Posted on January 19, 2020
Imagine a world that’s so quiet you can hear nature’s every stirring, a place where each breath holds a pristine bouquet of subtle fragrances and the sky is a continuously shifting kaleidoscope of indigo, blue, yellow, orange, and pink. Maybe you’ve already figured out that I’m describing the very world we live in, before the sun’s light and warmth entice the dirty, noisy, oblivious masses.
The morning magic begins long before the human eye can register detail and color, while a few stars still burn overhead and nearby objects loom as vague shapes. Lacking enough light for the eyes to do their thing, the human experience pre-sunrise is biased toward the non-visual senses, as the sounds of a gentle breeze, flowing water, and stirring creatures mingle with the smells of dew and plants.
For the next 30 minutes, the eastern horizon seems to brighten faster than the rest of the scene. Pushed by the approaching sun, the earth’s shadow hovers in the west, swallowing stars with its steely blue. Following the earth’s shadow is the belt of Venus, as the sun’s longest wavelengths battle through the atmosphere to color the sky pink.
Photographing this pre-sunrise show can begin earlier than your eyes might tell you. Experienced photographers understand that what we perceive as darkness is just our eyes’ relatively limited ability to gather light, combined with the brain’s insistence on processing this limited input instantaneously. But a camera’s sensor accumulates all the light that strikes it for whatever duration we prescribe, thereby stretching the “instant” of perception indefinitely and allowing us to use every possible photon.
Another advantage a digital sensor has over the human eye is its ability to extract color from this apparent darkness. The human eye uses rods and cones to collect light, with the rods doing the heavy lifting in low light, pulling enough monochrome information to discern shapes, but providing little help with color and depth. The cones that complete the scene with color and depth information don’t kick in until there’s much more light. But a digital sensor, though blind to depth, captures photons without discrimination, allowing it to “see” color in very low light.
The ability to capture aspects of the natural world that differ from the human perspective might just be my favorite thing about photography, and these sunrise moments provide a great opportunity to engage the camera’s strength. When the scene is in the same direction as the rising sun, I look for shapes to isolate against the sky, then underexpose enough to turn the shapes into silhouettes, and to prevent the color from being washed out by the sun’s brilliance. When the sun is rising at my back, I take the opposite approach, giving the scene extra light to extract invisible detail from the virtually shadowless light and reveal hidden color in the sky and landscape.
About this image
On the penultimate day of each Death Valley Winter Moon workshop, my group makes the scenic, 90 minute drive from Death Valley to Lone Pine for the workshop’s final sunset and sunrise. The view in the Alabama Hills faces west, so at sunset we’re photographing shaded mountains beneath the brightest part of the sky—not ideal conditions for photography. If we’re lucky enough to get clouds, these Alabama Hills sunsets can still be special, but really it’s the sunrise that we’re here for. At sunrise in the Alabama Hills, we face the Sierra as the sun rises at our back, first coloring the sky with the blue hues of Earth’s shadow, followed by the magenta and pinks of twilight wedge.
Another special aspect of an Alabama Hills sunrise is the Sierra Crest. Towering 10,000 feet above the surrounding terrain, Mt. Whitney and its neighbors jut into the twilight wedge, and for a few sweet seconds take on its pink pastels that photographers call alpenglow.
This year’s sunset was nothing spectacular, but we walked out to the famous Mobius Arch, checked out a couple of other less noteworthy arches nearby, and I pointed out some of the area’s many movie-shoot spots. I was also able to show everyone where the morning sun would rise, and where the moon would set, and introduce them to the most prominent peaks on display: Lone Pine Peak on the left, Mt. Whitney in the middle, and Mt. Williamson on the right.
The forecast for the next morning was clear skies—maybe not dramatic, but good for the planned moonset and ideal for alpenglow on the crest. My general rule for any location is to arrive at least 30 minutes before the “official” (flat horizon) sunrise time, but in the Alabama Hills in winter, I like to get out there even earlier because the warm light from the eastern horizon light reflects off the snow and granite makes the peaks appear to glow in the dark.
The next morning, loading up in the dark at the hotel I glance toward Mt. Whitney and saw a bank of clouds fringing the crest. At first I was concerned that these clouds would obliterate Mt. Whitney, but arriving at our spot in the Alabama Hills, I realized the peak was indeed out, its tip just barely poking into the clouds. We’d arrived about 45 minutes before sunrise, but I barked (gently) at everyone not to delay, that despite what their eyes told them, this light (that still required headlamps to navigate) makes for great photography. Most beelined to the arch, but I saw a telephoto opportunity and quickly set up right next to the car.
White with snow, Mt. Whitney stood in dramatic contrast to the dark sky and foreground. Using the thin strip of clouds to frame the crest, I started by including some of the sky above the clouds, but quickly tightened my composition to simplify the composition. My 30-second exposure to brightened the image far beyond what my eyes saw, and smoothed all detail from the shifting clouds.
The eastern horizon was already gold from the approaching sun, and while I couldn’t really tell that by looking at Whitney, it was apparent with my very first frame. The sun was more than a half-hour from rising, so the light you see on the clouds and Whitney is reflected from the horizon glow, while the darker terrain below Whitney was too low for a direct view of the horizon light.
Click an image for a closer look and to view a slide show.
Posted on February 9, 2018
My previous post was about dynamic juxtaposition in landscape photography—combining static landscape subjects with transient meteorological and celestial elements. The other side of the juxtaposition coin I call static juxtaposition: combining stationary landscape objects. I am a little reluctant to use the word “static” because there is one element that absolutely can’t be static in these compositions: You.
Since I don’t photograph people or wildlife, I often joke that I don’t photograph anything that moves. And because of this, I need to create motion by encouraging my viewers’ eyes to move through my frame, either providing a path for their eyes to follow and/or a place for them to land. Accomplishing this with static subjects isn’t necessarily difficult, but it does require some physical effort.
Most photographers don’t have a problem getting themselves to the general locations that align foreground and background subjects, but many get a little lazy once they’re there, planting their tripods clinging to the spot like a ship an anchor.
Once I’ve arrived at a location and identified my primary subject, I challenge myself to find at least one other element on a different plane. Sometimes that’s easy, other times…, not so much. Nevertheless, when my subject is in the distance, I look for something closer that has visual weight; likewise, if my subject is nearby, I want something with visual weight in my background. Visual weight is something that pulls the eye: a flower, tree, shrub, leaf, reflection, rock—I could go on, but you get the point. Sometimes it’s not even a distinct entity, but rather a pattern, texture, color, or splash of light.
My secondary subject can have strong aesthetic value or not—sometimes it’s there simply to balance the frame, while other times it has almost as much visual appeal as my primary subject. Regardless of its visual strength, my secondary subject’s placement, both in the frame and relative to the scene’s other visual elements, can make or break an image. And lacking a forklift, pretty much the only way to change the relative position of two static objects in a photographic frame is carefull positioning of the camera (and the photographer behind it!).
As a general rule I avoid merging my essential visual elements—to do conflates those elements and sacrifices the illusion of depth that’s so essential in a two-dimentional image. Another thing I try to avoid is objects with visual weight at the edge of my frame because anything that pulls my viewers’ eyes toward the image’s boundary dilutes its impact.
Viewers’ eyes move most effectively through a scene by following lines. Sometimes those lines are tangible, like a horizontal horizon, vertical waterfall, or diagonal river. But often it’s up to me to create virtual lines—an implicit, connect-the-dots path between visual elements, or textures and shapes that frame my primary subject and constrain my viewers’ eyes. For example:
Last week I was at Mobius Arch beneath Mt. Whitney, the final stop of my annual Death Valley photo workshop. After three days of spectacular Death Valley sunrises and sunsets that seem to be trying to outdo the one before it, I didn’t dare to hope that the string would continue when we moved to the Alabama Hills.
The real show here is sunrise, when day’s first rays of sun color the Sierra Crest with alpenglow’s pink hues, even on clear sky mornings. Sunsets here require a little help. The view here faces west, so at sunset you usually find yourself photographing the shaded side of your subjects against the brightest part of the sky—not really a recipe for success. But a few clouds on the western horizon not only add color and texture, they soften the light. And that’s what happened last week.
Before sunset the thin, translucent cirrus layer was lost in the late afternoon glare, but as the sun dropped below the horizon, the clouds picked up its refracted long wavelengths and colored the sky deepening shades of red. Soon the color was so intense that it shaded weathered granite boulders.
The three elements I wanted to feature in my composition were Mobius Arch, the Sierra Crest (Lone Pine Peak and Mt. Whitney), and the colorful sky. As dramatic as the Sierra Crest is, the star of this scene is the arch. With no real access to a telephoto view, filling my frame with the arch means a wide angle lens that includes too much sky. But the vivid color this evening gave me a rare opportunity to include a sky worthy of the rest of the scene.
My Sony 12-24 f/4 G lens allowed me to within a couple feet of the arch while still fitting it in my frame. With the Sierra Crest framed by the arch, I was careful to position myself so both Lone Pine Peak (on the left) and Mt. Whitney (on the right) were visible. Finally, I needed to decide the camera height. When the sky is less interesting, I raise my camera to fill the arch’s opening with the mountains and minimize the sky. But this evening the colorful sky was an asset, so I dropped as low as I could to maximize it.
At such a wide focal length, depth of field was a piece of cake—I didn’t need to check my hyperfocal app to know that I had lots of margin for error. Focusing toward the back of the arch, I easily achieved the front-to-back sharpness I wanted. Click.
Posted on October 10, 2017
This is an edited and updated version of my Eastern Sierra article that appeared in the September 2016 edition of “Outdoor Photographer” magazine
Skirting the east side of the Sierra Nevada, US 395 enchants travelers with ever-changing views of California’s granite backbone. Unlike anything on the Sierra’s gently sloped west side, Highway 395 parallels the range’s precipitous east flank in the shadow of jagged peaks that soar up to 2 miles above the blacktop. More than just beautiful, these massive mountains form a natural barrier against incursion from the Golden State’s major metropolitan areas, keeping the Eastern Sierra region cleaner and quieter than its scenery might lead you to expect.
It would be difficult to find any place in the world with a more diverse selection of natural beauty than the 120-mile stretch of 395 between Lone Pine and Lee Vining: Mt. Whitney and the Alabama Hills, the ancient bristlecones of the White Mountains (across the Owens Valley, east of the Sierra), the granite columns of Devil’s Postpile, Mono Lake and its tufa towers, and too many lake-dotted, aspen-lined canyons to count. Long a favored escape for hikers, hunters, and fishermen, in recent years photographers have come to appreciate the rugged, solitary beauty possible only on the Sierra’s sunrise side.
I prefer photographing most Eastern Sierra locations at sunrise, when the day’s first rays paint the mountains with warm light, and the highest peaks are colored rose by alpenglow. (Without clouds, Eastern Sierra sunset light can be tricky, as you’ll be photographing the shady side of the mountains against the brightest part of the sky.) Devoid of large metropolitan areas, low light pollution also makes the Eastern Sierra one California’s finest night photography destinations. But regardless of the time of day, the key to photographing the Eastern Sierra is flexibility—if you don’t like the light in one direction, you usually don’t need to travel far to find something nice in another direction.
Lone Pine area
The southern stretch US 395 bisects the Owens Valley, a flat, arid plane separating the Sierra Nevada to the west from the Inyo ranges to the east. Just west of Lone Pine lies the Alabama Hills. Named for a Confederate Civil War warship, the Alabama Hills’ jumble of weathered granite boulders and proliferation of natural arches would be photogenic in any setting. Putting Mt. Whitney (the highest point in the 48 contiguous states), Lone Pine Peak (the subject of Mac OS X Sierra’s desktop image), and the rest of the serrated southern Sierra crest seems almost unfair.
The Alabama Hills are traversed by a network of unpaved but generally quite navigable roads. To get there, drive west on Whitney Portal Road (the only traffic signal in Lone Pine). After 3 miles, turn right onto Movie Road and start exploring. If you’re struck by a vague sense of familiarity here, it’s probably because for nearly a century the Alabama Hills has attracted thousands of movie, TV show, and commercial film crews.
Mobius Arch (also called Whitney Arch and Alabama Hills Arch) is the most popular photo spot in the Alabama Hills. It’s a good place to start, but settling for this frequently photographed subject risks missing numerous opportunities for truly unique images here. To get to Mobius Arch, drive about a mile-and-half on Movie Road to the dirt parking area at the trailhead. Following the marked trail down and back up the nearby ravine, the arch is an easy ¼ mile walk. There’s not a lot of room here, but if the photographers work together it’s possible to arrange four or five photographers on tripods with Mt. Whitney framed by the arch. And don’t make the mistake many make: the prominent peak on the left is Lone Pine Peak; Mt. Whitney is serrated peak at the back of the canyon.
Sunrise is primetime for Alabama Hills photography, but good stuff can be found here long before the sun arrives. I try to be set up 45 minutes before the sun (earlier if I want to ensure the best position for Whitney Arch) to avoid missing a second of the Sierra’s striking transition from night to day.
The grand finale from anywhere in the Alabama Hills is the rose alpenglow that colors the Sierra crest just before sunrise. Soon after the alpenglow appears, the light will turn amber and slowly slide down the peaks until it reaches your location, warming the nearby boulders and casting dramatic, long shadows. But unless there are clouds to soften the light, you’ll find that the harsh morning light will end your shoot pretty quickly once the sunlight arrives on the Alabama Hills.
Whitney Portal Road (closed in winter) ends about 11 miles beyond Movie Road, at Whitney Portal, the trailhead for the hike to Mt. Whitney and the John Muir Trail. On this paved but steep road, anyone not afraid of heights will enjoy great views looking east over the Alabama Hills and Owens Valley far below, and up-close views of Mt. Whitney looming in the west. At the back of the Whitney Portal parking lot is a nice waterfall that tumbles several hundred feet in multiple steps.
The Alabama Hills are one of my favorite moonlight locations. Because the full moon rises in the east right around sunset, on full moon nights the Alabama Hills and Sierra crest are bathed in moonlight as soon as darkness falls. Lit by the moon, the hills’ rounded boulders mingle with long, eerie shadows, and the snow-capped Sierra granite radiates as if lit from within.
If you find yourself with extra time, drive about 30 miles east of Lone Pine on Highway 136 until you ascend to a plain dotted with photogenic Joshua trees—after you’ve finished photographing the Joshua trees, turn around and retrace the drive back to Lone Pine on 136 to enjoy spectacular panoramic views of the Sierra crest. And just north of Lone Pine on 395 is Manzanar National Historic site, a restored WWII Japanese relocation camp. Camera or not, this historic location is definitely worth taking an hour or two to explore.
Bristlecone pine forest
Continuing north from Lone Pine on 395, on your left the Sierra stretch north as far as the eye can see, while the Inyo mountains on the right transition seamlessly to the White Mountains. Though geologically different from the Sierra, the White Mountains’ proximity and Sierra views make it an essential part of the Eastern Sierra experience.
Clinging to rocky slopes in the thin air above 10,000 feet, the bristlecone pines of the White Mountains are among the oldest living things on earth—many show no signs of giving up after 4,000 years; at least one bristlecone is estimated to be 5,000 years old.
Abused by centuries of frigid temperatures, relentless wind, oxygen deprivation, and persistent drought, the bristlecones display every year of their age. Their stunted, twisted, gnarled, polished wood makes the bristlecones suited for intimate macros and mid-range portraits, or as a striking foreground for a distant panorama.
The two primary destinations in the bristlecone pine forest are the Schulman and Patriarch Groves. Get to the bristlecone pine forest by driving east from Big Pine on Highway 168 and climbing about 13 car-sickness inducing miles. Turn left on White Mountain Road and continue climbing another 10 twisting miles to reach the Schulman Grove. Despite the incline and curves, the road is paved all the way to this point. Stop at the Sierra panorama after about 8 miles for a spectacular view that also makes a great excuse to pause and collect yourself.
Stop at the small visitor center in the Schulman Grove to pay the modest use fee, then choose between the 1-mile Discovery loop trail, and the 4 1/2 mile Methuselah loop trail. Both trails are in good shape, but the extreme up and down in very thin air will test your fitness. Most of the trees on the Methuselah Trail get more morning light, while the majority of the Discovery Trail trees get their light in the afternoon.
If you’re unsure of your fitness, or have limited time, the Discovery Trail is definitely the choice for you. Because the photogenic trees start with the very first steps, on this trail you can turn around at any point without feeling cheated of opportunities to photograph nice bristlecones. And along the way you’ll appreciate the handful of benches for enjoying the view and catching your breath. Hikers who can make it to the top of the switchbacks are rewarded great views of the snow-capped Sierra across the Owens Valley.
The Discovery Trail climbs for a couple hundred more yards beyond the switchbacks, but just as you’re beginning to wonder whether all the effort is worth it, the trail levels, turns, and drops. Soon you’ll round a 90-degree bend and be rewarded for your hard work with two of the most spectacular bristlecones in the entire forest. Spend as much time here as you have, because the rest of the loop back to the parking lot has nothing to compete with these two trees.
The pavement ends at the Schulman Grove, but the unpaved 12-mile drive to the Patriarch Grove is navigable by all vehicles in dry conditions. Home to the Patriarch Tree, the world’s largest bristlecone pine, the Patriarch Grove is more primitive and much less visited than the Schulman Grove. Unlike the Schulman Grove, where I rarely stray far from the trail, I often find the most photogenic bristlecones here by venturing cross-country, over several small ridges east of the Patriarch Tree. Even without a trail, the sparse vegetation and hilly terrain provides enough vantage points that make getting lost difficult.
Clean air, few clouds, and very little light pollution make the bristlecone groves a premier night photography location. On moonless summer and early autumn nights, the bright center of the Milky Way is clearly visible from the slopes of the bristlecone forest. For the best Milky Way images, look for trees that can be photographed against the southern sky. And no matter how warm it is on 395 below, pack a jacket.
The bristlecone forest closes in winter.
An hour north of Lone Pine on 395 is Bishop. Its central location, combined with ample lodging, restaurant, and shopping options make Bishop an excellent hub for an Eastern Sierra trip—if you want to anchor in one spot and venture out to the other Eastern Sierra locations, Bishop is probably your best bet.
West of Bishop are many small but scenic lakes nestled in steep, creek-carved canyons that are lined with aspen (and some cottonwood) that turn brilliant yellow each fall. Many of these canyons can be accessed on paved roads, others via unpaved roads of varying navigability, and a few solely by foot.
Of these canyons, Bishop Creek Canyon is the best combination of accessible and scenic. To get there, drive west on Highway 168 (Line Street in Bishop). After about 15 miles you can decide whether to turn left on the road to South Lake, or continue straight to reach North Lake and Lake Sabrina (pronounced with a long “i”).
One of the area’s most popular sunrise spots, North Lake is a 1-mile signed detour on a narrow, steep, unpaved road—easily navigated in good conditions by all vehicles, but the un-railed, near vertical drop is not for the faint of heart. A mile or so beyond the turn to North Lake the road ends at Lake Sabrina, a fairly large reservoir in the shadow of rugged peaks and surrounded by beautiful aspen (but its bathtub ring when less than full is not for me).
South Lake is another aspen-lined reservoir that shrinks in late summer and autumn. Highlights on South Lake Road are a manmade but photogenic waterfall leaping from the mountainside, clearly visible on the left as you ascend, and Weir Lake, just before South Lake.
Both Bishop Canyon roads are worth exploring, especially in autumn, when the fall color can be spectacular. Each features scenic tarns and dense aspen stands accented by views of nearby Sierra peaks. Rather than beeline to a fall color spot, in autumn I drive the Sabrina and South Lake roads and pick the best color.
Highway 395 north of Bishop features a few of my favorite fall color destinations, including Rock Creek Canyon and McGee Creek. About a half hour north of Bishop, detour west off the highway to postcard-perfect Convict Lake. And just beyond the road to Convict Lake is the upscale resort town of Mammoth Lakes, just a few miles west of 395. The drive on 203 through Mammoth Lakes takes you past the Mammoth Mountain Ski slopes to Minaret Vista. This panoramic view of the sawtooth Minaret Range, Mt. Ritter, and Mt. Banner captures the essence of high Sierra beauty. From here, follow the road down the other side to see the basalt columns of Devil’s Postpile, and to take the short hike to Rainbow Fall.
Lee Vining area
Leaving Bishop, Highway 395 climbs steeply, crests near Crowley Lake, skirts the communities of Mammoth Lakes and June Lake, finally dropping down into the Mono Basin and Lee Vining. Though this is an easy, one-hour drive, you’ll feel like you’ve landed on a different planet. In October, detour onto the June Lake Loop, another popular fall color drive.
By far the most popular Mono Lake location is South Tufa, a garden of limestone tufa towers that line the shore and rise from the lake. Tufa are calcium carbonate protrusions formed by submerged springs and revealed when the lake drops. In addition to the striking tufa towers, South Tufa is on a point that protrudes into the lake, allowing photographers to compose with both tufa and lake in the frame while facing west, north, or east.
To visit South Tufa, turn east on Highway 120 about 5 miles south of Lee Vining. Follow this road for another 5 miles and turn left at the sign for South Tufa. Drive about a mile on an unpaved, dusty but easily navigated road to the large dirt parking lot. From here it’s an easy ¼ mile walk to the lake, but wear your mud shoes if you want to get close to the water. And don’t climb on the tufa.
While South Tufa can be really nice at sunset, mirror reflections on the frequently calm lake surface, and warm light skimming over the low eastern horizon, make this one of California’s premier sunrise locations. To get the most out of a sunrise shoot here, it’s a good idea to photograph South Tufa at sunset to familiarize yourself with the many possibilities here (and who knows, maybe you’ll get lucky and catch one of the Eastern Sierra’s spectacular sunsets).
In the morning, arrive at the lake at least 45 minutes before sunrise to ensure a good spot at this popular location—you can start shooting as soon as you arriving, using long exposures to brighten the scene and smooth the water. I usually start with scenes to the east, capturing tufa silhouettes against indigo sky and water. As the dawn brightens, keep your head on a swivel and be prepared to shift positions with the changing light.
As the sun approaches and the dynamic range increases in the east, I often turn to face west. Soon the highest Sierra peaks are colored with pink alpenglow, followed quickly by the day’s first direct sunlight. With the sun rising beneath the horizon behind me, its light slowly descends the Sierra peaks stretching before me. When the sunlight finally reaches lake level, for a few minutes the tufa towers are awash with warm sidelight, creating wonderful opportunities facing north. As with the Alabama Hills, without clouds to soften the sunlight and make the sky more interesting, the sunrise show is terminated quickly by contrasty light.
Other options in and near Lee Vining are the excellent Mono Lake visitor center on the north side of town, the small but very informative Mono Committee headquarters in the middle of town, any meal at the Whoa Nellie Deli in the Mobil Station (trust me on this), and Bodie, an extremely photogenic ghost town maintained in a state of arrested decay, less than an hour’s drive north. And a sinuous 20-minute drive west, up 120 (closed in winter) lands you at Tioga Pass, Yosemite’s east entrance and the gateway to Tuolumne Meadows.
Fall color in the Eastern Sierra
Each fall the Eastern Sierra becomes a Mecca for photographers chasing the vivid gold coloring the area’s ubiquitous aspen groves. The show starts in late September at the highest elevations, and continues well into October in some of the lower elevations. Fall color timing and locations vary from year-to-year, but the general fall color rule to follow here is: If the trees are still green, just keep climbing.
The best way to photograph the Eastern Sierra’s fall color is to explore: Pick a road that heads west and start climbing until something stops you. To give you a head start, here are a few of my favorite spots, from south to north. (Rather than beeline to specific locations in these ever-changing canyons, I’ve found it’s best to drive slowly and stay alert for opportunities along the way.)
Bishop Creek Canyon: Nice any season it’s open, Bishop Creek Canyon (detailed earlier) comes alive with gold each autumn. Aspen surrounding the canyon’s many lakes make for spectacular reflections. Of these, North Lake is probably the most popular, but autumn mornings can be extremely crowded here. The color in Bishop Creek Canyon usually peaks in late September at the highest elevations (near North Lake, Lake Sabrina, and South Lake), but lasts until mid-October farther down the canyon.
Rock Creek Canyon: Near the crest of the climb out of Bishop on 395, turn left at the sign for Rock Creek Lake. Climb this road along Rock Creek all the way up to its terminus at Mosquito Flat trailhead. Over 10,000 feet, this is the highest paved road in the Sierra. As with Bishop Creek Canyon, the best photography in Rock Creek Canyon is usually found at random points along the road—drive slowly and keep your eyes peeled.
McGee Creek: When you see Crowley Lake on the right, look for the road to McGee Creek on the left. This 2-mile unpaved road is navigable by all vehicles, but take it slow. It ends at a paved parking lot that’s the launching point for a hike up McGee Creek, into the canyon, and the mountains beyond. Unlike most other Eastern Sierra canyons, the dominant tree here is cottonwood. While I’ve had good success photographing along the creek right beside the parking lot, you can find nice color as far up the canyon as your schedule (and fitness) permits.
Convict Lake: The road to Convict Lake is just south of Mammoth Lakes. It’s a 2-mile paved drive to a beautiful lake nestled at the base of towering mountains—definitely worth the short detour off of 395.
June Lake Loop: Between Mammoth Lakes and Lee Vining is a 15 mile loop that exits 395 near the small town of June Lake (look for a gas station on the left) and returns to 395 a few miles down. Along the route you’ll find several lakes, and a waterfall at the very back of the loop (visible from the road).
Lundy Canyon: About 5 miles north of Lee Vining, turn left onto the Lundy Canyon road to enjoy one of my favorite Eastern Sierra fall color spots. The lower half of this road, below Lundy Lake, is often a good place to find late season color, but my favorite photo spots aren’t until road turns bad, just beyond the lake.
Driving slowly and with great care, most vehicles can make the 2 unpaved miles along Mill Creek to the end of the road. In addition to beautiful creek scenes, you’ll find several small, reflective beaver ponds along the way. If you make it to the end of the road, park and follow the trail up the canyon, through an aspen grove, for about ¼ mile to reach a small, waterfall-fed lake. The overgrown lakeshore makes photography here difficult, but a short walk along the shoreline to the left, toward the lake outlet, will take you to a massive beaver dam. Roll up your pants and get your feet (and more) wet for the best views of the lake.
Dunderberg Peak and Virginia Lakes: Shortly after the turn to Lundy Canyon, 395 climbs steeply to Conway Summit, at 8143 feet, the highest point on the entire route. On the left, just past a spectacular view of the entire Mono basin (worth the stop), is the road to Virginia Lakes. Here you’ll find some of the area’s earliest aspen to turn. Just beyond the Virginia Lakes road are colorful views of Dunderberg Peak and its aspen-blanketed slopes.
Posted on February 19, 2017
“… the mighty Sierra, miles in height, and so gloriously colored and so radiant, it seemed not clothed with light but wholly composed of it, like the wall of some celestial city…. Then it seemed to me that the Sierra should be called, not the Nevada or Snowy Range, but the Range of Light.” — John Muir
Anyone who has spent time in or around the Sierra Nevada has to agree that there’s something special about its interaction with light. Towering one to two miles above the surrounding terrain for nearly all of its 400-mile length, the Sierra Nevada are California’s most prominent natural feature. But it’s not just prominence that sets the Sierra apart. The Sierra are almost entirely granite, an intrusive igneous rock comprised primarily of light-toned feldspar and liberally infused with lustrous quartz and mica. Because igneous intrusive rocks form deep beneath the Earth’s surface, constituent minerals cool and harden slowly enough for large, reflective crystals to form.
In addition to its inherently reflective qualities, granite is quite hard and resistant to erosion. Unlike the overlying sedimentary and metamorphic rock that washed downhill as the Sierra pushed (and continues to push) upward, granite remains intact when subjected to wind and rain. Eventually small cracks form; water percolating into these cracks expands as it freezes, widening the cracks further until the granite fractures and a large block separates. The result is large vertical and domed surfaces whose extreme slope and hardness are particularly inhospitable to plant life, even well below the timberline. Granite’s hardness also means that rather than crumbling beneath the weight of the numerous glaciers to scour the Sierra, much of the Sierra granite has been polished to a glassy sheen.
Granite’s light complexion, reflective inclusions, and abundance of exposed, polished surfaces make the Sierra particularly inclined to reflect the color of whatever light illuminates it. This relationship with light is quite evident in Yosemite Valley, nestled in the range’s more moderately sloped west side. When the sun strikes Yosemite’s Half Dome and El Capitan at day’s end, warm sunset light paints these monoliths in brilliant orange and red hues just before the sun is snuffed by the horizon. While this color can be seen at sunset year round, it takes center stage each February when sunset shadow and light conspire to highlight normally insignificant Horsetail Fall’s tumble down El Capitan’s east face.
As exquisite as the light on Yosemite’s granite is, I’m even more drawn to the Sierra’s east side, which gets its best sun at sunrise. Unlike the Sierra’s gradually sloped, relatively moist, and largely foliated west slopes, the Sierra’s east side is much steeper, drier, and therefore sparsely foliated and more exposed. Enhancing the drama, the Eastern Sierra’s towering granite face also catches the earliest possible sunlight, sunlight that has traveled farther and through purer air (because there fewer airborne pollutants in the morning in general, and the sunlight east of the Sierra traverses much less densely populated terrain).
My favorite place to watch the light play on the Eastern Sierra granite is in and near the Alabama Hills, two vertical miles beneath Mt. Whitney and the Sierra’s most precipitous section. Looming above the Owens Valley, 14,505 foot Mt. Whitney is the highest point in the 48 contiguous United States. Unlike many towering peaks that stand by themselves, Mt. Whitney is bounded by 13,000 foot Lone Pine Peak and 14,000 foot Mt. Williamson, all connected by a serrated ridge of 13,000+ foot sharks tooth prominences.
Before sunrise I like to arrive early enough to see the Sierra crest reflect the pale blue of the pre-dawn sky, then watch it warm gradually as the sky brightened before the approaching sun. The color reaches a crescendo when the sun’s longest wavelengths first kiss the highest peaks with pink alpenglow. As the rest of the sun’s visible wavelengths join the party, the crest warms to amber before finally cooling beneath the daylight-blue sky.
At the end of the day the best color arrives after the sun has long disappeared behind the crest and the entire scene is illuminated by a sky well on its way to night. Though the mountains’ color is more subtle than the sunrise show, the Eastern Sierra’s granite when imbued with the pale mauve of evening twilight is no less beautiful. Eventually night takes over and once again the Sierra granite throbs a soft blue.
Early last October I guided my Eastern Sierra workshop group up to Whitney Portal at the base of Mt. Whitney to photograph cascading Whitney Portal Fall in late afternoon shade. On the drive back down we squeezed into a small turnout not too far down the road for the closest view of Whitney that doesn’t require a serious hike. This year’s group got a bonus when a thin slice of brand new moon appeared shortly after sunset.
Mounting my Sony 70-200 f4 on my a7RII, I framed the scene as tightly as I could while still including both Mt. Whitney and the crescent moon. Though the sky was clear, a steady stream of small clouds materialized as if issued by a cloud making machine just out of sight behind the crest to the right of Whitney. Each new cloud scooted to the left and dissipated quickly in drier air near the summit. After composing, metering, and focusing, I waited for the next cloud to appear and clicked this frame in the purple twilight.
Posted on March 4, 2016
Rules are important. The glue of civilization. And after a childhood constrained by bedtimes, homework, and curfews, it’s no wonder that as adults we honor rules simply because, well, simply because. (I mean, who doesn’t wait for however long it takes and with no car or cop in sight, for a light to change?)
As much as civil society relies on universal obedience, not all “rules” are created equal. And our reluctance to question authority inhibits growth. One example would be blind adherence to the (usually) well-intended photography “experts” proliferating in print, online, and (especially) in your local camera club. These self-proclaimed authorities have figured out that people who are just learning are less confident, and tend to respond more to authority than substance.
The camera club paradox
I think camera clubs are great for many reasons: they connect people with a common interest, facilitate the exchange of information and ideas, and provide a forum for sharing our photographic creations. Camera clubs spur us to get out and shoot when we otherwise might stay home, and offer the beginner rules that provide a stable foundation upon which to build her craft.
But camera clubs can also be a breeding ground for self-proclaimed experts, a status often not conferred to the person most qualified, but to the person who spews photographic dogma with the most authority. The result is well-intended but misinformed knowledge that infects a camera club like a mutated virus.
I’m especially troubled when I hear of images shared in a camera club photo competition that were dismissed without consideration because they violated the local “expert’s” idea of an unbreakable photographic rule. Some camera club capital “violations” I’ve seen firsthand or heard about (by no means a comprehensive list):
Each of these things can be a problem, but they can be a refreshing expression of creativity as well. And even if they are a problem, refusing to consider an image because it violates someone’s definition of “perfect” discounts all that’s potentially good about it.
If you’re an aspiring photographer and someone dismisses an image for a technical violation, take a step back, inhale, and remind yourself that there are very, very few absolutes in photography. In general, it’s helpful to remember that no matter how strongly it’s stated, advice that doesn’t feel right (even if you can’t articulate why) doesn’t need to be heeded. In fact, the next time someone starts feeding you photography advice in absolutes, run (don’t walk) to the nearest exit.
About this image
I jumped on my anti-expert soapbox after observing several recent workshop participants who were clearly constrained by “rules” enforced by their local camera club. And looking at this image, I realized that there are camera clubs that probably wouldn’t even consider it because I centered the horizon and the teddy-bear shaped rock in the foreground. I also captured a little more star motion than is ideal. But deal breakers? Not to me.
I’d taken my January Death Valley workshop group out to the Alabama Hills for a moonlight shoot on the workshop’s last night. A few in the group walked out to the arch, but most gravitated to this group of boulders a little south of the parking area. As I worked to get the group up to speed with moonlight photography, I tried a few frames of my own.
Most of my moonlight images are fairly wide, and even the closest focus point is far enough away to be at infinity, even wide open. But the rocks here were close enough, and my focal length was long enough (57mm), that I stopped down from f4 to f5.6 to increase my margin for error. And rather than autofocusing on the moon as I normally do, I focused toward the back of the foreground rocks. As I hope you can see in this low-res web version, I made the right focus choices.
The other problem I had to contend with was motion blur in the stars. At the 16mm to 24mm I typically use for night photography (to maximize the number of stars), motion blur isn’t much of a problem, even at 30 seconds. But at nearly 60mm, I didn’t think I could get away with 30 seconds. This is the first time I’d tried my Sony a7RII at night—I usually use my a7S, but I’d heard such good things about the a7RII’s high ISO capability that I thought I’d try it.
Bumping the ISO to 3200 (from my moonlight standard of 800), I was able to drop my shutter speed to 15 seconds. This image is so clean at 3200, and the star motion is visible enough, that I regret now that I didn’t go to ISO 6400 and cut my shutter speed to 8 seconds. Next time….
(Images that might not make the cut at a camera club competition)
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Posted on February 7, 2015
Like most people, my original expectation for my nascent mirrorless world was a significantly lighter backpack, and indeed, I haven’t been disappointed. In my Canon days my primary pack was an F-Stop Tilopa with a medium ICU (F-Stop’s interchangeable internal module for storing and organizing gear), which held my 5D Mark III, Canon 16-35 f/2.8, 24-105 f/4, and 70-200 L lenses, plus a Zeiss 28 f/2 (for night photography). Unless I specifically planned a shoot that required it, my Canon 100-400L and 100 macro lenses traveled with my backup Canon body in a separate bag—not a big deal when I’m driving to a destination, but pretty much a non-starter when I have to fly (which I’m doing more and more).
After moving to the mirrorless Sony a7R, I immediately started using my smaller F-Stop Guru backpack, which easily handled the new body and the Sony equivalent of my primary Canon glass: Sony/Zeiss 16-35 F/4 and 24-70 f/4, Sony 70-200 f/4 G, plus the (Canon mount) Zeiss 28 f/2 and a Metabones adapter that allows me to use my Canon glass on a Sony EF mount body. This configuration gave me essentially the same focal range I had with Canon, in a significantly smaller, lighter package. Not only that, I can use a lighter tripod and head. Score.
But, since I hate shooting without a backup body and had heard fantastic things about the camera, I soon purchased a Sony a6000. This amazing little mirrorless camera’s 1.5 crop sensor makes it an ideal complement to my full-frame a7R, has (slightly) more resolution than the 5DIII, and (so far) appears to offer (at least) comparable image quality, with better dynamic range than the Canon. And with a little bit of rearranging, I found I could fit the a6000 into my Guru bag without jettisoning anything else.
The result of this downsizing is a camera pack that’s light enough for hiking without feeling like a backpacker, and and for cycling without feeling like I’m about to tip over.
For my ultra-telephoto needs, my plan all along had been to to use the Canon 100-400 with the Metabones adapter. But since the 100-400 had always been my least favorite lens—awkward to use, and not particularly sharp—I had no real plans to add it to my regular lens rotation. But my ears perked up when I started hearing my friend and similarly recent Sony convert (and fellow pro photographer) Don Smith raving about the Tamron 150-600 lens. Hmmmm….
The Tamron 150-600 arrived shortly before I departed for last week’s Death Valley / Mt. Whitney Winter Moon photo workshop. Because the Tamron lens isn’t available with a Sony FE mount, it would require an adapter as well. Don had been shooting the Sony A-mount version of the Tamron paired with Sony’s converter; I opted for the Canon mount version, reasoning that I could use it on my remaining Canon bodies should the need ever arise, and I already have the Metabones adapter. (Word on the street is that the Sony A-mount Tamron with the Sony adapter has much better autofocus than the Canon/Metabones combination, but I don’t need autofocus.)
First reaction? This is not a small or light lens. But as soon as I started using it, two things became clear: it’s much easier to use than my Canon 100-400, and it’s noticeably sharper. Suddenly, size notwithstanding, I had a lens that I could see myself using regularly.
If I’d still been lugging my Canon gear, I’d have had to sacrifice essential lenses each time I planned to use the 150-600. But with the mirrorless system and a little reconfiguring of the compartments in the Tilopa ICU (moving around the padded, Velcro-attached partitions), I can now carry in a single camera backpack (that fits in every overhead bin I’ve ever encountered, including the puddle-jumpers): three Sony bodies (a7R, my brand new a7S, and the a6000), plus lenses that give me a focal length range from 16 to 900 mm (the 150-600 lens is a full-frame equivalent of 225-900 mm on the 1.5-crop a6000). Life’s good.
In the field
So, what does a photographer do with all this new imaging power? Use it, of course. Visiting familiar locations as much as I do, I can’t tell you how refreshing it is to find a completely new way to see these landscapes.
The image at the top of this post was from my first time using the Sony a6000 and Tamron 150-600. To get a better handle on the conditions, I left home two days before the workshop, spending the first night in Lone Pine, near the Alabama Hills just beneath Mt. Whitney. After a moonlight shoot in the Alabama Hills, the next morning I rose before sunrise, strolled from my hotel room across the highway, and set up my tripod with the Tamron 150-600 mounted and a6000 attached.
The first time I aimed this combination at Mt. Whitney (the highest peak in the 48 contiguous United States), zoomed all the way out to 900mm (600mm x 1.5), and dialed in the focus, was an epiphany. Previously unseen rocks and trees snapped into view, and vortices of wind-swept snow spun on the summit. Amazing to my eye, but at 900 mm actually too close to find a composition I liked. So I pulled all the way back to a little less than 400 mm (256 x 1.5), framed up the mountain, and waited for the pink that always kicks off a Mt. Whitney clear-sky sunrise.
I captured this frame about ten minutes before sunrise. Being a little concerned about such a long focal length in low light, I hedged my bets slightly by using ISO 200 to halve my shutter speed. Since I notice little difference between ISO 100 and 200 on the a6000, I think 200 will be my standard ISO when I use the 150-600 on this body. But we’ll see.
The rest of the week was a rediscovery of ultra-telephoto photography. When I first switched to digital about twelve years ago, I started with a 1.6 crop Canon 10D, and my only telephoto lens was a 70-300, making images up to 480 mm a routine part of my capture paradigm. Isolating distant subjects, magnifying closer subjects, compressing foreground and background subjects—it was all a simple matter of reaching into my camera bag. But since switching to full-frame, and replacing the 70-300 with the (faster, optically better) 70-200, ultra-telephoto photography took backseat to more conventional landscapes, and I eventually forgot how much I enjoyed it when it was more convenient. Ultra-telephoto became something I had to plan, rather than a creative option available whenever the inspiration struck.
Don was assisting my Death Valley workshop (Don and I trade off assisting many of each other’s workshops), and I’m sure by the end of the week the group had grown weary of hearing Don and I gush about the fun we were having with our new toys. Sand dunes, moonrise, moonset, distant peaks—no natural feature was safe from our magnifying eye. A particular highlight came dark and early one morning at Dante’s View, when I turned the a6000 and 150-600 to Jupiter, low on the horizon near Telescope Peak, gathered the group around my LCD, zoomed to 600mm, and shared the glowing disk of our solar system’s largest planet surrounded by the four Galilean moons.
The bottom line
Mirrorless has definitely meant a significantly smaller, lighter bag to handle my “meat and potatoes” 16-200 mm focal length range (that I never leave home without) when mobility is paramount—hiking or biking, I hardly know there’s anything on my back.
But equally significant is the way compact mirrorless gear also allows me expand my creative options without hiring a Sherpa. Now, in the same backpack that once maxed out with a single Canon body (most recently a 5D Mark III) and Canon lenses covering 16-200 mm, I can travel with three mirrorless bodies, plus lenses covering an effective focal range from 16-900 mm (including my 28 mm f/2 Canon-mount Zeiss for night photography). Life’s good.
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Posted on January 20, 2014
A good landscape image usually involves, well…, a good landscape. But that’s only half the equation—photographers also need photogenic conditions—soft light, interesting skies, dramatic weather, or anything else that elevates the scene to something special. While we have absolute control over the time and location of our photo outings, the conditions have a significant random (luck) component.
Despite being less than a day’s drive from many of the most treasured photo destinations in the world, most of my photo trips are planned months in advance. Workshops in particular require at least a year of advance planning on my part, and many months of schedule adjustment and travel arrangements for the participants. I think I’ve pretty much established that positive thinking, finger crossing, divine pleas, and ritual incantation (no virgin sacrifice yet) are of zero value where photography is concerned—sometimes conditions work out wonderfully, sometimes not so much. And while I’ve photographed my workshop locations many times, I know most of my workshop participants haven’t, which is why I do my best to schedule my workshops when the odds are best for interesting skies.
My annual Death Valley / Mt. Whitney photo workshop is a perfect example: Among the driest places on Earth, Death Valley gets only about an inch of rain each year and suffers from chronic blue skies. Ever the optimist, I schedule my DV/Whitney workshop from mid-January through early February, when the odds, though still low, are at least best for clouds. And while I’ve actually been pretty lucky with the clouds in past workshops, to hedge my bets further, I always schedule this workshop to coincide with a full moon—if we don’t get clouds, the moon always seems to save the day (and night).
This year’s DV/Whitney workshop wrapped up Saturday morning. Unfortunately, it landed in the midst of what is on its way to becoming an unprecedented drought in California. After two dry winters, this winter is worse—a persistent high pressure system has set up camp above California, creating an impenetrable force field that deflects clouds and and bathes the state weather that is absolutely beautiful for everything but photography. In this year’s DV/Whitney workshop’s four+ days, we enjoyed highs in the glorious 80s, and I don’t recall seeing a single cloud (though there were unconfirmed rumors of a cloud sighting on the distant horizon late in the workshop).
But cloudless skies don’t need to mean lousy photography—they just shrink the window of opportunity. Places like Mosaic Canyon and Artist’s Palette are nice in the early morning or late afternoon shade. And in general, when clouds aren’t in the picture, the best photography skies are on the horizon opposite the sun before sunrise and after sunset. Last week I made a point of getting my group on location at least 45 minutes before sunrise, and kept them out well past sunset to photograph Death Valley’s one-of-a-kind topography beneath twilight’s shadowless pink and blue pastels. Among other things, in this light the dunes were fantastic (I was able to find a relatively footprint free area) all the way from shadowless twilight through high contrast early morning light, and the first light on Telescope Peak from Badwater was wonderful.
But the workshop’s real highlight, the element that elevated our week into something special, was the moon. The real moon show didn’t begin until it showed up above the primary views on our final two sunrises, but we got a nice preview on our first sunset when the waxing gibbous disk rose into the twilight wedge above the mountains east of Hell’s Gate. The next evening I took the group to panoramic Dante’s View; while the prime objective was photographing Death Valley’s last light and the sun setting from 5,000 vertical feet above Badwater, I instructed everyone to walk across the parking lot after sunset to catch the nearly full moon rising above the equally expansive (though significantly less spectacular) panorama of distant peaks to the east. The moon arrived early enough to allow at least ten minutes of quality photography, then we just kind of hung out to watch it for a little while longer. Very nice.
Friday morning’s sunrise we found the moon glowing as promised in the predawn indigo above Zabriskie Point. As the morning brightened, we watched the nearly round disk slide through twilight’s throbbing pink before disappearing directly behind Manly Beacon just a few minutes after sunrise.
But as nice as the Zabriskie shoot was, I think my personal favorite was the workshop’s final sunrise from the Alabama Hills. The group, now expert at managing the difficult contrast between foreground shadows and brilliant moon, immediately spread out to find their own foreground. One or two headed straight for the Whitney Arch (aka, Mobius Arch), while the rest of us were quite content with the variety of boulders west and south of our the arch.
The thing that makes the Alabama Hills such a special location for sunrise is its position between towering peaks to the west, and relatively flat horizon to the east. At sunrise here, the Sierra crest juts into the blue and rose of the Earth’s receding shadow, then transitions to amber when the first rays of sunlight kiss its serrated peaks. You anticipate watch the sun’s arrival by watch the shadow descent the vertical granite until it bathes the weathered boulders with warm, ephemeral sunlight. Then, just like that, the show’s over.
I’ve shot this scene at sunrise so many times that I usually remain a spectator unless something special moves me to pull out my camera. Last Saturday, despite the absence of clouds, I just couldn’t resist the pull of the moon, which hovered like a mylar balloon in the night/day transition. At first there wasn’t enough light to photograph detail in the rocks and moon in a single frame, but eventually, with the help of a two-stop graduated neutral density filter, I was able to capture the image at the top of the blog.
Posted on March 1, 2013
It’s fun to browse the thumbnails from a shoot in chronological order to see the evolution of that day’s process. While can’t always remember specific choices, it’s always clear from the progression of my images that I was indeed quite conscious of what I was doing. I can look at one thumbnail and usually predict what the next will be.
This January morning in the Alabama Hills started for me about forty-five minutes before sunrise. When the sun finally warmed Mt. Whitney, a 95% waning gibbous moon was about to dip below the Sierra crest; comparing images, it’s clear I’d moved no more than twenty feet from the location of that morning’s earliest images. This is pretty typical of my approach—unlike many (but not all) photographers, who actively bounce around a location in search of something different, I tend to seek the scene until I find it, then work it to within an inch of its life. If I’m moving around, it usually means I haven’t found something that completely satisfies me.
Is mine the best approach? Of course not, but it is the best approach for me. There is no all encompassing rule for workflow in the field, except maybe to be true to your instincts. Because I happen to be very deliberate in my approach to many things, and can be incredibly (obsessively?) patient when I sense the potential for something I want, that’s the way I shoot. But, regardless of changing conditions and possible compositional variations, some photographers would go crazy locking into one scene. And just as my deliberate approach continually reveals details I’d have missed had I moved on sooner, it sometimes cheats me of even better opportunities waiting just around the corner. But I learned a long time ago not to stress about what I might be missing (because for me it’s even worse to chase what’s around the corner only to find what I end up with doesn’t match what I left).
Early on this chilly morning I found a relationship between a nearby stack of boulders and the distant Sierra peaks (Mt. Whitney in particular); the more time I spent with the scene, the more I saw and the better all the elements seemed to fit for me, so I just kept working. It didn’t hurt that conditions were changing almost as quickly as I could compose. Clouds ascended from behind Mt. Williamson as if churned out by a cloud making machine, sprinted south past Mt. Whitney, and disappeared behind Lone Pine Peak. On their way they took on whatever hue the rising sun was delivering, from white (before the sun) to vivid pink to amber.
Comparing today’s image to the image in my previous post, I see that my composition shifted to account for the moon. In the earlier image the most prominent boulder and Mt. Whitney serve as a set that anchors the center of the frame. In the later image I keep the set together but offset them to the left to balance the moon’s extreme visual weight. And while at first glance it appears both images were captured from the same spot with just slight focal length and direction adjustments, the height and position of the foreground boulder relative to Mt. Whitney’s summit shows that I’ve moved a little left and about twenty feet closer.
Relationships between elements in a frame are essential to an image’s success—controlling these relationships is a matter of moving up/down, left/right, forward/backward. Without remembering my decision to move that morning, I can still reconstruct my likely thought process: The more I worked the scene, the more clear I became on where the boulders’ left and right boundaries should be. Moving left and closer let me go wide enough to include the moon and clouds, fill the foreground with no more of the foreground boulders than I wanted, and balance the frame with the boulder/Whitney pair on the left and the moon on the right.
So while I do indeed stick with one scene for a long time, I’m far from static. Each frame is slightly different from the previous one. Like most of my favorite images, this Whitney sunrise moonset is an evolution; it started in the dark, evolving with the conditions and my growing familiarity with the scene’s elements.
There are no guarantees in nature, and I’ve had my share of “panic shoots” when something unexpected forced me to run around frantically searching for a scene to go with the moment. But when this morning’s dance of light, clouds, and moon blended into one of those magic moments photographers dream about, I was ready.
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Posted on February 24, 2013
Compared to the human eye, the camera’s vision has many shortcomings (as photographers are quick to lament). At the top of photographers’ list is the very narrow gap separating the brightest and darkest tones a camera can capture: dynamic range.
But while the camera taketh away, it also giveth. Experienced photographers understand that what we perceive as complete darkness is really just our eyes’ relatively limited ability to gather light, combined with the brain’s insistence on processing this limited input instantaneously. But a camera’s sensor (or a rectangle of unexposed film) can accumulate all the light striking it for whatever duration we prescribe, thereby stretching its “instant” of perception indefinitely. Advantage camera.
For example, the camera’s narrow dynamic range is (exquisitely) mitigated in the barely perceptible light preceding sunrise and following sunset. Unlike night photography, when the light in the sky is so faint that extremely long exposures are required to register any foreground detail, and daylight/moonlight photography, when unidirectional light casts high contrast shadows that exceed a camera’s dynamic range, pre-sunrise/post-sunset twilight light is spread so evenly overhead that most shadows disappear.
About this image
Horizon-to-horizon skylight made dynamic range a non-factor in the above Alabama Hills pre-sunrise scene, while my camera’s instant-stretching ability revealed beauty present in a landscape that was nearly invisible to my eyes.
White with snow and towering 10,000 vertical feet above the Alabama Hills, Mt. Whitney loomed in dramatic contrast to the dark sky and foreground. As my eyes adjusted to the limited light, the jumbled rocks of the Alabama Hills became vague, colorless shapes. Anyone relying on their eyes on this January morning would likely conclude that there’s not enough light for photography. But I knew better.
Juxtaposing a nearby fortress of boulders against Whitney’s serrated outline, I framed my image. While the mountains were the dominant feature to my eyes, I knew my long exposure would make the nearby rocks equally prominent—their sharpness was essential. Limited light made autofocus on the rocks out of the question, so I stopped down to f16 to increase my margin for error and focused manually.
As planned, a thirty-second exposure at ISO 400 uncovered volumes of invisible detail and color my eyes missed. (The scene took two or three exposures to get right as I really felt like I was composing blind.) Though I was photographing in a fairly stiff (and frigid!) breeze at 4,500 feet, it was nothing like the hurricane wind that smeared the clouds above Whitney to an ethereal glaze during the 30 second exposure. Another revelation of the long exposure was the sky’s exquisite, natural (not processing-enhanced) blue.
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Posted on January 24, 2012
The foreground for Mt. Whitney is the rugged Alabama Hills, a disorganized jumble of rounded granite boulders, familiar to many as the setting for hundreds of movies, TV shows, and commercials. These weathered rocks make wonderful subjects without the looming east face of the southern Sierra. What makes this scene particularly special is the fortuitous convergence of topography and light that rewards early risers with a skyline dipped in pink–add a few clouds and it’s a photography trifecta.
We’ve all seen the pink band above the horizon opposite the sun shortly before sunrise or after sunset. Sometimes called “the belt of Venus,” this glow happens because sunlight that skims the Earth’s surface just before sunrise (or shortly after sunset) has to battle its way through the thickest part of the atmosphere, which scatters the shorter wavelengths (those toward the blue end of the visible spectrum), leaving just the longer, red wavelengths capping the horizon. When mountains jut high enough to reach into this region of pink light, we get “alpenglow.” Towering above the terrain to the east, the precipitous Sierra crest, anchored by 14,500 foot Mt. Whitney (the highest point in the contiguous 48 states) and 13,000 foot Lone Pine Peak, is ideally located to receive this sunrise treatment.
The image above was captured on a frigid January morning. While the best light on the Sierra crest usually starts a couple of minutes before the “official” (flat horizon) sunrise, this morning Mt. Whitney hid behind the clouds until the alpenglow was well underway. Like a piece of art waiting for its spotlight, the cloudy shroud was pulled back just as the sunlight struck Mt. Whitney, and for a couple of minutes it appeared as if a giant paintbrush had dabbed the swirling canvas with pink.
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