Sunrise at Cocoa Beach: A Symphony of Colors on the Space Coast

Experience the breathtaking sunrise at Cocoa Beach, where the sky and sea blend in a symphony of colors. Discover the tranquility and beauty that awaits as the day dawns on Florida’s stunning Space Coast.

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Cocoa Beach, nestled in Brevard County, Florida, is renowned for its pristine sandy shores and the rhythmic lullaby of the Atlantic Ocean. It’s a place where the day often begins with an awe-inspiring sunrise. On the Space Coast, the first light of day is a daily masterpiece, a silent symphony of colors that paints the sky and reflects off the water.

As dawn approaches, the eastern horizon begins to glow with a soft, pre-dawn light. This quiet time, when the world is still asleep, offers a unique tranquility. The beach, usually bustling with surfers, sunbathers, and families, is calm and serene. The sand, cool underfoot, stretches out like a vast canvas, waiting for the sun to begin its artwork.

The first hues of sunrise start as a gentle blush, a hint of pink that softly caresses the sky. As the moments pass, this blush deepens into shades of orange and red, reminiscent of a painter’s palette. The ocean mirrors these colors, creating a breathtaking scene where sky and sea blend into one continuous expanse. It’s a moment that feels almost sacred, as if nature itself is preparing for a grand reveal.

The sun finally peeks above the horizon, a fiery orb that illuminates the world in golden light. This is the crescendo of the sunrise, a moment that seems to hold the breath of the world. The rays of light stretch out across the water, casting a shimmering path that invites the eyes to follow. It’s a path that feels both real and ethereal, leading not just across the sea, but into a day full of possibilities.

As the sun rises higher, the colors in the sky shift and change. The deep reds and oranges give way to softer yellows and then to the clear, bright light of morning. The ocean, too, transforms, taking on a deeper blue as the sunlight penetrates its depths. The waves, which had been gentle ripples in the pre-dawn light, now dance and sparkle, as if celebrating the arrival of the new day.

For those fortunate enough to witness it, a sunrise at Cocoa Beach engages all the senses. The cool breeze carries the fresh scent of saltwater, a reminder of the ocean’s vastness and power. The sound of the waves, steady and rhythmic, provides a soothing background score, while the occasional cry of a seabird adds a touch of the wild to the scene.

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There is a sense of community among the early risers who gather to watch the sunrise. Strangers often share nods and smiles, united by the shared experience of witnessing something so beautiful and ephemeral. It’s a reminder that, no matter our differences, moments of natural beauty can bring people together, fostering a sense of connection and shared humanity.

Cocoa Beach, known for its proximity to the Kennedy Space Center and its surf culture, offers much more than meets the eye. The sunrise is a daily reminder of the simple yet profound beauty of nature, a beauty that exists beyond the man-made attractions and the hustle and bustle of everyday life. It’s a call to pause, reflect, and appreciate the world around us.

In a place where rockets soar into the sky, touching the very edge of space, the sunrise at Cocoa Beach brings us back to Earth, grounding us in the timeless rhythm of the natural world. It’s a moment of peace and renewal, a gift from the universe to start the day with a heart full of wonder and gratitude.

So, whether you’re a local or a visitor, taking the time to watch the sunrise at Cocoa Beach is an experience not to be missed. It’s a chance to witness the world waking up, to feel a part of something larger than oneself, and to start the day with a renewed sense of awe and possibility.

Copyright 2024 Michael Stephen Wills All Rights Reserved

Newgrange IX

Discover the mysteries of the Newgrange monument’s Entrance Stone, a showcase of exquisite Neolithic rock art. Explore spirals, lozenges, and geometric designs that define European megalithic art and delve into their potential meanings and cultural significance. Join me in uncovering the secrets of this ancient Irish wonder.

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Juniper Sunrise

crack of dawn

In this post we start the day of my posting “Family Trek, July 19, 2008, when, well before the sun rose at 6:23 am Mountain Daylight Time (the Navajo Reservation observes daylight savings, the rest of Arizona does not), Pam and I were at the Spider Rock Overlook.

Most visitors to the canyon make use of a system of roads and parking lots next to strategic views.  There is the White House Overlook we visited our first day, July 18, to hike from the trailhead into the canyon.  There are also, on the south side of the canyon:

  • Tsegi Overlook, taken from a Navajo word that translates directly to “between the rocks” and usually refers to a deep canyon with steep cliffs.
  • Junction Overlook above the point where Canyon Del Muerto (see my posting “Sun and Shade, Canyon Del Muerto”, and Canyon De Chelly intersect.  There is an Anasazi ruin in the south-facing cliff across the canyon.
  • Sliding House Overlook, another Anasazi run across the canyon.
  • Face Rock Overlook, to view the eponymous formation.
  • Spider Rock Overlook, the most stunning rock formation. 
Sunrise Canyon De Chelly
Looking east from the Spider Rock overlook, Canyon De Chelly.

While getting ready I scoped out the location for interesting visual tropes.  Utah Junipers are exceptionally hardy shrubs, stressed individual plants grow into compelling forms shaped by hardship.  As the sun rose, this specimen emerged from the gloom and caught the first sun rays.

Juniper Sunrise
A distressed Utah Juniper on the edge of Canyon De Chelly overlooking Needle Rock a few moments after sunrise.

Enjoy!!

Click for the first posting of this series, “Portrait of a Navajo Guide.”
 

August Afternoon Fillmore Glen

Sunlight in Fillmore Glen Gorge

Augusts are typically dry in the Finger Lakes, drawing down creeks to a thin flow perfect for photography. I took the opportunity of Sunday leisure time to climb into Fillmore Glen gorge, set up the tripod and shoot.

The sun broke through the clouds for this shot.

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Copyright 2021 Michael Stephen Wills All Rights Reserved

Cocoa Beach Kite Skating

Kiteskaters and Cruise Ships

In the early morning hours of Sunday, September 10, 2017 as Hurricane Irma approached the Florida Keys, I cannot sleep, worried about family members north of Miami and in Daytona Beach. To pass the time, I returned to the golden hours of March 4, 2017 evening.  On vacation, Pam and I walked Cocoa Beach starting from Lori Wilson Park, headed north.

The light was perfect when I decided to switch to Raw-Jpeg mode, feeling the extra space was worth it.  I don’t know why I don’t shoot Raw 100% of the time, as always, in retrospect, I regret using jpeg only. The camera was the Sony Alpha 700 dslr with a DT 18-200mm f3.5-6.3 lens purchased 2008 after an expedition to the Superstition Wilderness.

After capturing a wedding photo shoot and surfers there was this set of two Kite Skaters going at least 20 miles an hour. The Sony Alpha was quick enough to capture some of the action in raw mode, I am not satisfied with the sharpness of the images as the lens was not fast enough.

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Overview, Approaching Kite skater

We had never watched kite skaters before and were prepared to understand the vision from watching distant kite surfers out beyond the breakers. North winds are the best for any type of kiting on Cocoa Beach and, that day, the wind was northeast. These riders zipped by in less than a minute. The sport is low key, it does not exist on Wikipedia. Image that. These two are having a fantastic time and stayed upright, going on and on and on down the miles long beach.

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Sailskater Dreamview with Cruise Ship

1990 KiteSkate pioneers on the USA east coast experimented with four-line controllable parafoil kites powering in-line skates for exciting rides on asphalt surfaces.

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Her partner approaches

The name “Wheels of Doom” suggest the danger of going this fast over a hard, rough surface.

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He makes it look easy

These Cocoa Beach riders are outfitted for speed and safety: pads, helmets.

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He maneuvers kite overhead to slow down.

Barefeet?? Unprotected skin? They must know how to dress, though maybe not.  He has never fallen?

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Full speed ahead with the kite positioned forward.

The beach within the tide line is solid, the pebbles, broken shells and such unforgiving as asphalt.

Click this link for another Cocoa Beach post
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Copyright 2022 Michael Stephen Wills All Rights Reserved

McMath-Pierce Solar Telescope – 3

Adaptive optics

These views within the McMath–Pierce solar telescope enclosure were captured during a guided tour of the instrument, April 20, 2005. By way of orientation, the observation room we visited is near the location labeled “4” on the model of the following photograph or the “Observation Room” of the drawing.

We learned each of the sets of mirrors is considered a separate telescope. The first step in designing the new solar telescope was to determine the optimal image scale. Working on the spectra of the solar granules, on the physical structure of the sunspots and their associated magnetic fields, requires a considerable image size. Past experience has shown that the optimal image of the sun should be approximately 0.91 meters. The highlight of our visit to the Main Observation room was meeting with the technician operating the recently developed low-cost adaptive optics system.

Tip-tilt correction and low order wavefront correction is available with a number of portable optical benches.  These are primarily used with the Main spectrograph and the Solar Stellar spectrograph on the Main telescope, but due to their compact mounting they could be used with other telescopes and instruments in the facility.

This configuration uses a rapidly deformable mirror to correct distortions introduced by the turbulent atmosphere. Using sensors to measure the degree of image distortion, the adaptive optics system adjusts the shape of the mirror accordingly and converts a blurred image into a clear one. The following image demonstrates the correction. “Low-cost” = $25,000 in 2003 US dollars. Under references is a link to a full description of the device by the creator.

A main area of ​​study in the observatory is the structure of sunspots, which are relatively cold, dark spots on the surface of the Sun created by intense magnetic activity.

Some of the most important discoveries made at McMath-Pierce include the detection of water vapor in the Sun, the measurement of kilogauss magnetic fields (thousands of times stronger than those on Earth) outside sunspots and the detection of a natural maser (like a laser, but with a microwave instead of visible light) in the Martian atmosphere.

Over the years and technological advances, the National Solar Observatory has moved its headquarters from Tucson to Boulder, Colorado. The organization abandoned its solar telescopes at Kitt Peak and in New Mexico for a larger instrument in Hawaii, the Daniel K. Inouye Solar Telescope on the island of Maui, which began operating in 1919.

References:
Wikipedia “McMath–Pierce solar telescope”

“Low Cost Adaptive Solar Optics” by Christopoher Kellar

Insights into the architectural design.

National Solar Observatory website..

Copyright 2022 Michael Stephen Wills All Rights Reserved

McMath-Pierce Solar Telescope – 2

The Mirrors

These views within the McMath–Pierce solar telescope enclosure were captured during a guided tour of the instrument, April 20, 2005. By way of orientation, think of yourself at the location labeled “4” on this model. This is the only large telescope where humans can view the interior and visually experience the light paths “bouncing” between the mirrors.

McMath–Pierce solar telescope has three heliostats mounted on a 110-foot tower adjacent to a slanted enclosure. The 2.03-meter heliostat feeds a 1.61-meter primary mirror, there are 1.07-meter and 0.91-meter primary mirrors fed by a pair of 0.81-meter heliostats. Here we are inside the slanted enclosure, looking up the shaft to the tower mounted heliostats, readily identified as the three circles, the largest at center (3.51 feet in diameter). The smaller (2.66 feet) heliostats named “East” (on left) and “West.”

Built in 1962, the building was designed by American architect Myron Goldsmith and Bangladeshi-American structural engineer Fazlur Rahman Khan. It was the largest solar telescope and the largest unobstructed aperture telescope in the world. It is named after the astronomers Robert Raynolds McMath and Keith Pierce. Painted white to reflect sunlight to reduce heat accumulation, the enclosure is water cooled to prevent convection currents through the column of air within the slanted enclosure, keeping the air as still as possible along the light path between the mirrors.

In the three photographs following, we face the underground portion of the slanted shaft and (what looks to be) the 0.91 meter (2.99 feet) primary concave mirror. I say that because in some of the photographs a beam of light, to the left of the mirror, can be seen travelling further underground, presumably to the largest primary mirror. As there is only one such light beam, I conclude the west heliostat is inactive.

Here we looking up the slanted enclosure. Look carefully at the first photograph, below, to see reflections on the glass partition. The observation platform was separated from the light paths to maintain the stillness of the air column. The two mirrors of the first photograph are the third mirror, reflecting concentrated sunlight from the 0.91 and 1.61-meter primary mirrors into the observatory rooms. The mirror for the 1.07-meter primary is out of sight in foreground, I believe this set of three mirrors (West heliostats, primary and third) was out of service.

The second photograph, on right, is a close up of the third mirror for the largest primary. A foreshortened, perfectly round light disk is clearly visible.

Here we are inside the slanted enclosure, facing the underground portion of the slanted shaft and (what looks to be) the 0.91-meter primary concave mirror. In the lower right corner is the reverse side of the third mirror for the largest primary mirror, the 1.61-meter.

Reference: Wikipedia “McMath–Pierce solar telescope”
Copyright 2022 Michael Stephen Wills All Rights Reserved

Oceans’ Eons

Tranquil Morning Surf with Peaceful Music for Tranquility, Relaxation, Meditation.

For full peace and tranquility view on a large screen “smart” television.

Eight minutes of ocean waves and gentle music in 4K UHD.

Anatomy of Dawn

Subcategories of Twilight and more

Use your pinky finger to apprehend the sky dome. Imagine yourself at sea, out of sight of land, on a calm day. Keeping your arm extended, place your pinky-tip on the horizon due east, raise your arm directly overhead. The average sized pinky-tip will have spanned 90 of its lengths. The distance measured from the horizon to directly overhead, the zenith, is 90 degrees of sky dome, about one pinky-width per degree, one-fourth of the entire 360 degrees of sky around your spot on the globe.

The apparent width of the sun disk from earth covers 1/2 degree of sky dome. The disk center point moves 15 degrees per hour (360/24 = 15). Using these facts to estimate time to sunset is relatively straightforward. Estimating time to dawn from the sky is more difficult. This graphic, “Twilight-dawn subcategories,” is a way to grasping what happens. Your position on the earth globe affects the experience. For example, at northern latitudes above 60°34′ summer nights never become darker than civil twilight because the sun’s midpoint never drops lower than 6 degrees below the horizon. Civil twilight lasts all night long summer times in parts of Sweden and Finland.

The date-time stamp on the first photograph of this series is 6:46:23 am, Cocoa Beach sunrise for February 1st was 7:09:40, 00:23:17, 23.283 minutes in decimal notation, later. This duration divided by 60 minutes in an hour and multiplied by the sun’s apparent velocity across the sky (15 degrees per hour) and minus the .25 degree between sun’s center and disk edge, gives the sun’s center as 5.57 degrees below the horizon: this is a photograph of the sky a minute or so after the sun passed civil dawn into civil twilight. I am not more exact because this calculation does not account the deviation of the sun path from due east at this latitude, lengthening civil twilight duration by almost a minute.

The following photograph is time-stamped 7:05:06, 4.567 minutes until sunrise, sun center is just below the horizon, setting the dark clouds of the previous photograph fleetingly on fire.

Sunrise has passed in the following photographs, obscured by clouds and making for a great light show. Enjoy!!

References

“Dawn” Wikipedia page, the graphic “Twilight-dawn subcategories,” and the descriptions of subcategories came from this page.