilled, so thrilled that it didn’t immediately register that the storm was moving our direction. I started at 400mm, but by the time I captured this frame I was just a little more than 100mm. That’s still a pretty safe distance, but with night almost on us and another cell moving in from the east, we decided to take our winnings and go home.
One final note: If you check my exposure settings, you’ll see that my shutter speed here was .4 seconds, well outside the 1/20-1/4 second range I suggest. But if you look at the other settings, you’ll see that I’d opened up to f/7.1, and had cranked my ISO to 400, an indication that twilight was settling in. Successful lightning photograph is all about contrast, and the darker the sky, the better the bolt stands out, even in a longer exposure. Had we stayed past dark (and lived), we could have jettisoned the Lighting Triggers and used multi-second exposures.
Join Don Smith and me in our next Grand Canyon Monsoon Photo Workshop
Read my article in Outdoor Photographer magazine, Shooting the Monsoon
Click an image for a closer look and slide show. Refresh the window to reorder the display.
Posted on December 30, 2018
I’ve always struggled with the “top-whatever” end-of-year countdown of my favorite images because the choices are so subjective and mood dependent, and so many images are favorites as much for their memories as they are for their aesthetic value. And coming up with a predetermined number is arbitrary, and inevitably requires choices I don’t want to make and will almost certainly regret later. One year I may have only seven or eight images that thrill me; the next year I might have two dozen. This year I chose 27, and I still have some left to process.
So rather than attempt to rate and rank my images at year’s end, I prefer using them as a catalyst for reflection. Each December I go through everything I’ve processed from the waning year (this year I know of several that would certainly qualify as a highlight but they’re as yet unprocessed) think about the circumstances of their capture.
I remember the New Year’s Eve solo drive to Yosemite to photograph the full moon rising behind, followed by a night drive to the other side of the Sierra (a six hour drive in winter) where I hoped to capture the full moon setting behind Mt. Whitney. The Yosemite part of that trip was spectacular, the Mt. Whitney half was a photography flop, but I enjoyed the entire journey.
I remember nearly a month in New Zealand, photographing the South Island’s unmatched beauty in its most beautiful season (hint: brrrrrrr). In New Zealand I hiked on a glacier, photographed the (far superior) Southern Hemisphere version of Milky Way, was chased through a fjord by leaping dolphins, witnessed one of the most vivid crimson sunrises I’ve ever seen, and logged hundreds of quality kilometers with a group of wonderful people.
I remember a solo drive to Yosemite to photograph fresh snow, never a sure thing regardless of the forecast. I approached Yosemite on the evening prior, I felt like a lone spawning salmon fighting up current against the continuous stream of headlights evacuating Yosemite in advance of the storm. I settled into my room in dark and dry Yosemite Valley, and woke to so much snow that I couldn’t find my car. I’m convinced there is nothing, nothing on Earth more beautiful than Yosemite Valley with fresh snow, and with the park mostly vacant and the noise-damping quality of powdery snow, for a few hours I felt like I had heaven all to myself.
I remember chasing lightning on the Grand Canyon’s North Rim, the thrill (and relief) when everyone in both workshop groups captured lightning, and an especially spectacular lightning storm that started in the telephoto distances and chased us to the cars. This year’s Grand Canyon workshops were altered by fires burning in and near the park and I feared that they’d spoil the photography—instead, in addition to all the lightning, we ended up with spectacular red-rubber-ball sunrises and sunsets that allowed genuinely unique images in this heavily photographed destination.
I remember arriving on the Big Island shortly after Kilauea had shut down after 35 years of continuous eruption, and discovering that between the just-concluded Kilauea eruption and the recently depart remnants of Hurricane Lane, I’d lost nearly half of my locations. Instead I ended up finding alternate photo spots that I like even better than the ones I lost. The high point (literally and figuratively) of that trip turned out to be a chilly, first-ever sunset and Milky Way shoot from atop 13,800 foot Mauna Kea.
I remember my Yosemite Fall Color workshop group finding Yosemite Valley at peak fall color, and three beautiful moonrises in my just concluded winter moon workshop. And while thousand of photographers jockeyed for position beneath bone dry Horsetail Fall in February, my workshop group set up elsewhere and photographed one of the most beautiful sunsets of the year.
I remember way back in January, along with my Death Valley workshop group, photographing my first-ever lunar eclipse (on the heals of my first-ever solar eclipse in August of 2017).
And I remember trudging through Grand Canyon sand by starlight to a spot that I’d decided before nightfall was probably not a good Milky Way candidate, and discovering that I was wrong. It turned out the level of the Colorado River level had changed in the night, replacing mushy sand with a swirling pool that rendered the Milky Way’s reflection as a luminous abstract.
I could go on and on about my memories of 2018, but all these great memories also remind me of the unknown highlights in store for 2019. Certainly the planned trips, which include my first-ever Iceland visit (with Don Smith in preparation for our 2020 workshop), my first-ever Oregon Coast workshop (with Don Smith), another raft trip through the Grand Canyon, a return visit to New Zealand, and on and on. But what excites me more than anything is the inevitable surprises, those special moments that dazzle when dazzling is the last thing you expect. Bring it on!
(Click an image for a bigger view, and to see a slide show)
Posted on August 18, 2018
Lightning (at a safe distance) is pretty cool. It has always fascinated me, partly for the ephemeral power that can explode a tree and disappear before my brain can register its existence, but also because lightning is a rare sight for these California eyes. What what exactly is going on in a lightning bolt? I thought you’d never ask….
The shocking truth about lightning
Lightning is an electrostatic discharge that equalizes negative/positive polarization between two objects. For example, when you get shocked touching the doorknob in your bedroom, you’ve been struck by your own personal lightning bolt. You got zapped because, courtesy of that carpet you just dragged your fuzzy slippers across, you picked up a few extra electrons that the doorknob was more than happy to relieve you of.
While the polarization process that happens in an electrical storm isn’t as thoroughly understood as the one in your bedroom, it’s generally accepted that a thunderstorm’s vertical, convective air motion shuffles electrons in the atmosphere. To jar your high school science memories, convection occurs when a fluid substance heats, becomes less dense, and rises until it cools and becomes dense enough to sink. (You initiate convection when you boil water.)
The is up/down circular flow of atmospheric convection happens when air near the ground warms, expands, and rises. The rising air carries water vapor; since cooler air can’t hold as much moisture as warm air, the ascending water vapor eventually condenses into clouds. The convective motion jostling the water and ice molecules inside the clouds strips the molecules of electrons. Electrons are negatively charged and more dense than the surrounding air; freed of their conventional bonds, these electrons fall earthward. Overhead, the clouds relieved of many electrons are suddenly positively charged, while the ground below has been rendered negatively charged by virtue of its new electron surplus.
Because nature abhors any imbalance, these opposite charges attract each other. The extreme polarization in a thunderstorm—positive charge at the top of the cloud, negative charge near the ground—is quickly (and violently) equalized: lightning! So I guess you could say that lightning is God’s way of telling Earth, “Stop being so negative!”
With lightning comes other atmospheric changes. The sudden infusion of a 50,000 degree electric charge displaces the surrounding air very suddenly, creating an audible compression wave that we know as thunder.
The visual component of the lightning bolt that caused the thunder travels to you at the speed of light, over 186,000 miles per second. But lightning’s aural component, thunder, only travels at the speed of sound, a mere 750 miles per hour (or so)—a million times slower than light.
Because lightning and its thunder are simultaneous, and we know how fast each travels, we can compute the lightning’s approximate distance. (Thunder’s speed varies slightly with atmospheric conditions; light’s speed is non-negotiable.) From our human perspective the lightning arrives instantaneously, but moving at 750 miles per hour, thunder takes around five seconds to travel a mile. So, dividing by five the number of seconds to elapse between the lightning’s flash and its thunder’s crash gives you the lightning’s distance in miles (divide the interval by three for the approximate distance in kilometers). For example, if ten seconds pass between the lightning and the thunder, the lightning struck about two miles away, fifteen seconds elapsed means it’s about three miles away, and so on.
This speed difference also explains why lightning comes and goes in milliseconds, while its thunder can rumble and roll for several seconds. Because a lightning bolt can travel many miles, the thunder from its nearest portions reaches you much sooner than its most distant components.
About this image
Each summer moisture from the Gulf of Mexico makes its way up into the American Southwest. The combination of moist air and extreme heat (to kick off convection) makes August ripe for thunderstorms at the Grand Canyon. For the last six years, Don Smith and I have scheduled two photo workshops hoping to photograph these thunderstorms and their effects (clouds, rainbows, and especially lightning).
Bit with unseasonably dry air in place, the forecast at the start of this year’s first Grand Canyon Monsoon workshop wasn’t especially favorable for lightning. I told the group during the orientation that I wasn’t concerned, that I’ve often seen forecasts like this change suddenly—then anxiously monitored every subsequent NWS forecast update with crossed fingers. In the meantime, we were all quite content photographing incredible smoke effects, courtesy of three nearby wildfires.
By the end of our second day I started seeing hints of moisture returning to the forecast toward the end of the workshop, with each forecast looking a little more promising than the one prior. By day four, the workshop’s final full day, I was downright optimistic.
We’ve always had better lightning success on the North Rim. Partly because the view faces south, the direction from which the storms tend to arrive, and partly because our cabins at Grand Canyon Lodge are right on the rim. Grand Canyon Lodge also has a pair of view decks, shielded by lightning rods, that are ideal for photographing lightning.
The lightning started firing early on our final evening. We all rushed to the rim, attached our Lightning Triggers, and pointed toward the most promising clouds. Much to my relief, it wasn’t long before everyone in the group had at least one lightning image, and most had many more than just one.
But feeling a bit greedy, with nice clouds overhead, and the smoke that had set up camp in the canyon for most of the week suddenly scoured by heavy rain, I realized that all we needed to ignite a sunset lightshow was a little sunlight. I glanced westward and saw signs of clearing. Dare I hope for a sunset to go with this lightning? As if by divine intervention, the sun emerged from the clouds just a few minutes before sunset, infusing the canyon and its diaphanous rain bands with light that started amber and reddened with each passing minute.
When the choice is between a (relatively) bland scene most likely to get lightning, and better a composition with just a slight chance for lighting, I usually take my chances and opt for the better composition. In this case the lightning had shifted a little north of the canyon, but I pointed my camera toward the better light over the canyon and crossed my fingers. So irresistible was the light that while waiting (and not wanting to change my composition and miss a lightning strike), I pulled my a7RII from my bag and clicked a couple of handheld frames due south, where no lightning was possible but the light was especially sweet. (Anyone who knows me will be shocked to hear that I took a picture without a tripod.)
Though several bolts fired during the five or so minutes before the sun disappeared, the one in this image was the only lightning I captured with the great sunset light. But all I wanted was one sunset strike, and I felt extremely lucky that it arrived just as the magenta glow reached its crescendo.
The lightning waxed and waned for several more hours. With the sun down the sky soon darkened enough for me to remove my Lightning Trigger and switch to long exposures in Bulb mode. I stayed until after 10:00, wrapping up with a couple of 20+ minute exposures that captured more than a dozen strikes each.
Posted on June 3, 2018
It was 4:00 a.m. and I’d spent the last two hours photographing the Milky Way’s brilliant core above the Colorado River. In about 75 minutes the guides would be ringing the “coffee’s ready” gong, signaling the start of another day at the bottom of the Grand Canyon. Collapsing my tripod, I performed a little mental math and found slight relief in the knowledge that I might be able to squeeze in one more hour of sleep. That relief vanished in the time it took to turn and glance toward the northern sky and see the Big Dipper, suspended like a celestial mobile in the notch separating the canyon walls.
My Milky Way position had been chosen for its unobstructed view of the southern sky; the best view of the Big Dipper was clear across the campsite, at a sheltered pool just beyond our rafts. The moonless night sky at the bottom of the Grand Canyon is so dark that the Milky Way casts a slight shadow, but once your eyes adjust, it’s surprisingly easy to navigate without adding light. Trudging across through the sand, I passed a handful of other solitary photographers, anonymous shapes enjoying the darkness as much as I was. I stopped few times to answer questions and point out the Big Dipper, then moved on.
Setting up on the steep, sandy slope above the river, I gazed at the Big Dipper and privately chuckled at my good fortune—this prime photo opportunity hadn’t manifest because I proactively made myself seek a scene away from my original subject (as I encourage my students to do), it was a chance glance after I’d mentally put myself to bed. When we landed at that spot the prior afternoon, I’d been so focused on the southern exposure and the Milky Way opportunity in that direction that I hadn’t even considered that there might be something facing north too. Shame on me, but sometimes it’s better to be lucky than good.
Checking my first Big Dipper frame, a couple of things became instantly obvious: though sunrise was still an hour away, and my eyes could detect no sign of its approach, with the same exposure I’d been using for most of the night, the sky was noticeably brighter on my LCD; more significantly, the Big Dipper was reflecting in the river. I realized that pool below me, while not flowing, was sloshing enough that the reflection didn’t stand out to my eyes, but it was smoothed enough by a multi-second exposure that the water mirrored a blurred but clearly visible reflection of the bright Dipper stars.
From my elevated vantage point, part of the handle’s reflection was lost to the sandy beach—I needed to move closer to the river to include the entire reflection. Remember when I said it’s surprisingly easy to navigate in the moonless darkness? On my first step toward the river I learned that functional night vision applies to avoiding objects, not to depth perception. So, as that first step dropped earthward and I waited for it to touch down, where I expected sand I found only air. The rest of me followed quickly and I was in free-fall. Fortunately the fall was not far, just a couple of feet, but it’s amazing how the disorientation of a blind fall slowed time enough for me to curse the darkness before my graceless splat onto the damp beach.
The beach was damp because the place I landed had been river when I went to bed. I popped up almost as quickly as I landed, the unwitting beneficiary of artificial tides induced by upstream releases from the Glen Canyon Dam, timed to meet the power needs of Las Vegas and the rest of the Southwest sprawl. Had I fallen a few hours earlier, I’d have splashed in chilly river water—not enough river to sweep me to my death, but definitely enough to soak me and my camera. So I found myself sandy but otherwise unscathed—glancing about to see if anyone had seen my fall, I instantly forgave the darkness that had made me more or less invisible. The Rokinon lens I’d had on my camera was caked with sand; since it was too dark to clean it, I switched to my Sony 16-35 f/2.8 GM.
The rest of the shoot was fairly uneventful, at least until my final frame. Over the next few minutes I inched even closer to the river, which I discovered had receded enough to add about six feet of soggy shore. With each frame I verified my focus, tweaked my composition, and experimented with different exposures.
On my final few frames I was comfortable enough with all of the photography variables that I wasn’t even thinking about the next shot, and instead simply stood and took in the night sky. As I waited for my last frame of the night to complete, a brilliant meteor sprung from the darkness and split the Dipper’s handle. It came and went in a heartbeat, and I held my breath until the image popped up on my LCD and I confirmed that I’d captured it. The perfect cap to a spectacular night.
Posted on May 27, 2018
Nothing in my life delivers a more potent dose of perspective than viewing the world from the bottom of the Grand Canyon. Days are spent at the mercy of the Colorado River, alternately drifting and hurtling beneath mile-high rock layers that tell more than a billion years of Earth story. And when the sun goes down, the ceiling becomes a cosmological light show, each pinpoint representing a different instant in our galaxy’s past.
More than any of my five trips through the Grand Canyon, I’ll remember this year’s for its night skies. The wall-to-wall blue that dogged our daylight photography darkened to just what the night-photography doctor ordered, and we took full advantage. Excited about the potential for stars, each day I powwowed with our lead guide, the amazing Lindsay, to identify potential campsites with the best views of the night sky in general, and the best views of our Milky Way’s brilliant galactic core in particular.
But targeting a Milky Way campsite is easier in theory than execution. In the Northern Hemisphere, even when the galactic core reaches its highest point, it’s still fairly low in the southern sky. So given the Grand Canyon’s general east/west orientation, the best Milky Way views are usually blocked by the canyon’s towering walls. Even identifying a potential campsite on a north/south oriented stretch of the river doesn’t ensure success because Colorado River campsites in the Grand Canyon are first-come, first-served. So even though the other groups on the river don’t usually think strategically about photographing the night sky like I do, each campsite has its own appealing qualities and there’s never a guarantee that any given one will be free when we get there.
In general, my raft trips’ first night or (maybe) two usually provide our best Milky Way opportunities because the first 75 miles of the Colorado River downstream from our put-in at Lee’s Ferry runs pretty much north/south. With the river running north/south, the canyon walls are to the east and west and we usually get a pretty clear view of the north and south horizons. Just downstream from the confluence of the Colorado and Little Colorado Rivers, the canyon bends more or less permanently east/west and Milky Way core views are few and far between.
This year, our day-one campsite got us a decent but not quite perfect view of the southern sky. Nevertheless, many rafters rose and gave it a try, with varying degrees of success—at the very least, it was good practice, and much was learned. On day two we had a magnificently open sky, but the southern horizon was behind us as we faced the river, so the Milky Way’s center rose above lots of shrubs and rocks. That night I and a few others photographed the view across the river toward the Big Dipper, North Star, and fainter part of the Milky Way in Cassiopeia, but a handful had some success photographing the brighter Milky Way from a hill facing south.
I knew days four and five would be long shots for Milky Way photography because Lindsay and I had in mind an east/west trending day-4 site directly across the river from Deer Creek Fall (fingers crossed), one of the trip’s photographic highlights. And there were no good candidates for day 5 (we ended up camping beneath Toroweap). But Lindsay had an ace up her sleeve for day 3, our first day on the east/west portion of the river, if we could pull it off.
In addition to being the day we bend west, day three is the much anticipated “rapid day.” After warming up with a couple of days of fairly infrequent mild to medium rapids, the action on day three ramps up considerably, both in rapid frequency and intensity. Rapid day is always so much fun, for most of the rafters the thoughts of night photography take backseat thrills and laughter.
While everyone else’s attention was on the river, in the back of my mind I was crossing my virtual fingers for the prosaically named Camp 118 (for the number of miles downstream from our starting point at Lee’s Ferry). Camp 118 had been on my radar since Lindsay had told me about it on our first day, citing a bend in the river that gives the spot a view of the southern sky that’s very rare on this part of the river. But she warned me that Camp 118 has other benefits that make it popular among all the trips on the river, and gave us a no better than 50 percent chance of scoring it.
Equal parts exhausted and exhilarated, late in the afternoon of day three we rounded a bend and found Camp 118 free and clear. Phew. As soon as we landed I did a quick check with my compass app and confirmed that the river here pointed due south. Camp 118 also had a long south-facing sandy beach that would give everyone ample room to setup and move around in the dark without getting in anyone else’s way. Once the boat was off-loaded I gathered the troops and told them to prepare for some the best Milky Way photography of the trip.
One more Grand Canyon Milky Way obstacle I forgot to mention is that even in the most favorable locations, the galactic core doesn’t rotate into the slot between the canyon walls until 2:00 a.m. or later. Often rafters go to bed with every intention of rising to photograph it, but when the time comes, their resolve has burrowed deep into the cozy folds of their sleeping bag. The best antidote is to be as prepared as possible before going to bed. At the very least, I prescribe the following: identify your composition, set up your camera, lens, and tripod, set your exposure, focus at infinity, and have your camera ready atop the tripod beside your cot. Better still, if it can be done without risk of someone stumbling over it in the dark, leave the camera composed and focused at your predetermined shooting spot.
I woke at 2:00 a.m. and found many already at work on the Milky Way, which was just making its way into view above the canyon wall in the east. During the next two-and-a-quarter hours I worked the scene while the galactic core slid from left to right, first above the river and finally down toward the wall on the west side of the river. I used both my Sony a7SII and a7RIII bodies, and my Rokinon 24mm f/1.4, Sony 12-24 f/4 G, and Sony 16-35 f/2.8 GM lenses.
Since getting my 42 megapixel a7RIII, I’ve been happy enough with its night photography results that I’d almost forgotten about my 12 megapixel a7SII. In fact, I seriously considered leaving my a7SII at home for this trip. I’m so glad I didn’t. Using the two side-by-side like this, offered an instant reminder why the a7SII is the night photography king. Combined with the light gathering ability of an f/1.4 lens, with my a7SII I can look through my viewfinder and focus perfectly in about three seconds. I can also get crazy-bright images in crazy-dark conditions like this.
I usually feel like the “star” of night images is the sky; because vertical orientation gives me the most sky and least foreground, most of my night images are oriented vertically, especially when the more or less vertically oriented Milky Way is present. But one of my goals for this trip was more horizontal Milky Way images, so I made a point of setting aside my vertical bias and shooting a lot of horizontal frames. This image (like all of my images) is a single click (no composite of multiple frames) with no artificial light added (no light painting or any other light besides stars and skylight). I saw several meteors that night, but have no specific memories of the small one darting across the upper middle of this frame.
I wrapped up with this scene a little before 4:00 a.m., but heading back to bed I saw the Big Dipper cradled between the two canyon walls, just above the north horizon, too beautiful to resist. I ended up photographing another 20 minutes or so on the other side of camp, ending up with one of my favorite images of the trip, including a meteor I very much remember. But that’s a story for another day….
A few tips for photographing the Milky Way
I have an entire article that spells out Milky Way photography, but here’s the CliffsNotes (is that still a thing?) version:
Click an image for a closer look and slide show. Refresh the window to reorder the display.