Wilderness Portraits by Lloyd Paul Aiello

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  • A juvenile male Mallard Duck (Anas platyrhynchos) is illuminated by a ray of early morning sunlight.
    _LPA0396-mallard-duck-sun-pond.tif
  • On August 21, 2017 the path of the first solar eclipses over the Unites States in 38 years traversed approximately 2,500 miles of the country from Newport, Oregon to McClellanville, South Carolina.  Just outside Shoshoni, Wyoming, the path passed over Boysen Reservoir.  At this location, totality lasted 2 minutes and 22 seconds, being at its maximum about 11:40 am.  With the moon blocking the solar disk during totality, red flares called solar prominences become visible at the edge of the dark disk.  The red-glowing looped material is plasma, a hot gas composed of electrically charged hydrogen and helium. These prominences look small in relation to the size of the sun, but typically extend over many thousands of kilometers with the largest on record being estimated at over 800,000 kilometres (500,000 miles).  A prominence forms over timescales of about a day and may persist for several weeks or months.<br />
<br />
During the total solar eclipse, the sun’s outer atmosphere called the corona becomes visible as it extends millions of miles into space.  The corona consists of extremely hot ionized gases which exceed 1 million degrees Kelvin – 150- to 450-times hotter than the surface of the sun.  Being over 1 million million times less dense and much hotter than the sun’s surface and the solar prominences, the corona actually produces about one-millionth as much visible light, thus becoming visible from earth typically only during a total solar eclipse. The sun’s magnetic fields bend the corona into its remarkable shapes.<br />
<br />
In this image, 10 different photographic exposures of the solar eclipse were composited to show the eclipsing moon, solar prominences and the corona.  The image was then manipulated by a process involving radial blur subtraction and image offset overlay to accentuate the pattern of the corona. The coloration of the eclipsing moon and the solar prominences were retained in this rendition.  (exposure stack of 10 images)
    total-solar-eclipse-sun-corona-overl...tif
  • _LPA0097-Edit-boy-jump-teton-river-i...tif
  • LB catches a 19.5 inch Rainbow Trout on a dry fly while flyfishing on the Upper Narrows of the Teton River near Drggs, Idaho. The fish was released unharmed after the photograph.
    _LPA0035-Edit-Rainbow-Trout-Teton-Ri...tif
  • Sitting at the base of the Temple of the Moon, LB (age 8) gazes at sunrise reflecting off the 400-foot-tall Temple of the Sun in Cathedral Valley, Capital Reef National Park, Utah. The spectacular monolith is composed of Entrada Sandstone deposited 160 million years ago in the Jurassic period.  This fine-grained sandstone is formed by the deposition of silt in tidal flats. It crumbles easily to a fine sand which is rapidly removed by water, thus creating the sheer walls rising directly from their base. Seen two thirds of the way up the face, the Entrada sandstone is covered by a hard cap of grayish-green sandstone and siltstone of the Curtis Sandstone formation, protecting the monolith from erosion. Above the Curtis sandstone formation is the thinly-bedded, reddish-brown siltstone of the Summerville sandstone formation.
    _LPA6214-Edit-temple-of-the-sun-sunr...tif
  • Small water pockets in the sandy river bed reflect surrounding cliffs bathed in golden light at Crack Canyon of the San Rafael Reef, Utah.
    _LPA7048-reflection-gold-water-canyo...tif
  • AJ (age 10) and LB (age 8) pause to gaze at the morning light reflecting off the surrounding cliffs while hiking through Crack Canyon in Utah.
    _LPA7069-climbing-sillouette-cliff-u...tif
  • AJ ( age 8) smiles in anticipation of ice cream on a warm California day.
    P-000038-smile-girl-ice-cream.tif
  • The sun shines through the trees and reflections dance atop the Concord River as it flows through Great Meadows National Wildlife Refuge in Concord, Massachusetts.  The refuge consists of more than 3,800 acres of which roughly 85 percent is comprised of freshwater wetlands stretching along 12 miles of the Concord and Sudbury Rivers. It is a nesting, resting, and feeding habitat for wildlife, especially migratory birds, that is protected by the U.S. Fish and Wildlife Service.  Over 220 species of birds have been identified in the refuge.  The first tract of refuge land was donated by Samuel Hoar in 1944. (single fisheye exposure)
    _LPA0292-4x6-concord-river-fisheye.tif
  • Mom and Dad setting milkweed seeds free to fly upon the breeze on a perfect fall day at Great Meadows National Wildlife Refuge in Concord, Massachusetts.
    _LPA0296-Edit-sunstar-sun-milkweed.tif
  • A flock of 16 Canada geese (Branta canadensis) fly south past the sun as they begin their migration to warmer climates for the winter. During migration, Canada geese often fly in a distinctive V-shaped flight formation, at a usual altitude of 1 km (3,000 feet). The maximum flight ceiling of Canada geese is unknown, but they have been reported at 9 km (29,000 feet).<br />
<br />
(single image, no filter)
    _LPA0252-Edit-canada goose-geese-sun...tif
  • A flock of 15 Canada geese (Branta canadensis) fly south into the sun as they begin their migration to warmer climates for the winter. During migration, Canada geese often fly in a distinctive V-shaped flight formation, at a usual altitude of 1 km (3,000 feet). The maximum flight ceiling of Canada geese is unknown, but they have been reported at 9 km (29,000 feet).<br />
<br />
(single image, no filter)
    _LPA0247-Edit-2-goose-geese-sunstar-...tif
  • On August 21, 2017 the path of the first solar eclipses over the Unites States in 38 years traversed approximately 2,500 miles of the country from Newport, Oregon to McClellanville, South Carolina.  Just outside Shoshoni, Wyoming, the path passed over Boysen Reservoir.  At this location, totality lasted 2 minutes and 22 seconds, being at its maximum about 11:40 am.  With the moon blocking the solar disk during totality, red flares called solar prominences become visible at the edge of the dark disk.  The red-glowing looped material is plasma, a hot gas composed of electrically charged hydrogen and helium. These prominences look small in relation to the size of the sun, but typically extend over many thousands of kilometers with the largest on record being estimated at over 800,000 kilometres (500,000 miles).  A prominence forms over timescales of about a day and may persist for several weeks or months.<br />
<br />
During the total solar eclipse, the sun’s outer atmosphere called the corona becomes visible as it extends millions of miles into space.  The corona consists of extremely hot ionized gases which exceed 1 million degrees Kelvin – 150- to 450-times hotter than the surface of the sun.  Being over 1 million million times less dense and much hotter than the sun’s surface and the solar prominences, the corona actually produces about one-millionth as much visible light, thus becoming visible from earth typically only during a total solar eclipse. The sun’s magnetic fields bend the corona into its remarkable shapes.<br />
<br />
In this image, 10 different photographic exposures of the solar eclipse were composited to show the eclipsing moon, solar prominences and the corona.  (exposure stack of 10 images)
    total-solar-eclipse-sun-corona-squar...tif
  • On August 21, 2017 the path of the first solar eclipses over the Unites States in 38 years traversed approximately 2,500 miles of the country from Newport, Oregon to McClellanville, South Carolina.  Just outside Shoshoni, Wyoming, the path passed over Boysen Reservoir.  At this location, totality lasted 2 minutes and 22 seconds, being at its maximum about 11:40 am.  With the moon blocking the solar disk during totality, red flares called solar prominences become visible at the edge of the dark disk.  The red-glowing looped material is plasma, a hot gas composed of electrically charged hydrogen and helium. These prominences look small in relation to the size of the sun, but typically extend over many thousands of kilometers with the largest on record being estimated at over 800,000 kilometres (500,000 miles).  A prominence forms over timescales of about a day and may persist for several weeks or months.<br />
<br />
During the total solar eclipse, the sun’s outer atmosphere called the corona becomes visible as it extends millions of miles into space.  The corona consists of extremely hot ionized gases which exceed 1 million degrees Kelvin – 150- to 450-times hotter than the surface of the sun.  Being over 1 million million times less dense and much hotter than the sun’s surface and the solar prominences, the corona actually produces about one-millionth as much visible light, thus becoming visible from earth typically only during a total solar eclipse. The sun’s magnetic fields bend the corona into its remarkable shapes.<br />
<br />
In this image, 10 different photographic exposures of the solar eclipse were composited to show the eclipsing moon, solar prominences and the corona.  (exposure stack of 10 images)
    total-solar-eclipse-sun-corona.tif
  • On August 21, 2017 the path of the first solar eclipses over the Unites States in 38 years traversed approximately 2,500 miles of the country from Newport, Oregon to McClellanville, South Carolina.  Just outside Shoshoni, Wyoming, the path passed over Boysen Reservoir.  At this location, totality lasted 2 minutes and 22 seconds, being at its maximum about 11:40 am.  With the moon blocking the solar disk during totality, red flares called solar prominences become visible at the edge of the dark disk.  The red-glowing looped material is plasma, a hot gas composed of electrically charged hydrogen and helium. These prominences look small in relation to the size of the sun, but typically extend over many thousands of kilometers with the largest on record being estimated at over 800,000 kilometres (500,000 miles).  A prominence forms over timescales of about a day and may persist for several weeks or months.<br />
<br />
During the total solar eclipse, the sun’s outer atmosphere called the corona becomes visible as it extends millions of miles into space.  The corona consists of extremely hot ionized gases which exceed 1 million degrees Kelvin – 150- to 450-times hotter than the surface of the sun.  Being over 1 million million times less dense and much hotter than the sun’s surface and the solar prominences, the corona actually produces about one-millionth as much visible light, thus becoming visible from earth typically only during a total solar eclipse. The sun’s magnetic fields bend the corona into its remarkable shapes.<br />
<br />
In this image, 10 different photographic exposures of the solar eclipse were composited to show the eclipsing moon, solar prominences and the corona.  The image was then manipulated by a process called embossing where each pixel is replaced either by a highlight or a shadow, depending on light/dark boundaries on the original image.  The final image represents the rate of color change at each location of the original. This approach accentuates the pattern
    total-solar-eclipse-sun-corona-embos...tif
  • On August 21, 2017 the path of the first solar eclipses over the Unites States in 38 years traversed approximately 2,500 miles of the country from Newport, Oregon to McClellanville, South Carolina.  Just outside Shoshoni, Wyoming, the path passed over Boysen Reservoir.  At this location, totality lasted 2 minutes and 22 seconds, being at its maximum about 11:40 am.  With the moon blocking the solar disk during totality, red flares called solar prominences become visible at the edge of the dark disk.  The red-glowing looped material is plasma, a hot gas composed of electrically charged hydrogen and helium. These prominences look small in relation to the size of the sun, but typically extend over many thousands of kilometers with the largest on record being estimated at over 800,000 kilometres (500,000 miles).  A prominence forms over timescales of about a day and may persist for several weeks or months.<br />
<br />
During the total solar eclipse, the sun’s outer atmosphere called the corona becomes visible as it extends millions of miles into space.  The corona consists of extremely hot ionized gases which exceed 1 million degrees Kelvin – 150- to 450-times hotter than the surface of the sun.  Being over 1 million million times less dense and much hotter than the sun’s surface and the solar prominences, the corona actually produces about one-millionth as much visible light, thus becoming visible from earth typically only during a total solar eclipse. The sun’s magnetic fields bend the corona into its remarkable shapes.<br />
<br />
In this image, 10 different photographic exposures of the solar eclipse were composited to show the eclipsing moon, solar prominences and the corona.  The image was then manipulated by a process called embossing where each pixel is replaced either by a highlight or a shadow, depending on light/dark boundaries on the original image.  The final image represents the rate of color change at each location of the original. This approach accentuates the pattern
    total-solar-eclipse-sun-corona-embos...tif
  • On August 21, 2017 the path of the first solar eclipses over the Unites States in 38 years traversed approximately 2,500 miles of the country from Newport, Oregon to McClellanville, South Carolina.  Just outside Shoshoni, Wyoming, the path passed over Boysen Reservoir.  At this location, totality lasted 2 minutes and 22 seconds, being at its maximum about 11:40 am.  With the moon blocking the solar disk during totality, red flares called solar prominences become visible at the edge of the dark disk.  The red-glowing looped material is plasma, a hot gas composed of electrically charged hydrogen and helium. These prominences look small in relation to the size of the sun, but typically extend over many thousands of kilometers with the largest on record being estimated at over 800,000 kilometres (500,000 miles).  A prominence forms over timescales of about a day and may persist for several weeks or months.<br />
<br />
During the total solar eclipse, the sun’s outer atmosphere called the corona becomes visible as it extends millions of miles into space.  The corona consists of extremely hot ionized gases which exceed 1 million degrees Kelvin – 150- to 450-times hotter than the surface of the sun.  Being over 1 million million times less dense and much hotter than the sun’s surface and the solar prominences, the corona actually produces about one-millionth as much visible light, thus becoming visible from earth typically only during a total solar eclipse. The sun’s magnetic fields bend the corona into its remarkable shapes.<br />
<br />
In this image, 10 different photographic exposures of the solar eclipse were composited to show the eclipsing moon, solar prominences and the corona.  The image was then manipulated by a process involving radial blur subtraction and image offset overlay to accentuate the pattern of the corona. The coloration of the eclipsing moon and the solar prominences were retained in this rendition.  (exposure stack of 10 images)
    total-solar-eclipse-sun-corona-overl...tif
  • On August 21, 2017 the path of the first solar eclipses over the Unites States in 38 years traversed approximately 2,500 miles of the country from Newport, Oregon to McClellanville, South Carolina.  Just outside Shoshoni, Wyoming, the path passed over Boysen Reservoir.  At this location, totality lasted 2 minutes and 22 seconds, being at its maximum about 11:40 am.  With the moon blocking the solar disk during totality, red flares called solar prominences become visible at the edge of the dark disk.  The red-glowing looped material is plasma, a hot gas composed of electrically charged hydrogen and helium. These prominences look small in relation to the size of the sun, but typically extend over many thousands of kilometers with the largest on record being estimated at over 800,000 kilometres (500,000 miles).  A prominence forms over timescales of about a day and may persist for several weeks or months.<br />
<br />
During the total solar eclipse, the sun’s outer atmosphere called the corona becomes visible as it extends millions of miles into space.  The corona consists of extremely hot ionized gases which exceed 1 million degrees Kelvin – 150- to 450-times hotter than the surface of the sun.  Being over 1 million million times less dense and much hotter than the sun’s surface and the solar prominences, the corona actually produces about one-millionth as much visible light, thus becoming visible from earth typically only during a total solar eclipse. The sun’s magnetic fields bend the corona into its remarkable shapes.<br />
<br />
In this image, 10 different photographic exposures of the solar eclipse were composited to show the eclipsing moon, solar prominences and the corona.  The image was then manipulated by a process called embossing where each pixel is replaced either by a highlight or a shadow, depending on light/dark boundaries on the original image.  The final image represents the rate of color change at each location of the original. This approach accentuates the pattern
    total-solar-eclipse-sun-corona-solar...tif
  • On August 21, 2017 the path of the first solar eclipses over the Unites States in 38 years traversed approximately 2,500 miles of the country from Newport, Oregon to McClellanville, South Carolina.  Just outside Shoshoni, Wyoming, the path passed over Boysen Reservoir.  At this location, totality lasted 2 minutes and 22 seconds, being at its maximum about 11:40 am.  With the moon blocking the solar disk during totality, red flares called solar prominences become visible at the edge of the dark disk.  The red-glowing looped material is plasma, a hot gas composed of electrically charged hydrogen and helium. These prominences look small in relation to the size of the sun, but typically extend over many thousands of kilometers with the largest on record being estimated at over 800,000 kilometres (500,000 miles).  A prominence forms over timescales of about a day and may persist for several weeks or months.<br />
<br />
During the total solar eclipse, the sun’s outer atmosphere called the corona becomes visible as it extends millions of miles into space.  The corona consists of extremely hot ionized gases which exceed 1 million degrees Kelvin – 150- to 450-times hotter than the surface of the sun.  Being over 1 million million times less dense and much hotter than the sun’s surface and the solar prominences, the corona actually produces about one-millionth as much visible light, thus becoming visible from earth typically only during a total solar eclipse. The sun’s magnetic fields bend the corona into its remarkable shapes.<br />
<br />
In this image, 10 different photographic exposures of the solar eclipse were composited to show the eclipsing moon, solar prominences and the corona.  The image was then manipulated by a process called embossing where each pixel is replaced either by a highlight or a shadow, depending on light/dark boundaries on the original image.  The final image represents the rate of color change at each location of the original. This approach accentuates the pattern
    total-solar-eclipse-sun-corona-solar...tif
  • A grasshopper sits on a young girl's shoulder as they gaze out over Boysen Reservior near Shoshoni, Wyoming.
    _LPA0293-Edit-girl-grasshopper-wyomi...tif
  • _LPA0079-Edit-jump-girl-teton-river-...tif
  • _LPA0078-Edit-jump-girl-teton-river-...tif
  • _LPA0078-Edit-jump-girl-teton-river-...tif
  • AJ (age 10) and LB (age 8) pause to gaze at the morning light reflecting off the surrounding cliffs while hiking through Crack Canyon in Utah.
    _LPA7069-climbing-children-sillouett...tif
  • A water pocket on the canyon floor reflects the surrounding cliffs bathed in golden light at Crack Canyon of the San Rafael Reef, Utah.
    _LPA7060-gold-river-reflections-crac...tif
  • The sun shines through the trees and reflections dance atop the Concord River as it flows through Great Meadows National Wildlife Refuge in Concord, Massachusetts.  The refuge consists of more than 3,800 acres of which roughly 85 percent is comprised of freshwater wetlands stretching along 12 miles of the Concord and Sudbury Rivers. It is a nesting, resting, and feeding habitat for wildlife, especially migratory birds, that is protected by the U.S. Fish and Wildlife Service.  Over 220 species of birds have been identified in the refuge.  The first tract of refuge land was donated by Samuel Hoar in 1944. (single fisheye exposure)
    _LPA0292-concord-river-square.tif
  • The ahermatypic Orange Cup Coral (Balanophyllia elegans) extends its 2-inch-long yellow-spotted tentacles to feed at night 50 feet below the surface of the Red Sea at "The Temple", Sinai, Egypt.  Although this organism closely resembles in an anemone, it is actually a true hard coral. Corals are carnivorous animals which feed upon microscopic zooplankton by trapping them with their tentacles. Most corals possess a symbiotic relationship with a class of algal cells known as zoozanthellae and are thus termed hermatypic.  Since algal cells undergo photosynthesis, hermatypic corals can also obtain energy from sunlight. In addition, zoozanthellae reduce the concentration of carbon dioxide within the cells of the hermatypic coral and thus help precipitate calcium carbonate from seawater. Calcium carbonate is a chemical from which a corals calcareous skeleton is made. However, Balanophyllia elegans is an ahermatypic coral and does not associate with algal cells. Consequently, these corals consist of a single polyp and secrete only a simple thin skeleton. Unlike their hermatypic counterparts, ahermatypic corals may be found in all oceans of the world and at depths beyond the reach of sunlight. The white soft coral at bottom (Xenia) exhibits a slow, rhythmic opening and closing movement of unknown function.
    P-000169-orange-cup-coral-red-sea.tif
  • Fiery clouds fil the evening sky over an area of forest partially burned by the Steamboat Fire in Yosemite National Park, California.  The Steamboat fire started on August 7, 1990 and eventually destroyed 6,106 acres of woodland. Wildfires have historically been considered disasters, but it is now understood that fire is an integral component of forest life.  Naturally occurring fires thin the woodlands, increase sunlight to the forest floor, and allow for recycling of nutrients to the soil.  Thus, wildfires actually encourage the germination and regrowth of the forest plants and trees.
    Image 013-Edit-sunset-wildfire-sky-f...tif
  • A 2 inch long Dog Day or Annual Cicada (Tibicen canicularis) clings to a Day Lilly (Hemerocallis ) petal in the morning sunlight.
    _LPA4644-cicada-insect-day-lilly.tif
  • Although not a true spider, Daddy longlegs (order Opiliones) go by many names including harvestman, cellar spiders, granddaddy long-legs, carpenter spider, daddy long-legger, vibrating spider and skull spider.  Daddy longlegs are closely related to scorpions (order Scorpiones) but, because of their appearance, are often mistaken as spiders (order Araneida or Araneae). However, unlike true spiders, in which the body is divided into two distinct segments, daddy longlegs look as though they have only one segment because of a broad fusion that makes the juncture between the two segments almost indiscernible.  They are widely distributed and abundant in both temperate and tropical climates of both hemispheres.<br />
<br />
The body of a daddy longlegs is 0.6 to 23 mm (0.02 to 0.9 inch) long, although the bodies of most species are between 3 and 7 mm (0.12 and 0.28 inch). The legs can exceed 15 cm (5.9 inches) in length.  Many species of daddy longlegs are omnivorous, feeding on small insects, mites, spiders, snails, and vegetable matter.  Daddy longlegs typically have two eyes located on a central knob on the front of the body although certain types lack eyes. Eggs are laid in the soil in autumn and hatch with the warmth of spring. Many species of daddy longlegs live less than one year, although some may survive for several years.<br />
<br />
This individual was photographed on a screen door retroilluminated by the early morning sunlight where over 100 daddy longlegs had congregated to feed on small insects attracted to a nearby light left on overnight.
    _1LA9448-Edit-daddy-longlegs-spider-...tif
  • Fiery clouds fil the evening sky over an area of forest partially burned by the Steamboat Fire in Yosemite National Park, California.  The Steamboat fire started on August 7, 1990 and eventually destroyed 6,106 acres of woodland. Wildfires have historically been considered disasters, but it is now understood that fire is an integral component of forest life.  Naturally occurring fires thin the woodlands, increase sunlight to the forest floor, and allow for recycling of nutrients to the soil.  Thus, wildfires actually encourage the germination and regrowth of the forest plants and trees.
    Image 013-Edit-sunset-wildfire-sky-f...tif
  • Clouds resembling the flames of a raging wildfire light the evening sky over an area of forest partially burned by the Steamboat Fire in Yosemite National Park, California.  <br />
The Steamboat fire started on August 7, 1990 and eventually destroyed 6,106 acres of woodland. Wildfires have historically been considered disasters, but it is now understood that fire is an integral component of forest life.  Naturally occurring fires thin the woodlands, increase sunlight to the forest floor, and allow for recycling of nutrients to the soil.  Thus, wildfires actually encourage the germination and regrowth of the forest plants and trees.
    Scan-101211-0003-Edit-sunset-wildfir...tif
  • Clouds resembling the flames of a raging wildfire light the evening sky over an area of forest partially burned by the Steamboat Fire in Yosemite National Park, California.  <br />
The Steamboat fire started on August 7, 1990 and eventually destroyed 6,106 acres of woodland. Wildfires have historically been considered disasters, but it is now understood that fire is an integral component of forest life.  Naturally occurring fires thin the woodlands, increase sunlight to the forest floor, and allow for recycling of nutrients to the soil.  Thus, wildfires actually encourage the germination and regrowth of the forest plants and trees.
    Scan-101211-0003-Edit-sunset-wildfir...tif
  • A new moon rises at sunset near an old tree burned during the Steamboat Fire, in Yosemite National Park, California.  The Steamboat fire destroyed 6,106 acres of woodland. Wildfires have historically been considered disasters, but it is now understood that fire is an integral component of forest life.  Naturally occurring fires thin the woodlands, increase sunlight to the forest floor, and allow for recycling of nutrients to the soil.  Thus, wildfires actually encourage the germination and regrowth of the forest plants and trees. Indeed, for over 4,000 years, the American Indians used fire in this area to cultivate the landscape.
    Scan-101211-0014-Edit-sunset-moon-tr...tif
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