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Sweet Dream

  • By Tom Serio Photography By Billy Black
  • Updated: July 3, 2015

voyager 860

How do you pay homage to your favorite drink? Well, you could name your yacht after it.

That’s what the owners of the [Outer Reef][] 860 CPMY (cockpit motoryacht) did. Ti Punch takes her name from an island favorite flavored-rum cocktail. The word ti (pronounced tee) in Creole means petite, or small.

Well, there’s nothing small about the 860, be it the size of the yacht or the imagination of her owners.

Outwardly, the 860 commands a second look. Broad shoulders in the form of generous bow flare blend aft along the faux-planked hull and a high freeboard. The exterior is accented by a Kingston-gray Awlgrip stripe that runs along the top sheer line of the hull, hinting at the contemporary color scheme found within her interior spaces.

That impressive interior starts off with a voluminous salon. There’s a semicircular bar with granite countertop, glass stowage and fridge in the port aft corner plus an entertainment center with a flat-screen TV to starboard — a great setup for having afternoon cocktails and then stepping out to watch the sun set. An L-shaped sofa to port and a ­starboard-side love seat make for a nice after-dinner conversation spot. A coffee table, end tables, an ottoman and bar stools offer more seating, and there’s still plenty of room for guests to stand and mingle. A mirrored-ceiling inlay adds to the open feel of the room.

The owners really put their stamp on Ti Punch , including the use of high-gloss American walnut cabinetry and varying shades of blue and gray (separately and in combination) for her interior color theme. Gray is not my favorite color, as I often associate it with naval vessels, but it is used throughout the galley and forward dining/helm area, and I have to admit that I liked it. It may come across as a bit utilitarian, but it’s easy on the eyes, defines the space between the salon and forward areas, allows for ample light to brighten the interior spaces and works well with the wood and fabrics.

voyager 860

In the galley, all of the upper and lower cabinets are finished in a gray veneer, which complements the stainless-steel appliances, including the Bosch dishwasher, KitchenAid trash compactor, Bosch full-size oven and four-burner cooktop, and LG microwave. Across the way is an LG side-by-side refrigerator/freezer and six-drawer pantry finished in a satin-­walnut veneer. The granite countertops are gray-infused, highlighted with flecks of blue. Chrome push-button latches on drawers and doors are a classy touch.

Forward of the galley are the dinette and helm. An L-shaped settee to port lets guests sit for a meal or take in the view underway. The dinette table is finished like the counters, gray with blue highlights, and works with the varying light-and-dark-gray-patterned cushions.

A wall raises and lowers hydraulically behind the dinette seat, separating the salon and galley spaces from the dinette and helm. Close it from the lower station for privacy or during night cruising, or keep it open for stem-to-stern visibility. A pocket door closes off the walkway.

Five large windows allow for easy viewing from the lower helm. Wrapped in gray vinyl, the helm can accommodate almost any electronics suite an owner desires. Ti Punch has three Masters display monitors running Furuno software, ABT-TRAC bow and stern thrusters and Caterpillar engine monitors. Twin Stidd helm chairs ensure the pilot and co-pilot are kept comfortable on long passages.

voyager 860

Access to the staterooms is via a stairway to starboard of the helm. There’s nothing small about the full-beam master, which has a king-size berth (7 inches of cushy mattress), two cedar lockers, six cabinets, two vanities, four portlights, nine LED overhead lights, twin sinks in the head and one large shower stall. Gray vinyl padding on some walls accents the varnished beachwood finish.

Forward is a VIP stateroom featuring a tapered queen berth, twin cedar lockers and an en suite head with shower. A guest stateroom aft and to port has a twin berth, and the fourth space to starboard has over-under bunks, which is a great spot for the kids.

Like the 860’s salon, her upper deck is expansive and the helm area is the gathering point. It’s a full-beam setup with twin Stidd helm chairs, port and starboard L-shaped settees with tables, full controls for the captain and a hardtop secured like the Rock of Gibraltar. Ti Punch’s owners opted for a full enclosure, which converts this spot into an all-weather area with an ­air-conditioning/reverse-heat system.

Behind the aft curtains are stowage cabinets and a food-prep station with sink, grill and fridge. This is the place for afternoon lunch in the Bahamas. Swing gates section off the after end of the deck that houses the davit, Sea-Doo and inflatable tender. The gates are a great safety feature, especially if there are little ones or pets roaming the deck.

The owners powered this long-range, 95-ton, horizon-chasing yacht with twin 1,150-horsepower Caterpillar C18 ACERT diesels, which are surrounded by sturdy grab rails. All servicing points are easily accessible, as are the Racor filters, sea chests and fuel-management valves. The engine room’s solid floor panels lift effortlessly for access to the bilge.

Outer Reef must follow the adage that “a happy crew means a happy yacht,” because the crew quarters just abaft the engine room are pretty stylish. A settee with table, fridge, microwave, cooktop and TV fit out the galley, with berths for two to three people and a head with shower stall.

Back at sea level there’s a fighting-chair-equipped lower cockpit because the owners are into fishing, diving and other on-the-water activities. Ti Punch also has a swim platform that’s more like a mini beach, a great spot to catch some rays in a secluded cove.

Outer Reef sales representative Mike Schlichtig said these owners’ cruising plans have changed from those of their previous yacht, an 82-footer. Desiring to spend more time fishing and scuba diving, and to have a full-time captain, the owners wanted a “setup for getting out of Dodge.” That’s not uncommon, with boater demographics changing when it comes to yachts like those from Outer Reef. “Clients are now in their 50s, where seven years ago they were 65 to 70 years old,” commented Schlichtig. He added that buyers are looking for a yacht that offers the feeling of a home environment, but with more range.

Secure handling and maneuverability were evident on the 860 as we navigated the constricted New River in Fort Lauderdale, Florida, and then hit the open water. With the ABT-TRAC stabilizers energized and the pointy end effortlessly knocking down a 3-foot white-capped chop, there was nary a bump, grind or groan to be had. Outer Reef’s yachts have a reputation for competently handling open seas, and the 860 is certainly up to the task of maintaining that reputation.

If exploring the sea is your goal, the Outer Reef 860 CPMY deserves your attention. She’s built for going long, is finished to a high standard, and can be tailored to just about any owner’s desire. You can even name her after your favorite cocktail, but sorry … Ti Punch is already taken.

Built For The Sea

The Outer Reef 860 CPMY comes from three molds and features a hand-laid, solid fiberglass hull bottom with PVC coring used above the waterline for added strength without added weight. Her hull is finished in a white gelcoat, while a vinylester barrier prevents osmosis and blistering. Full-length engine stringers give her structure serious backbone. There is a full keel that extends below the propellers to protect the 860’s running gear in the event of an accidental grounding. Outer Reef’s patented Quiet Roll spray-rail system aims to deflect water in big seas and reduce hull noise, making all passages peaceful ones.

voyager 860

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NASA solar sail to be Siriusly visible in orbit from Earth

Look out for a new star next week.

NASA is to send a solar sail demonstrator into orbit next week, and there is a good chance that the sail, measuring 860 square feet (80 square meters), will be visible from Earth.

NASA Advanced Composite Solar Sail System unfurled on the floor with engineers working on it

Advanced Composite Solar Sail System (click to enlarge) Pic: NASA

The primary goal of the Advanced Composite Solar Sail System (ACS3) mission is to demonstrate the deployment of a new composite boom made from flexible polymer and carbon fiber materials.

Despite being stiffer than previous designs, the tube-shaped boom can be squashed flat and rolled like a tape measure, according to Keats Wilkie, the mission's principal investigator at NASA's Langley Research Center in Hampton, Virginia.

Wilkie said: "Booms have tended to be either heavy and metallic or made of lightweight composite with a bulky design – neither of which work well for today's small spacecraft."

However, this approach means that the sail's booms can be reduced to a small package "while offering all the advantages of composite materials, like less bending and flexing during temperature changes."

Handy, because the 12U CubeSat built by NanoAvionics is hardly a behemoth.

voyager 860

Assuming the boom works well, the team hopes to test the sail's performance by angling it to adjust the spacecraft's orbit.

The ACS3 is a secondary payload on Rocket Lab's "Beginning Of The Swarm" mission, due to be launched from the company's Launch Complex 1 on April 24. The primary payload on the mission is NEONSAT-1, an Earth observation satellite with a high-resolution camera designed to monitor natural disasters on the Korean Peninsula. Funded by the South Korean government, NEONSAT-1 is due to be joined by other NEONSAT satellites in 2026 and 2027 to build out a constellation.

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ACS3 will operate in a Sun-synchronous orbit, approximately 600 miles (1,000 kilometers) above the Earth. Once in orbit, it will unroll its composite booms, and then, approximately 25 minutes later, the solar sail will deploy. Cameras onboard the spacecraft will monitor the deployment.

According to NASA: "With its large sail, the spacecraft may be visible from Earth if the lighting conditions are just right. Once fully expanded and at the proper orientation, the sail's reflective material will be as bright as Sirius, the brightest star in the night sky."

Well, it's large compared to the NanoAvionics spacecraft bus. At roughly six US parking spots, the sail would be dwarfed by the ISS solar array wings, but should all go well, larger-scale models could be designed and launched.

According to NASA: "This boom design could potentially support future solar sails as large as 5,400 square feet (500 square meters), about the size of a basketball court, and technology resulting from the mission's success could support sails of up to 21,500 square feet (2,000 square meters) – about half a soccer field."

"Seven meters of the deployable booms can roll up into a shape that fits in your hand," said Alan Rhodes, the mission's lead systems engineer at NASA's Ames Research Center.

"The hope is that the new technologies verified on this spacecraft will inspire others to use them in ways we haven’t even considered." ®

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The most distant human-made object

Computer-generated view of a Voyager spacecraft far from the Sun.

No spacecraft has gone farther than NASA's Voyager 1. Launched in 1977 to fly by Jupiter and Saturn, Voyager 1 crossed into interstellar space in August 2012 and continues to collect data.

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Voyager 1 has been exploring our solar system for more than 45 years. The probe is now in interstellar space, the region outside the heliopause, or the bubble of energetic particles and magnetic fields from the Sun.

  • Voyager 1 was the first spacecraft to cross the heliosphere, the boundary where the influences outside our solar system are stronger than those from our Sun.
  • Voyager 1 is the first human-made object to venture into interstellar space.
  • Voyager 1 discovered a thin ring around Jupiter and two new Jovian moons: Thebe and Metis.
  • At Saturn, Voyager 1 found five new moons and a new ring called the G-ring.

In Depth: Voyager 1

Voyager 1 was launched after Voyager 2, but because of a faster route, it exited the asteroid belt earlier than its twin, having overtaken Voyager 2 on Dec. 15, 1977.

Voyager 1 at Jupiter

Voyager 1 began its Jovian imaging mission in April 1978 at a range of 165 million miles (265 million km) from the planet. Images sent back by January the following year indicated that Jupiter’s atmosphere was more turbulent than during the Pioneer flybys in 1973–1974.

Beginning on January 30, Voyager 1 took a picture every 96 seconds for a span of 100 hours to generate a color timelapse movie to depict 10 rotations of Jupiter. On Feb. 10, 1979, the spacecraft crossed into the Jovian moon system and by early March, it had already discovered a thin (less than 30 kilometers thick) ring circling Jupiter.

Voyager 1’s closest encounter with Jupiter was at 12:05 UT on March 5, 1979 at a range of about 174,000 miles (280,000 km). It encountered several of Jupiter’s Moons, including Amalthea, Io, Europa, Ganymede, and Callisto, returning spectacular photos of their terrain, opening up completely new worlds for planetary scientists.

The most interesting find was on Io, where images showed a bizarre yellow, orange, and brown world with at least eight active volcanoes spewing material into space, making it one of the most (if not the most) geologically active planetary body in the solar system. The presence of active volcanoes suggested that the sulfur and oxygen in Jovian space may be a result of the volcanic plumes from Io which are rich in sulfur dioxide. The spacecraft also discovered two new moons, Thebe and Metis.

Voyager 1 at Saturn

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Following the Jupiter encounter, Voyager 1 completed an initial course correction on April 9, 1979 in preparation for its meeting with Saturn. A second correction on Oct. 10, 1979 ensured that the spacecraft would not hit Saturn’s moon Titan.

Its flyby of the Saturn system in November 1979 was as spectacular as its previous encounter. Voyager 1 found five new moons, a ring system consisting of thousands of bands, wedge-shaped transient clouds of tiny particles in the B ring that scientists called “spokes,” a new ring (the “G-ring”), and “shepherding” satellites on either side of the F-ring—satellites that keep the rings well-defined.

During its flyby, the spacecraft photographed Saturn’s moons Titan, Mimas, Enceladus, Tethys, Dione, and Rhea. Based on incoming data, all the moons appeared to be composed largely of water ice. Perhaps the most interesting target was Titan, which Voyager 1 passed at 05:41 UT on November 12 at a range of 2,500 miles (4,000 km). Images showed a thick atmosphere that completely hid the surface. The spacecraft found that the moon’s atmosphere was composed of 90% nitrogen. Pressure ad temperature at the surface was 1.6 atmospheres and 356 °F (–180°C), respectively.

Atmospheric data suggested that Titan might be the first body in the solar system (apart from Earth) where liquid might exist on the surface. In addition, the presence of nitrogen, methane, and more complex hydrocarbons indicated that prebiotic chemical reactions might be possible on Titan.

Voyager 1’s closest approach to Saturn was at 23:46 UT on 12 Nov. 12, 1980 at a range of 78,000 miles(126,000 km).

Voyager 1’s ‘Family Portrait’ Image

Following the encounter with Saturn, Voyager 1 headed on a trajectory escaping the solar system at a speed of about 3.5 AU per year, 35° out of the ecliptic plane to the north, in the general direction of the Sun’s motion relative to nearby stars. Because of the specific requirements for the Titan flyby, the spacecraft was not directed to Uranus and Neptune.

The final images taken by the Voyagers comprised a mosaic of 64 images taken by Voyager 1 on Feb. 14, 1990 at a distance of 40 AU of the Sun and all the planets of the solar system (although Mercury and Mars did not appear, the former because it was too close to the Sun and the latter because Mars was on the same side of the Sun as Voyager 1 so only its dark side faced the cameras).

This was the so-called “pale blue dot” image made famous by Cornell University professor and Voyager science team member Carl Sagan (1934-1996). These were the last of a total of 67,000 images taken by the two spacecraft.

Voyager 1’s Interstellar Mission

All the planetary encounters finally over in 1989, the missions of Voyager 1 and 2 were declared part of the Voyager Interstellar Mission (VIM), which officially began on Jan. 1, 1990.

The goal was to extend NASA’s exploration of the solar system beyond the neighborhood of the outer planets to the outer limits of the Sun’s sphere of influence, and “possibly beyond.” Specific goals include collecting data on the transition between the heliosphere, the region of space dominated by the Sun’s magnetic field and solar field, and the interstellar medium.

On Feb. 17, 1998, Voyager 1 became the most distant human-made object in existence when, at a distance of 69.4 AU from the Sun when it “overtook” Pioneer 10.

On Dec. 16, 2004, Voyager scientists announced that Voyager 1 had reported high values for the intensity for the magnetic field at a distance of 94 AU, indicating that it had reached the termination shock and had now entered the heliosheath.

The spacecraft finally exited the heliosphere and began measuring the interstellar environment on Aug. 25, 2012, the first spacecraft to do so.

On Sept. 5, 2017, NASA marked the 40th anniversary of its launch, as it continues to communicate with NASA’s Deep Space Network and send data back from four still-functioning instruments—the cosmic ray telescope, the low-energy charged particles experiment, the magnetometer, and the plasma waves experiment.

The Golden Record

The Titan/Centaur-6 launch vehicle was moved to Launch Complex 41 at NASA's Kennedy Space Center in Florida to complete checkout procedures in preparation for launch.

Each of the Voyagers contain a “message,” prepared by a team headed by Carl Sagan, in the form of a 12-inch (30 cm) diameter gold-plated copper disc for potential extraterrestrials who might find the spacecraft. Like the plaques on Pioneers 10 and 11, the record has inscribed symbols to show the location of Earth relative to several pulsars.

The records also contain instructions to play them using a cartridge and a needle, much like a vinyl record player. The audio on the disc includes greetings in 55 languages, 35 sounds from life on Earth (such as whale songs, laughter, etc.), 90 minutes of generally Western music including everything from Mozart and Bach to Chuck Berry and Blind Willie Johnson. It also includes 115 images of life on Earth and recorded greetings from then U.S. President Jimmy Carter (1924– ) and then-UN Secretary-General Kurt Waldheim (1918–2007).

By January 2024, Voyager 1 was about 136 AU (15 billion miles, or 20 billion kilometers) from Earth, the farthest object created by humans, and moving at a velocity of about 38,000 mph (17.0 kilometers/second) relative to the Sun.

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The VOYAGE Power Catamaran is an outstanding one of a kind yacht, built and designed for extreme comfort and luxury yachting. This stunning, spacious motor yacht cruises at 15 knots, providing a comfortable ride to your next charming destination, and offers a panoramic upper deck lounge that can be fully enclosed for a quick squall, or opened up to the warm sea breeze.

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The VOYAGE 650 Power Cat offers six, deluxe King size en-suite cabins for up to 12 guests.

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Poly Voyager Free 60 User Manual

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  • Load Software
  • Update Your Poly Device
  • Replace Eartips
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  • Power On/Off Your Earbud System
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  • Connect and Pair
  • Pair to Mobile Device
  • Adjust the Volume
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  • Voice Assistant (Smartphone Feature)
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  • Make/Take/End Calls
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  • Page 1 Voyager Free 60 True Wireless Earbuds with Basic Charge Case User Guide...

Page 2: Table Of Contents

Page 3: your earbud system, page 4: earbud button controls, page 5: earbud swipe sensor controls, page 6: load software, page 7: fit, page 8: charge, page 9: quick charge, page 10: power, page 11: connect and pair, page 12: the basics, page 13: anc and transparency mode, page 14: make/take/end calls, page 15: more features, page 16: connect new earbud, page 17: troubleshooting, page 18: general, page 19: safety warnings.

  • Page 20 • RECYCLING: The product battery must be recycled or disposed of properly. Contact your local recycling center for battery removal and proper disposal. • Use only the charger supplied by Poly to charge the product and follow the charging instructions provided. Alternatively, if your headset is designed to be charged with your cell phone charger, use only cell phone chargers approved and provided by your cell phone manufacturer.

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Toroidally focused ultrasonic flaw detectors

  • Acoustic Methods
  • Published: 28 July 2011
  • Volume 47 , pages 308–310, ( 2011 )

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  • A. V. Shevelev 1 &
  • Zh. V. Zatsepilova 2  

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New-type toroidally focused ultrasonic flaw detectors, whose application provides an appreciable increase in the flaw detection rate with retention of high sensitivity to flaws, are considered. The construction of a flaw detector is presented, the sizes of a gauge for the formation of the toroidal surface of a lens are given, and the technology of the manufacturing of a toroidal lens is described.

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Influence of Pitch of Ultrasonic Antenna Array on Efficiency of Extraction of a Signal from Structural Noise in Flaw Detection

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Ermolov, I.N., Aleshin, N.P., and Potapov, A.I., Nerazrushayushchii control’ (Nondestructive Testing), book 2: Akusticheskie metody kontrolya (Acoustic Testing), Moscow: Vysshaya shkola, 1991.

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Nerazrushayushchii kontrol’ (Spravochnik) (Nondestructive Testing: Handbook), Klyuev, V.V., Ed., vol. 3: Ul’trazvukovoi kontrol’ (Ultrasonic Testing), Moscow: Mashinostroenie, 2006.

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Elektrostal Polytechnic Institute, Branch of the National University of Science and Technology “MISIS”, ul. Pervomaiskaya 7, Elektrostal, Moscow oblast, 144000, Russia

A. V. Shevelev

Elektrostal Heavy Engineering Plant JSC, ul. Krasnaya 19, Elektrostal, Moscow oblast, 144005, Russia

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Correspondence to Zh. V. Zatsepilova .

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Original Russian Text © A.V. Shevelev, Zh.V. Zatsepilova, 2011, published in Defektoskopiya, 2011, Vol. 47, No. 5, pp. 19–22.

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Shevelev, A.V., Zatsepilova, Z.V. Toroidally focused ultrasonic flaw detectors. Russ J Nondestruct Test 47 , 308–310 (2011). https://doi.org/10.1134/S1061830911050093

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Received : 14 January 2011

Published : 28 July 2011

Issue Date : May 2011

DOI : https://doi.org/10.1134/S1061830911050093

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