Posted on March 3, 2019
As aggressively as I seek creative ways to express nature with my camera, and as important as I think that is, sometimes a scene is so beautiful that it’s best to just get out of the way and let the scene speak for itself. I had one of those experiences last month at Tunnel View in Yosemite.
There’s a reason Tunnel View is one of the most photographed vistas in the world: El Capitan, Half Dome, Cathedral Rocks, Bridalveil Fall—each would be a landscape icon by itself; put them all together in one view and, well…. But the view this evening was truly transcendent, even by Yosemite standards. In Yosemite Valley below, trees and granite still glazed with the snowy vestiges of a departing storm seemed to throb with their own luminance. And above Half Dome a full moon rose through a sky that had been cleansed of all impurities by the departing storm, an otherworldly canvas of indigo, violet, and magenta.
On these crystal-clear, winter-twilight moonrises, the beauty rises with the moon, reaching a crescendo about 20 minutes after sunset, after which the color quickly fades and the landscape darkens. Unfortunately, a some point before the crescendo, the dynamic range becomes so extreme that no camera (not even the dynamic range monster Sony a7RIII) can simultaneously extract usable detail from a daylight-bright moon and dark landscape.
I’d driven to Yosemite solely to photograph this moonrise, an eight hour roundtrip for 40-minutes of photography. Starting with the moon’s arrival about 20 minutes before sunset, I’d juggled three camera bodies and two tripods, first shooting ultra long, then gradually widening to include more of the snowy landscape. Already my captures had more than justified the time and miles the trip would cost me, but watching the moon traverse the deepening hues of Earth’s shadow, I wasn’t ready to stop.
I’ve learned that with a scene this spectacular, conveying the majesty doesn’t require me to pursue the ideal foreground, or do creative things with motion, light, or depth of field. In fact, I’ve come to realize that sometimes a scene can be so beautiful that creative interpretations can dilute or distract from the very beauty that moves me. On this evening in particular, I didn’t want to inject myself into that breathtaking moment, I just wanted to share it.
To simply my images, I opted for a series of frames that used tried-and-true compositions that I’d accumulated after years (decades) of photographing here, the compositions I suggest as “starters” for people who are new to Yosemite, or use myself to jump-start my inspiration: relatively tight horizontal and vertical frames of El Capitan, Half Dome, Bridalveil Fall; El Capitan and Half Dome; or Half Dome and Bridalveil Fall. In the image I share above I concentrated on Half Dome and Bridalveil Fall, capping my frame with the wispy fringes of a large cloud that hovered above Yosemite Valley.
Simplifying my compositions had the added benefit of freeing all of my (limited) brain cells to concentrate on the very difficult exposure. The margin for error when photographing a moon this far after sunset is minuscule—if you don’t get the exposure just right, there’s no fixing it in Photoshop later: too dark and there’s too much noise in the shadows; too bright and lunar detail is permanently erased. The problem starts with the understandable inclination to expose the scene to make the landscape look good on the LCD, pretty much guaranteeing that the moon will be toast. Compounding this problem is the histogram, which most of us have justifiably come to trust as the final arbiter for all exposures. But when a twilight moon (bright moon, dark sky) is involved, even the histogram will fail you because the moon is such a small part of the scene, it barely (if at all) registers on the histogram.
Rather than the histogram, for these dark sky moon images I monitor my LCD’s highlight alert (“blinking highlights”), which is usually the only way to to tell that the moon has been overexposed. If the moon is flashing, I know I’ve given the scene too much light and need to back off until the flashing stops—no matter how dark the foreground looks. This is where it’s essential to know your camera, and how far you can push its exposure beyond where the histogram and highlight alert warn you that you’ve gone too far.
When I’m photographing a full moon rising into a darkening sky, I push the exposure to the point where my highlight alert just starts blinking (only the brightest parts of the moon, not the entire disk, are flashing), then I give it just a little more exposure. I know my Sony a7RIII well enough to know that I can still give it a full stop of light beyond this initial flash point and still recover the highlights later. The shadows? In a scene like this they’ll look nearly black, a reality my histogram will confirm, but I never cease to be amazed by how much detail I can pull out of my a7RIII’s shadows in Lightroom and Photoshop.
I continued shooting for several minutes after this frame, and discovered later that even my final capture contained usable highlights and shadows. I chose this image, captured nearly five minutes before I quit, because it contained the best combination of color, lunar detail, and clean (relatively noise-free) Yosemite Valley.
Posted on February 24, 2019
Roll over, Ansel
Several years ago, while thumbing through an old issue of “Outdoor Photographer” magazine, I came across an article on Lightroom processing. It started with the words:
“Being able to affect one part of the image compared to another, such as balancing the brightness of a photograph so the scene looks more like the way we saw it rather than being restricted by the artificial limitations of the camera and film is the major reason why photographers like Ansel Adams and LIFE photographer W. Eugene Smith spent so much time in the darkroom.”
While it’s true that Ansel Adams and W. Eugene Smith were indeed darkroom masters, statements like this only perpetuate the myth that the photographer’s job is to reproduce the scene “the way we saw it.” And because I imagine that using Ansel Adams himself to peddle this notion must send Ansel rolling in his grave, I’ll start by quoting the Master himself:
Do these sound like the thoughts of someone lamenting the camera’s “artificial limitations” and photography’s inability to duplicate the world the “way we saw it”? Take a look at just a few of Ansel Adams’ images and ask yourself how many duplicate the world as we see it: nearly black skies, exaggerated shadows and/or highlights, and skewed perspectives that intentionally emphasize one subject over another, and on and on. And no color! (Not to mention the fact that every image is a two-dimensional rendering of a three-dimensional world.) Ansel Adams wasn’t trying to replicate scenes more like he saw them, he was trying to use his camera’s unique (not “artificial”) vision to show us aspects of the world he wanted us to see, qualities we might otherwise miss or fail to appreciate.
The rest of the OP article contained solid, practical information for anyone wanting to come closer to replicating Ansel Adams’ traditional darkroom techniques in the contemporary digital darkroom. But the assertion that photographers are obligated to photograph the world as they saw it baffles me.
You’ve heard me say this before
The camera’s vision isn’t artificial, it’s different. Dynamic range, focus, motion, and depth are all rendered differently in a camera than they are to the human eye. And while the human experience of any scene is 360 degrees, a still images is constrained by a rectangular box. Forcing images to be more human-like doesn’t just deny the camera’s unique ability to expand viewers’ perception of the world, it’s literally impossible. Which is why I’ve always felt that the best photographers are the ones who embrace their camera’s vision rather than trying to “fix” it.
For example, limiting dynamic range allows us to emphasize color and shapes that get lost in the clutter of human vision; a narrow range of focus can guide the eye and draw attention to particular elements of interest and away from distractions; and the ability to accumulate light over a photographer-controlled interval exposes color and detail hidden by darkness, and conveys motion in an otherwise static medium.
But what about that rectangular box that constrains the world of a still image? I can think of no better way to excise distractions and laser-focus viewers’ attention on the target subject than taking advantage of the camera’s finite world. While many nature photographers default to their wide angle lenses to expand the visual box surrounding their landscape images and save their long lenses for wildlife, a telephoto lens is an essential landscape tool. The world can be a busy place—in even the most spectacular of vistas, so much is happening visually that going wide in a still photo to include as much beauty as possible introduces many extraneous features, and risks shrinking the scene’s most compelling elements to virtual insignificance.
The best way to overcome wide angle scene dilution is to forego the conventional view (the first thing everyone sees), identify the aspects of the scene that make it special, and isolate them with a telephoto lens. Whether it’s a striking mountain or tree, backlit poppy, or rising moon, isolation enlarges the target subject and removes any ambiguity about what the image is about. And an intimate, up-close perspective of a subject more commonly seen from a distance can be truly mesmerizing.
About this image
I stood atop two feet of packed snow at Tunnel View, more than eight miles from Half Dome, and ten miles from the ridge that would be ground zero for the moonrise that had drawn me in the first place. Along with two other photographers who also seemed aware of the moon’s plans, I had the best (least obstructed) Tunnel View vantage point to myself. Rising full moon or not, before me the table was set for a spectacular Yosemite feast: Brand new snow glazed every exposed surface, and in the pristine winter air, Tunnel View’s veritable who’s who of Yosemite landmarks—El Capitan, Cloud’s Rest, Half Dome, Sentinel Rock, Sentinel Dome, Cathedral Rocks, and Bridalveil Fall—seemed etched into the scene. Above, dark clouds boiled atop El Capitan, while wispy fog radiated from the valley floor.
Occasionally a tourist would wander up and request help identifying Horsetail’s microscopic filament on El Capitan’s vast granite; one or two even pointed at Bridalveil Fall and asked if that was Horsetail Fall. A couple of people, blissfully oblivious to the Horsetail Fall phenomenon, simply wanted their picture taken with this iconic Yosemite backdrop.
About 150 feet down the wall to my right, at least two-dozen photographers on tripods were inexplicably crammed into a significantly less desirable view. While that vantage point gave them an acceptable sightline to Horsetail Fall (as did my own), the rest of the magnificent Tunnel View vista was partially obscured by trees. The only explanation I could muster for their odd choice was that the first to arrive for some reason set up there, and each subsequent photographer assumed that since others have set up here, this must be the spot.
While Horsetail Fall was irrelevant to my objective this evening, the overnight snow still clinging to the trees was undeniable bonus. Getting to Tunnel View had been an adventure, worse even than I’d expected, and I was glad that I’d allowed ample time. The difficulty started with a 30-minute (Horsetail Fall gawker infused) queue at the Arch Rock entrance station. My suspicion that these were mostly inexperienced photographers and tourists (who’d just read an article or seen a news segment and decided to check it out) was confirmed when I was forced to navigate a slalom course of slipping, sliding, spinning cars that had ignored the very clearly communicated chain controls. The serious photographers, those who had photographed Horsetail Fall before, or who had the sense to research the phenomenon well in advance, had been in position for the five-minute show for hours.
With the moon’s imminent arrival upon a scene that already bordered on visual overload, my plan to ensure that the main purpose of my visit didn’t get swallowed by Tunnel View’s conventional post-storm majesty was to start, while the moon was still right on the horizon, with extremely tight compositions. As the moon rose, I planned to widen my focal length, gradually including more scene and turning the moon into more of an accent.
To achieve this, I was flanked by two tripods, and had three camera bodies fired up and ready for action: my Sony a7RIII, a7RII, and a6300. Atop my Really Right Stuff TVC-24L tripod was my a6300 loaded with my Sony 100-400 GM and Sony 2X teleconverter. This combination gave me a 600-1200mm full-frame equivalent focal range (because the a6300 is a 1.5-crop APS-C sensor). When including the rising moon required reducing my focal length below 800mm, I’d switch to my higher resolution, full frame Sony a7RII. And because the moon would rise just about 20 minutes before sunset, I also had to be aware of the possibility that Horsetail Fall would fire up. To handle that possibility, and to cover all my general wide composition needs, mounted on my RRS TQC-14 tripod was my Sony a7RIII and Sony 24-105 f/4 lens.
I pointed my a6300/100-400 at the point where I expected the moon to appear about 20 minutes before sunset, zoomed all the way out to 800mm (1200mm full-frame equivalent), metered, focused, and waited. I started clicking almost immediately after seeing the moon’s leading edge nudge through the trees, refining my composition slightly after each click until I had the right balance of moon and Half Dome. It always surprises me how quickly the moon moves, speed that’s magnified tremendously at such an extreme focal length. Spending the next 40 minutes frantically changing focal lengths, switching lenses and camera bodies, re-metering and re-focusing, and bouncing between tripods, I felt like the percussionist in a jazz band.
When the moon climbed far above Yosemite Valley and the dynamic range between the daylight-bright moon and nighttime landscape made photography impossible, I paused before packing up my gear and just marveled at the beauty. Horsetail Fall had caught a few late rays of sunlight but never did completely light up. I thought about the disappointment of frigid photographers who had waited patiently in the valley below for a show that didn’t happen, and counted my blessings.
Click an image for a closer look and slide show. Refresh the window to reorder the display.
Posted on December 23, 2018
With a wide variety of spectacular and diverse east-facing views, I can think of no better place to photograph a moonrise than Yosemite. I especially like the December full moon because it aligns so well with Half Dome, not just on the night it’s full, but on the nights leading up to the full moon.
When I realized that this year’s December full moon was so close to Christmas, I almost didn’t schedule my annual Yosemite Winter Moon workshop, but then I figured that since I’ll be there anyway, I may as well. I’m so glad I did—the workshop filled, and the skies were clear enough (never a sure thing in December) that we photographed the moon on three of the workshop’s four nights, culminating in a very special moonrise to wrap up the workshop (a topic for a future blog post).
The closer it is to full, the closer to sunset the moon rises, arriving several hours before sunset a few days before it’s full, then a little later each evening before rising right around sunset on the full moon day. Since a waxing (increasing in fullness) moon is always higher at sunset than it will be the next day, with a little planning, it’s possible to time several consecutive days’ shoots to coincide with the moon rising right around sunset. For this year’s workshop I’d planned three sunset moonrises for my group, each (more or less) aligning the moon and Half Dome, getting farther from Half Dome each day.
About this image
While the first of my planned moonrise shoots was Wednesday, when the moon rose above the flat horizon about two hours before sunset, the horizon in Yosemite is anything but flat. I took my group to a favorite location beside the Merced River on Yosemite Valley’s east side, less than three miles from Half Dome, where the relatively steep view angle to the top of Half Dome means that it takes the moon a couple of hours to climb into view here.
Though not labeled on the map, this spot isn’t a secret to photographers, so I arrived about 45 minutes early, partly to allow everyone time to prepare, but also to ensure that we wouldn’t need to battle anyone else for position. I told everyone that the moon would appear at around 4:30 from directly above the top of Half Dome, and suggested that they be ready with their compositions beforehand.
My own composition had been planned long in advance—having photographed more than my share of moonrises from this wide angle location, I decided on an extreme telephoto approach this time. I added my Sony 2X teleconverter to my Sony 100-400 GM lens, mounted the pair on my tripod, and attached my (full frame) Sony a7RIII. I pointed my 800mm of focal length at Half Dome’s summit and waited. <Continues below>
I never tire of seeing the glow of the moon’s leading edge peak above the horizon, and this evening was no exception. When the moon nudged into view, the sounds of chatter and laughter were instantly replaced by clicking shutters. Watching the moon grow in my viewfinder, I adjusted my composition slightly before each click. When the moon gained separation from the granite to become fully visible, I panned slowly to the right and saw that with the right framing it would appear nestled into a subtle bowl-shaped curve atop Half Dome and locked in a composition that would last for a few minutes as the moon continued its ascent. A thin wisp of cloud scooted through the scene as I clicked this frame, lit by the day’s final rays.
One more thing
Looking at the distant world at 800mm reveals previous invisible detail. So once I’d settled on a composition that I could stick with for a few clicks, I allowed my eye wander the frame and noticed dangling icicles lining Half Dome’s rim. I continue to be blown away by the sharpness of the Sony 100-400; not only is this lens unbelievably sharp, I literally cannot tell a difference when I pair it with the Sony 2X teleconverter.
Posted on December 16, 2018
Nothing draws the eye quite like a large moon, bright and bold, with a striking foreground. But something happens when you try to photograph the moon—somehow a moon that looks to the eye like you could reach out and pluck it from the sky, shrinks to a small white speck in a photo.
While a delicate accent of moon is great when properly framed above a nice landscape, most people like their moons BIG. The trick isn’t photographing a large moon, it’s photographing a large moon with a nice landscape.
Bigger is better
Crescent or full, the moon will be as big as the focal length you choose—photograph it at 16mm and the moon registers as a tiny dot; photograph it at 600mm and your moon dominates the frame.
But a landscape image with a large moon requires more than just a long focal length. If big was all that mattered, you could attach your camera to a telescope, point skyward, and get a huge moon. But without a landscape to go with your huge moon, no one would know whether you took the picture standing on a beach in Hawaii, atop a glacier in New Zealand, or beside the garbage cans in your driveway.
“Big moon” is a subjective label, but I usually won’t use it unless I can photograph the moon at 200mm or longer. And while a 200mm lens is okay, the moon doesn’t really start to jump out of the frame for me until I approach 400mm.
My go-to big moon lens is my Sony 100-400 GM because it provides good magnification along with focal length wiggle-room for pulling back when I need to fit a foreground subject that’s a little too close. A telephoto zoom also provides focal length flexibility that allows you to balance your composition, or add variety with a series of different compositions. Of course you can always switch lenses mid-shoot, but you don’t fully appreciate how fast the moon is moving in the sky until you try to align it with a terrestrial subject in a telephoto composition.
When I want a moon even bigger than 400mm gives me, I add a 2X teleconverter and voilà, I’m at 800mm. Bigger still? Out comes my 1.5-crop body and I’m zoomed all the way to a 1200mm equivalent.
Often the most difficult part of including a large moon with a specific landscape subject is finding a vantage point far enough back to fit the subject and the moon. But the farther back from your foreground subject you can position yourself, the longer the focal length you can use, and the bigger the moon will be.
For example, I love photographing a big moon rising behind Half Dome in Yosemite. But at Yosemite’s popular east-side locations, even 200mm is too close to get the moon and all of Half Dome in my frame. And while Yosemite’s most distant east-facing Half Dome vistas are up to 10 miles away, Half Dome is large so that even at that distance the longest focal length that will include the moon and all of Half Dome isn’t much more than 400mm.
A little easier for me is including a big moon with smaller foreground objects like a prominent tree. Near my home in Northern California are rolling hills topped by solitary oaks that make perfect moon foregrounds when I can shoot up so they’re against the sky. And since these trees are much smaller than Half Dome, even vantage points that are less than a mile away lets me zoom all the way up to 1200mm.
Depth of field
With subjects so far away, it’s easy to forget about depth of field. But extreme focal lengths mean extremely limited depth of field. Depth of field isn’t a concern when Half Dome is your closest subject and it’s ten miles distant, but when your foreground is an oak tree on a hill that’s a mile away, you absolutely need to consider the hyperfocal distance.
For example, at 800mm and f/11 (with a full frame sensor), the hyperfocal distance is about a mile-and-a-quarter (look it up)—focus on the tree and the moon will be soft; focus on the moon and the tree is soft. But if you can focus on something that’s a little beyond the tree, at maybe one-and-a-half miles away, the image will be sharp from front to back.
When I’m not sure of my subject distance, I estimate as best I can, focus on a point beyond my foreground subject, then review my image magnified to check sharpness. If my focus point is in my frame, great, but I won’t hesitate to remove my camera from the tripod to focus on something behind me that’s the right distance (if you do this, to prevent refocusing, be sure you use back-button focus or are in manual focus mode when you click your shutter). It’s always best to get the focus sorted out before the moon arrives, a good reason to arrive at a new location well in advance of the moon’s arrival.
Location, location, location
As your focal length increases, your compositional margin for error shrinks. You can’t expect to go out on the evening of a full or crescent moon, look to the horizon, and automatically put the moon in the frame with your planned foreground subject.
Even when the moon and your foreground do align, once the moon appears, you’ll only have a few minutes before it rises out of your telephoto frame. This means extreme telephoto images that include both the moon and a foreground subject are only possible when the moon is right on the horizon, making proper timing essential.
Like the sun, the moon traces a different path across the sky each day. This path changes with each lunar cycle (from full, to new, back to full); whether the moon is full or crescent, a location that perfectly aligns the moon and foreground one month will probably be nowhere close the next.
Coordinating all the moving parts (moon phase and position, foreground subject alignment, subject distance, and rise/set timing) requires some planning and plotting. When I started photographing the moon, in the days before smart phones and apps that do the heavy lifting, I had to refer to tables to get the moon’s phase and position in the sky, manually plot the alignment, then apply the Pythagorean theorem to figure the timing of the moon’s arrival above (or disappearance behind) the terrain.
Today there are countless apps that will do this for you. Apps like The Photographer’s Ephemeris and Photo Pills (to name just two of many) are fantastic tools that give photographers access to moonrise/set data for any location on Earth. There is a bit of a learning curve (so don’t wait until the last minute to plan your shoot), but they’re infinitely easier than the old fashioned way.
When the moon is a small accent to a wide scene, it’s often enough to just show up on its full or crescent day and shoot it somewhere above your subject. But because the margin of error is so small, planning for a big moon image is best done months in advance.
I identify big-moon candidate locations near home and on the road, and am always on the lookout for more. My criteria are a prominent subject that stands out against the sky, with a distant east or west facing vantage point. Over the years I’ve assembled a mental database ranging from hilltop trees near home, to landscape icons like Half Dome, Mt. Whitney, and Zabriskie Point (Death Valley).
With my subjects identified, I do my plotting (I still do it the old fashioned way) and mark my calendar for the day I want to be there. That often means waiting close to a year for the alignment I want. And if the weather or schedule doesn’t cooperate, my wait can be longer than that.
About this image
<Some may recognize this from the horizontal version of this moonrise I’ve shared for years; I just processed this vertical version.>
A few years ago I scheduled a spring Yosemite workshop to coincide with a 3% crescent moon that I’d computed would slip into the narrow gap between El Capitan and Half Dome about 45 minutes before sunrise on our final morning. Though we were all at the same place, photographing the same thing, the true magic was simply being there to witness a special moment that probably won’t repeat for decades.
The afternoon before this moonrise, I brought the group to this spot on Big Oak Flat Road so they could familiarize themselves with the location and plan their compositions. During this preview someone asked exactly where the moon would rise, and I confidently blurted that it will appear in the small notch separating El Capitan and Half Dome, between 5:15 and 5:20 a.m. I’d never actually photographed a moonrise from this spot, and as I spoke to the group I became painfully aware of how small the opening is—even the slightest error in my plotting could find the moon blocked by El Capitan or Half Dome.
Sunday morning we departed dark and early (4:45 a.m.), full of anticipation. We arrived at Half Dome View a little after 5:00, early enough to enable everyone to set up their tripods, frame their compositions, and prepare their exposure settings. Then we waited, all eyes locked on the notch.
And then there it was, the slightest point of moonlight edging into that small gap between Yosemite’s iconic monoliths. Phew. The rest of the morning was a blur of shutter clicks and exclamations of delight.
Before the shared euphoria abated, I suggested to everyone that they take a short break from photography and simply appreciate that they’re probably witnessing the most beautiful thing happening on Earth at this moment (a feeling every nature photographer should experience from time to time). It’s always exciting to witness a moment like this, a breathtaking convergence of Earth and sky that may not occur again exactly like this in my lifetime. It’s even more rewarding when the event isn’t an accident, that I’m experiencing it because of my own effort, and that I get to share the fruit of my perspiration with others who appreciate the magic just as much as I do.
Posted on November 25, 2018
I love the iconic captures as much as the next person—scenes like Yosemite’s Horsetail Fall in February, Upper Antelope Canyon’s famous light shaft, or McWay Fall’s tumble into the Pacific, are both gorgeous and a thrill to photograph. But standing elbow-to-elbow with hundreds (or thousands!) of photographers, each recording virtually identical images that are already duplicates of thousands of prior images, while nice, doesn’t necessarily stimulate my creative juices.
Once upon a time photographing even the most popular scenes in solitude wasn’t difficult. The tourists who overwhelm the best known views during the comfortable times of day would vacate just when the photography started getting good. But with the proliferation of digital photographers and easy exchange of information in our connected world, there aren’t many photography secrets anymore, and the opportunities to make unique images have become more challenging than ever. And if you do capture something special, posting it online is sure to immediately draw photographers like cats to a can opener.
Given that Yosemite Valley’s eight square miles attracts over five million visitors each year, you’d think it would be impossible to find unique perspectives. But on even the busiest summer day, rising for sunrise will give you at least a couple of peaceful hours. And of course in Yosemite’s backcountry, while relatively crowded by wilderness standards, solitude is always just a short detour away.
But the iconic spots earned their recognition for a reason, and first-time (or infrequent) Yosemite visitors want to see them too. For my workshops, in addition to sharing with my students a variety of my favorite more hidden Yosemite spots, I’ve learned to take them to the Yosemite locations they’ve come to know from a lifetime time of viewing Yosemite pictures.
The first visits to vistas like Glacier Point, Tunnel View, Valley View, and Sentinel Bridge still inspire the awe they always have. It’s easy for photographers, overcome by the majesty before them, to fall back on their memory of others’ images and settle for their own version of the same thing. Rather than suggest that my students avoid doing this (for many, these images are the very reason they signed up in the first place), I suggest that they start with the iconic shots they know, but don’t make it their goal. Rather, I encourage them to use those familiar imagers as a starting point for a fresh take that’s more uniquely theirs. I won’t pretend that this approach always, or even frequently, results in something that no one has ever captured, but I think everyone’s photography benefits when that is the goal—not just the images captured today, but the ability to see and execute better images tomorrow as well.
In this year’s Yosemite Fall Color and Reflections workshop we spent most of our time bouncing from one beautiful scene to the next. Autumn, with its colorful leaves and ubiquitous reflections, provides more opportunities for unique captures than any other season, and the color this years was fantastic. But that didn’t prevent us from checking off the icons.
Speaking of icons, my rule of thumb in Yosemite is El Capitan in the morning and Half Dome in the afternoon. But after breakfast one morning, one of the cars said they wanted to go check out Sentinel Bridge, one of the best Half Dome reflections in the park. Normally I resist photographing Half Dome in the morning because its face doesn’t get direct sunlight until late afternoon, but on the way to breakfast I’d noticed the cottonwoods upstream were beautifully backlit and I thought it might be worth checking out. So I scrapped my original plans and we detoured back to the bridge (hey, never let it be said that I’m not flexible).
I’m so glad I listened to the votes from the other car that morning because we ended up with one of the workshop’s highlight shoots. Half Dome was in full shade, sky was a bland blue mixed with a few thin clouds, but the backlit trees were off the charts. We all started with the wider, more conventional views, capturing Half Dome and the trees doubled by their reflection. But that doesn’t take long, and soon I was encouraging everyone to keep working it.
When working out a composition, I always try to figure out where the scene’s action is. In this scene the highlight for me was the upstream trees and their reflection. Wanting as little as possible of the fairly boring sky, I went with a horizontal composition. I also thought a horizontal composition would be best for framing the cottonwoods and reflection with the shaded trees on both sides of the river. To leave no ambiguity about what this image is about, I removed the actual Half Dome entirely, leaving its reflection for context only.
With my Sony 24-105 f/4 G on my Sony a7RIII, I zoomed to a composition that put the “action” front and center, making sure to get all of Half Dome’s reflection but minimal sky, balancing the backlit trees and their reflection toward the top of the from, and framing everything with the darker trees on the edges. Depth of field and motion weren’t concern, so I went with my default ISO 100 and f/11, focused, and clicked.
As anyone who has been in one of my workshops knows, the first click is a draft, an image to review and refine. Evaluating the picture on my LCD, I ran my eyes around my frame and made a few micro adjustments to ensure a tight composition without cutting off the tops of the sunlit tree in the top center, the shaded trunks on the left and right, and the cloud above (below?) Half Dome.
Judging from the variety of images shared in the image reviews, this shoot was a highlight for everyone else too. Some found their own takes on this upstream scene, while a few ventured across the road to capture a completely different scene looking downstream. Not a bad result for a location that wasn’t even on my radar for that morning.
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Posted on November 18, 2018
Yosemite, like most of the Sierra Nevada, was carved from an intrusive igneous rock (subterranean magma that cooled without reaching the surface). This subterranean magma cooled slowly enough for its primary constituents, quartz and feldspar, plus mica and other minerals, to form crystals that fuse into an extremely hard matrix: granite. The granite waited patiently in the dark while overhead oceans advanced and receded, leaving thousands of feet of new sediment behind.
Beginning tens of millions of years ago, a slow-motion collision of tectonic plates uplifted the granite and its overlying sedimentary layers. As the ancient mountain range rose, erosion accelerated the demise of the sedimentary layers, eventually exposing the much harder granite. As the uplift continued, rivers moved faster, carving V-shaped river valleys that included the predecessor of what we now know as Yosemite Valley.
Then came the glaciers, an irresistible force meeting granite’s immovable object. Instead of breaking apart and collapsing as a lesser rock might, Yosemite’s granite stood tall as the glaciers cleared out the ancient Yosemite Valley, carving it into the U-shaped feature we know today—a flat floor bounded by vertical cliffs.
Granite’s hardness also affects the way it breaks up when exposed to the elements of weathering. Instead of crumbling under wind and rain like softer rock, or cleaving along aligned planes of weakness, granite retains its shape until fracturing along microscopic cracks caused by external stress such as pressure or weathering. These cracks allow water to seep into the rock. Of course you remember from high school science (right?) that unlike most substances, water expands when it freezes. This expansion pushes open the cracks, allowing even more water to seep in after the ice melts. This crack/seep/freeze/expand cycle continues until the rock fails, splitting along the expanded crack. In this process large chunks of granite are shed, often quite suddenly, while the remaining granite stands tall.
Granite’s unique qualities are on exquisite display in Yosemite Valley, where streams bursting with snowmelt tumble over shear granite walls, and granite monoliths tower 3,000 feet above the Merced River. Yosemite and Bridalveil Falls are Yosemite’s most recognized waterfalls, but look up on a spring day and you might count a dozen or more. The waterfalls dominate in spring, but Yosemite’s monoliths endure year-round, drawing visitors from around the world in every season. El Capitan, the largest chunk of granite in the world, is a climbers’ mecca, and few mountains have a more recognizable profile than Half Dome.
Half Dome is a bit of a misnomer, but one look at it the name is easy to visualize a rounded dome that lost a full half of its mass to a passing glacier. The reality is that Half Dome’s current shape is fairly close to the rock that was exposed by millions of years of erosion. While Yosemite’s glaciers filled most of Yosemite Valley, Half Dome was tall enough to protrude from the ice sheet and avoid direct contact. Half Dome’s shear face resulted from a single fracture that separated a large slice of granite to expose the flat granite face we all recognize.
After a nice day photographing fall color and reflections El Capitan’s shadow, we finished our day at Glacier Point for a face-to-face view Half Dome. The gray stratus blanket that had permitted a full day of sweet photography in diffuse the sunlight was about to become a liability for anyone longing for a colorful sunset.
Half Dome gets light all the way up to, and in fact even a couple of minutes beyond, the “official” (flat horizon) sunset. But because the view of Half Dome faces east, and the view to the west is obscured by terrain, there’s no way to know whether the horizon is clear in the direction of the setting sun. Even on cloudy days like this, my rule in Yosemite is to never give up on sunset until at least five minutes the after the official sunset time has passed. When a couple of people in the group started rumbling about heading back to the cars, I issued one of my favorite Yosemite proclamations to all within earshot: Never try to predict the conditions in five minutes based on the conditions now. I knew the odds were long for capturing anything more than darkening shades of gray fading to black, but without cameras they’d be zero.
I have no idea whether they truly believed me, or simply stayed put to humor me, but either way, I started to look pretty smart about five minutes before sunset when we spotted a faint glow on Half Dome. I held my breath as the sun slipped into a clear slot of unknown size on the horizon behind us to paint Half Dome with warm light. I hadn’t planned to shoot that evening, but as the light intensified I was glad I’d dragged my bag around anyway. As I quickly set up my tripod and extracted my camera, I urged everyone to keep shooting because there was no guarantee that this would last—just as I’ve witnessed many of these last minute miracles in Yosemite, I’ve also seen euphoria dashed in a heartbeat when the sun was suddenly snuffed right at the climactic moment (Horsetail Fall is notorious for this). But this evening the light held strong, warming to a golden crescendo, then fading to pink that intensified to a rich red that colored the sky from horizon to horizon.
The light tones of quartz and feldspar, plus its crystalline nature, make granite especially reflective. So while Yosemite isn’t especially known for its sunsets, when they do get red like this, granite’s inherent reflectivity causes the entire landscape to throb with a crimson glow. It’s one of my favorite phenomena in nature.
I ended up photographing the entire sunset with my Sony 100-400 GM lens on my Sony a7RIII. Not because I didn’t have a wealth of wide angle shots to choose from (I did!), but because I was working with my group and the telephoto compositions were simpler. Simpler in the sense that (for me at least) a wide shot requires a bit more strategic planning to first identify the frame’s foreground, middle-ground, and background elements, then position myself to give them a coherent relationship. A telephoto composition, on the other hand, has always felt more intuitive than strategic (though each generally requires elements of strategy and intuition), so I’m usually able to put my camera and telephoto to my eye, then move and zoom until something feels right.
With so many views at Glacier Point, the group had scattered a little before sunset, so I was only with about half of them for the good stuff at the end. Back at the cars I checked in with those who had gone elsewhere and found that while most had photographed it, a couple had watched the show from the parking lot. Sigh.
Posted on September 2, 2018
My relationship with Yosemite rainbows goes all the way back to my childhood, when a rainbow arcing across the face of Half Dome made my father more excited than I believed possible for an adult. I look back on that experience as the foundation of my interest in photography, my relationship with Yosemite, and my love for rainbows. So, needless to say, photographing a rainbow in Yosemite is a pretty big deal for me.
A few years ago the promise (hope) of lightning drove me to Yosemite to wait in the rain on a warm July afternoon. But after sitting for hours on hard granite, all I got was wet. It became pretty clear that the storm wasn’t producing any lightning, but as the sky behind me started to brighten while the rain continued falling over Yosemite Valley, I realized that conditions were ripe for a rainbow. Sure enough, long after I would have packed up and headed home had I been focused solely on lightning, this rainbow was my reward.
The moral if my story is that despite all appearances to the contrary, rainbows are not random—when sunlight strikes raindrops, a rainbow occurs, every time. The reason we don’t always see the rainbow not because it isn’t happening, it’s because we’re not in the right place. And that place, geometrically speaking, is always the same. Of course sometimes seeing the rainbow requires superhero ability like levitation or teleportation, but when we’re armed with a little knowledge and anticipation, we can put ourselves in position for moments like this.
I can’t help with the anticipation part, but here’s a little knowledge infusion (excerpted from the Rainbow article in my Photo Tips section).
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 and longer infrared waves that warm our atmosphere. These wavelengths bookend a very narrow range of wavelengths the human eye sees.
Visible wavelengths are captured by our eyes and interpreted by our brain. When the our eyes take in light consisting of the full range of visible wavelengths, we perceive it as white (colorless) light. We perceive color 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. 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 and scattered by the surface, enabling us to see the water; some light passes through the water’s surface, enabling us to see what’s in the water; and some light is reflected by the surface, enabling us to see reflections.
(From this point on, for simplicity’s sake, it might help to visualize what happens when water strikes a single drop.)
Light traveling from one medium to another (e.g., from air into water) refracts (bends). Different wavelengths refract different amounts, causing the light to split into its component colors. Light that passes through a water refracts (bends). Different wavelengths are refracted different amounts by water; this separates the originally homogeneous white light into the multiple 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, and the bottom color is always violet.
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 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’s sometimes helpful 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 belowthe 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 in Hawaii 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 order of the colors is the secondary rainbow is reversed.
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.
Click an image for a closer look and slide show. Refresh the window to reorder the display.