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Collection Name: MS482 Miscellaneous Missouri Photograph Collection
Description: Computerized illustration of the pattern of the dress version of the "Show Me" Tartan, Missouri's official state tartan. Design by Kenneth Slayor. Visit the Secretary of State's State Symbol website for more information on the State Tartan.
Photographer/Studio: Kenneth Slayor, Chilhowee, MO
Coverage: United States - Missouri
Date: c2019
Rights: permission granted
Credit: Courtesy of Missouri State Archives
Image Number: MS482_Digital013.tif
Institution: Missouri State Archives
There's a new casino in Prince Rupert. There are no real card games with dealers but they have slot machines, computerized Bingo and this game of Backjack. I played for a little while and lost $20 so I put another $20 in and eventually won my money back. At one point I was up $8. I walked away with a half hour of entertainment and even.
The "dealer" even moved their hands like they were dealing cards and moving chips. The dealer also changed - we saw at least 4 different settings and dealers.
PEARL HARBOR (July 02, 2014) Vice Adm. Matthew Nathan, Navy Surgeon General and Chief of the Bureau of Medicine and Surgery, is shown the computerized tomography (CT) scan aboard the People’s Liberation Army (Navy) hospital ship Peace Ark (T-AH 866) during a tour as part of exercise Rim of the Pacific (RIMPAC) 2014. Twenty-two nations, more than 40 ships and submarines, more than 200 aircraft and 25,000 personnel are participating in RIMPAC from June 26 to Aug. 1, in and around the Hawaiian Islands. The world's largest international maritime exercise, RIMPAC provides a unique training opportunity that helps participants foster and sustain the cooperative relationships that are critical to ensuring the safety of sea lanes and security on the world's oceans. RIMPAC 2014 is the 24th exercise in the series that began in 1971. (U.S. Navy photo by Mass Communication Specialist 2nd Class Amanda R. Gray/Released)
Click To See Review Janome 8050 Sewing Machine ---- Maybe if you're looking for the review on Janome 8050 Sewing Machine at discount price, We have found a good deal and prices for this product on Amazon. Get it today!. Check out the product description. Janome Factory Refurbished in the Factory Sealed Box with Janome 20 Year Warranty! The Janome Model 8050 is a one of a kind computerized sewing machine. The featured LCD screen and computer memory program enables easy sewing for your project.50 Built-in Stitches including 3 types of 1-step buttonholesSews up to 820 stitches per minuteTouch Panel for stitch selectionLCD message and display screenPerfect Automatic One-step Sensor ButtonholesPowerful DC motor for extra powerBuilt-in Needle ThreaderJam-proof Full Rotary All Metal HookTop loading magnetic drop-in bobbin case system for easy insertion, removal and cleaningRuns whisper-quietBlanket StitchesAutomatic Stop Needle Up or Down Position ControlsFeatures: * Easy conversion to free arm Needle Up/Down - needle automatically stops up for easy fabric removal or Down for quick pivoting your choice Fail-safe needle insertion 15 Needle Positions for precise needle placement Auto-declutch bobbin winding See-through bobbin cover for checking thread supply One-hand side thread cutter Easy lay-in threading Horizontal spool pin for snag-free performance Extra-high presser foot lift accommodates thick seams and bulky fabrics SFS (Superior Feed System) 7-piece feed dog insures precise control of all fabrics Free Arm for sleeves, cuffs and hard-to-reach areas Quilting guide for parallel rows of stitches Drop-feed for free motion applications, darning, attaching buttons 7 mm (1/4") stitch width for attractive designs Built-in storage compartment Halogen lamp provides bright swing area Steady, consistent electronic speed control Convenient carrying handle Touch Panel for stitch selection LCD message and display screen Perfect one-step Sensor Powerful DC motor for extra power Built-in Needle Threader. Where to buy this Janome 8050 Sewing Machine? Special Offer, Click Here! www.amazon.com/gp/product/B004AQHUF8/ref=as_li_ss_...
Cruise in comfort aboard Bali Bounty Cruises 600 passenger catamaran. With a cruising speed of up to 30 knots, you may sit back, relax and enjoy full staff service while reading the daily newspaper or viewing our onboard video entertainment. We sail from Bali every day.
Bounty Cruises is equipped with state of the art computerized stabilizer and meets with International Safety Standards. Complete with an executive standard of service, the Bounty Catamaran is three decks of pure luxury.
Day Cruise
Join our cruise for a full day of water activities above and below the sea from our 48 m pontoon at the beautiful crystal clear bay on Nusa Lembongan Island. Your day includes hotels transfers, morning and afternoon tea, snorkelling, surf ski, unlimited banana boat rides, 44 m waterslide, glass bottom boat rides, village tour and a scrumptious buffet lunch. Optional extras include diving with BIDP, surf bike and massages.
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Illustration part of the "Amber Tapestry" by Gray Morrow, depicting various characters from the Amber series by Roger Zelazny.
Moire, queen of the undersea reflection of Amber, Rebma (Amber spelled backwards!). Moire and Llewella are half-sisters through their mother Moins. Llewella was a by-blow of Oberon, who seems to have raped, coerced, or seduced every woman of title in the surrounding area.
Moire allows Corwin to walk the Rebma pattern although she declines him troops, as any conflict in Amber is reflected in its underwater sister kingdom. She engages in a short and pleasant dalliance with Corwin which produces no offspring. She also requires Random to marry her courtier Vialle, in repayment for his previous seduction and abandonment of her firstborn daughter Morganthe who killed herself when Random left her. The child of that union, Martin, is Moire's grandson and eventually becomes quite important to Random. In the second half of the Amber series, Martin becomes friends with Corwin's son Merlin and seems to have a very cyber-punk leaning, adding digital and computerized enhancement to his body.
The battery-powered LRV was specially designed to meet the demands of extended lunar exploration and featured computerized navigation, a portable television system capable of sending color images back to Earth via satellite, the ability to carry almost four times its weight, and special wire-mesh wheels capable of navigating the difficult lunar surface. Additionally, special materials provided the LRV protection from lunar temperatures ranging from -200°F to over 200°F. It proved to be a robust vehicle and greatly expanded the possible zone of exploration from each landing site.
The Museum's LRV was built by Boeing as an engineering mock-up, used for form/fit checkout and astronaut demonstrations. It was donated by the Friends for Long Island's Heritage in 1991.
All of the décor elements are manufactured and pre-assembled using cutting-edge computerized equipment to ensure exact alignment with the design intent as well as precision measurements to create seamless on-site implementations.
To see the new casino design and renovation project visit - www.i5design.com/portfolio/casino-design/ft-gibson-casino/
The Baiyoke tower is the highest building in Thailand where you can enjoy the spectacular view of Bangkok and beyond the metropolis, up to the Gulf of Thailand. Maps, computerized multimedia kiosks and coin-activated telescopes help you identify what is laying 250 meters down below your feet. Read more at: baiyokesky.baiyokehotel.com
In 1964, ticketing was computerized on the DELTAMATIC system. On display, at the top, are a headset and key board from the automated reservations machine. On the bottom is seating chart with tabbed stickers to put on passenger boarding passes (as show on the right).
The Spirit of Delta, or Delta Ship 102, housed in Hangar 2 of the Delta Heritage Museum, was Delta Airline's first Boeing 767-200. This aircraft was acquired in 1982 and paid for by Delta employees and retirees who raised $30 million as a gift to the Company. On May 7, 2006 it was pulled into the museum where it was transformed into a unique exhibition space and opened to the public on December 15--24 years after its first flight.
The Delta Heritage Museum, an aviation and corporate museum housed in two 1940's era Delta Air Lines maintenances hangars outside Atlanta Hartsfield International Airport, was established in 1995. The hangars were used until the 1960's when the Delta Technical Operations Center, formerly known as the Jet Base, was completed. The museum's collections and facilities include a number of historical aircrafts including the Spirit of Delta, Delta's first 767, and Ship 41, the first DC-3 to carry Delta passengers, as well as an archives of artifacts related to Delta and its ancestor airlines, an aviation reference library, and a replica of the first Delta station in Monroe, Louisiana.
I've heard some people only like beaches and resorts as their holiday destination. Though I also appreciate those attractions, my family has always balanced our outings with historical areas and places of culture. Okay, I realize you can't get a rich dark tan inside of a museum, but the valuable knowledge and experience will be with you the rest of your life.
While driving cross-country, we made an unplanned stop at a historical pioneer settlement, which was an authentic replication of the way rural people once lived in America's early history. As we strolled around the grounds dotted with cabins, barns, places of trade, churches, and all the other structures pertinent to early pioneers, we would stop and carry-on conversations with the 'inhabitants' who kept in character by acting as if they didn't know we were from hundreds of years in their future. It was fun trying to fool them with our modern gadgets, but we also learned much about the way things were done 'back then'.
The young woman depicted in this painting was busy pulling weeds out of the garden. Her clothes were full and designed to fully protect the skin from the sun's mid-day rays... in contrast to the way we normally dress in the present era. Her life would have been hard. Her day was spent working from sun-up to sun-down in the dust and the dirt. Traveling to beach resorts and other tourist attractions wouldn't have been a part of her world at all.
Six hundred miles later, Carol and I were at the beach.
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The artist is both professionally trained and self-taught in traditional art mediums... as well as utilizing the computer for yet another means to a visual end.
My subjects include the familiar world around us... nature in all it's beauty; the four seasons; people; places; the effects of our involvement upon our world; the animal world; etc.
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Equipment: Celestron NexStar 8SE Computerized Telescope, CGEM Mount, 80mm PHD guide scope. Camera: Canon T1i
While riding Space Mountain, I kept hearing a computerized voice saying "Zone 13, rerouting. Zone 12, rerouting. Zone 11, etc..." Then we suddenly came to a stop at some trim breaks.
A few moments passed, the music stopped, then the lights came on. A few moments after that, a group of 5 team members came rushing up the steps and said "Hang on, you're about to do something most people don't get to do!" I assumed we were going to be walked off but they ended up pushing us down the track like it was a bobsled!
We were at nice gentle coast all the way to the loading area, where, they relocked our safety latches, and sent us off again.
Long before today's blow-everything-up computerized action movies, bards recited poems that had the power to elicit images such as this one in their listeners' imaginations and those of highly skilled painters.
========================================================
Gillis van Valckenborch (1570-1622)
Oil on canvas.
EKM VM 140
Kardriorg Palace Art Museum
Tallinn, Estonia
Thehistorical painter Gillis van Valckenborch, who escaped religious persecution by moving from the southern Netherlands to Frankfurt, painted this dramatic night scene on the basis of the story of the destruction of Troy from Homer's Iliad.
He has depicted the moment when th spirit of the fallen hero Achilles ap-peared and demanded the sacrifice of
the traitorous Polyxena, the daughter of King Priam of Troy, who had been promised to him as a wife.
Polyxena escaped death thanks to Odysseus's masterful diplomacy: to appease Achilles's wrath, a new marriage contract was concluded between Polyxena and Achilles's son Pyrrhus.
As was characteristic of the art of the era, the central story is hidden in the abundance of human figures (lower right) which emphasise the chaos accompanying the destruction of the city.
Proper anchoring requires knowledge, experience, skill, the right gear, and a measure of good luck.
When we anchor Salvation II, we're relying on several hundred feet of anchor chain and an anchor to keep the boat - all 60,000 pounds of it - from "dragging anchor," or taking off on its own across the water like a dog that has escaped his tether.
Once the anchor has been lowered and set, a process I won't describe here, the question then becomes whether the anchor is holding.
There are many ways to figure this out. If there's a strong wind and/or a swift current, you're going to know right away, because the scenery on the shore is going to start moving.
What we do is get out our dedicated laptop that has computerized charts and a feed for a GPS device. Once the chart plotter software and GPS are up and running, I turn on a feature that shows the boat's track with a red line. In this photo, the taupe represents the shore; the blue, shallow water; and the white, deeper water.
An anchor isn't a pin driven through the heart of the boat that keeps it motionless. The boat will move in response to the winds and, more importantly, the tides.
This is a photo of the computerized chart showing the boat's motion at anchor. The boat is the green icon. The red lines trace the boat's motion on the water.
What we're looking for is that nice, reassuring snarl of red lines. It tells us the boat is moving, but only as far as the anchor will let it.
What we don't want to see is the little green icon representing the boat moving away from the snarled red lines on a more or less straight course, dragging its anchor behind it.
You won't be tested on this, but we will.
Buttonholer attachment and cams. I hated making buttonholes as it was so hard to line up--same with the cams. I love the computerized machines so much--it's all easier!
Triangulum Galaxy
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Triangulum Galaxy
VST snaps a very detailed view of the Triangulum Galaxy.jpg
Galaxy Messier 33 in Triangulum
Observation data (J2000 epoch)
Pronunciation/traɪˈæŋɡjʊləm/
ConstellationTriangulum
Right ascension01h 33m 50.02s[1]
Declination+30° 39′ 36.7″[1]
Redshift-0.000607 ± 0.000010[1]
Helio radial velocity-179 ± 3 km/s[2]
Galactocentric velocity-44 ± 6 km/s[2]
Distance (comoving)970 kpc (3.2 Mly)[3]
Apparent magnitude (V)5.72[1]
Characteristics
TypeSA(s)cd[2]
Mass5 × 1010[4] M☉
Number of stars40 billion (4×1010)[6]
Size18.74 kpc (61,120 ly)
(diameter; 25.0 mag/arcsec2 B-band isophote)[5][6]
Apparent size (V)70.8 × 41.7 moa[1]
Other designations
NGC 0598, MCG+05-04-069, UGC 1117, PGC 5818[2]
The Triangulum Galaxy is a spiral galaxy 2.73 million light-years (ly) from Earth in the constellation Triangulum. It is catalogued as Messier 33 or NGC (New General Catalogue) 598. With the D25 isophotal diameter of 18.74 kiloparsecs (61,100 light-years), the Triangulum Galaxy is the third-largest member of the Local Group of galaxies, behind the Andromeda Galaxy and the Milky Way. It is one of the most distant permanent objects that can be viewed with the naked eye.[7]
The galaxy is the smallest spiral galaxy in the Local Group (although the smaller Large and Small Magellanic Clouds may have been spirals before their encounters with the Milky Way), and is believed to be a satellite of the Andromeda Galaxy or on its rebound into the latter due to their interactions, velocities,[8] and proximity to one another in the night sky. It also has an H II nucleus.[9]
Contents
1Etymology
2Visibility
3Observation history
4Properties
4.1Location – distance – motion
4.2Structure
4.3Star formation
4.4Discrete features
4.5Relationship with the Andromeda Galaxy
4.6Planetary nebulae
5See also
6References
7Further reading
8External links
Etymology
The galaxy gets its name from the constellation Triangulum, where it can be spotted.
It is sometimes informally referred to as the "Pinwheel Galaxy" by some astronomy references,[10] in some computerized telescope software, and in some public outreach websites.[11] However, the SIMBAD Astronomical Database, a professional database, collates formal designations for astronomical objects and indicates that Pinwheel Galaxy refers to Messier 101,[12] which several amateur astronomy resources including public outreach websites identify by that name, and that is within the bounds of Ursa Major.[13][14]
Visibility
Under exceptionally good viewing conditions with no light pollution, the Triangulum Galaxy can be seen with the 20/20 vision naked eye;[15] to those viewers, it will sometimes be the farthest permanent entity visible without magnification.[16][17] Its light diffuses (spreads) across a little more than a pinprick of the unmagnified sky, the cause of which is its broadness – this astronomers term a diffuse, rather than compact, object.
Observers range from finding the galaxy easily visible by direct vision in a truly dark (and impliedly dry, cloud-free) sky to needing to use averted vision in rural or suburban skies with good viewing conditions.[15] It has been chosen as one of the critical sky marks of the Bortle Dark-Sky Scale,[18] supported by its relative invariability, reasonable northern declination, and brightness described.
Observation history
The Triangulum Galaxy was probably discovered by the Italian astronomer Giovanni Battista Hodierna before 1654. In his work De systemate orbis cometici; deque admirandis coeli caracteribus ("About the systematics of the cometary orbit, and about the admirable objects of the sky"), he listed it as a cloud-like nebulosity or obscuration and gave the cryptic description, "near the Triangle hinc inde". This is in reference to the constellation Triangulum as a pair of triangles. The magnitude of the object matches M33, so it is most likely a reference to the Triangulum Galaxy.[19]
The galaxy was independently discovered by Charles Messier on the night of August 25–26, 1764. It was published in his Catalog of Nebulae and Star Clusters (1771) as object number 33; hence the name M33.[20] William Herschel compiled his extensive catalog of nebulae, he was careful not to include most of the objects identified by Messier.[21] However, M33 was an exception, and he cataloged this object on September 11, 1784, as H V-17.[22]
Herschel also cataloged the Triangulum Galaxy's brightest and largest H II region (diffuse emission nebula containing ionized hydrogen) as H III.150 separately from the galaxy itself; the nebula eventually obtained NGC number 604. As seen from Earth, NGC 604 is located northeast of the galaxy's central core. It is one of the largest H II regions known, with a diameter of nearly 1500 light-years and a spectrum similar to that of the Orion Nebula. Herschel also noted three other smaller H II regions (NGC 588, 592, and 595).
It was among the first "spiral nebulae" identified as such by Lord Rosse in 1850. In 1922–23, John Charles Duncan and Max Wolf discovered variable stars in the nebulae. Edwin Hubble showed in 1926 that 35 of these stars were classical Cepheids, thereby allowing him to estimate their distances. The results were consistent with the concept of spiral nebulae being independent galactic systems of gas and dust, rather than just nebulae in the Milky Way.[23]
NGC 604 in the Triangulum Galaxy
NGC 604 in the Triangulum Galaxy
Composite of about 54 different pointings with Hubble's Advanced Camera for Surveys.[24]
Composite of about 54 different pointings with Hubble's Advanced Camera for Surveys.[24]
Properties
The Triangulum Galaxy is the third largest member of the Local Group of galaxies. It has a diameter measured through the D25 standard - the isophote where the surface brightness of the galaxy reaches 25 mag/arcsec2, to be about 18.74 kiloparsecs (61,100 light-years),[5] making it roughly 60% the size of the Milky Way. It may be a gravitationally bound companion of the Andromeda Galaxy. Triangulum may be home to 40 billion stars, compared to 400 billion for the Milky Way, and 1 trillion stars for Andromeda Galaxy.[6]
The disk of Triangulum has an estimated mass of (3–6) × 109 solar masses, while the gas component is about 3.2 × 109 solar masses. Thus, the combined mass of all baryonic matter in the galaxy may be 1010 solar masses. The contribution of the dark matter component out to a radius of 55×103 ly (17 kpc) is equivalent to about 5 × 1010 solar masses.[4]
Location – distance – motion
Triangulum (M33; lower left of center) and Andromeda Galaxy (M31; above center)
Estimates of the distance from the Milky Way to the Triangulum Galaxy range from 2,380×103 to 3,070×103 ly (730 to 940 kpc) (or 2.38 to 3.07 Mly), with most estimates since the year 2000 lying in the middle portion of this range,[25][26] making it slightly more distant than the Andromeda Galaxy (at 2,540,000 light-years). At least three techniques have been used to measure distances to M 33. Using the Cepheid variable method, an estimate of 2,770×103 ± 130×103 ly (849 ± 40 kpc) was achieved in 2004.[27][28] In the same year, the tip of the red-giant branch (TRGB) method was used to derive a distance estimate of 2,590×103 ± 80×103 ly (794 ± 25 kpc).[29] The Triangulum Galaxy is around 750,000 light years from the Andromeda Galaxy.[30]
In 2006, a group of astronomers announced the discovery of an eclipsing binary star in the Triangulum Galaxy. By studying the eclipses of the stars, astronomers were able to measure their sizes. Knowing the sizes and temperatures of the stars, they were able to measure the absolute magnitude of the stars. When the visual and absolute magnitudes are known, the distance to the star can be measured. The stars lie at the distance of 3,070×103 ± 240×103 ly (941 ± 74 kpc).[25] The average of 102 distance estimates published since 1987 gives a distance modulus of 24.69, or .883 Mpc (2,878,000 light-years).[31]
The Triangulum Galaxy is a source of H2O maser emission.[32] In 2005, using observations of two water masers on opposite sides of Triangulum via the VLBA, researchers were, for the first time, able to estimate the angular rotation and proper motion of Triangulum. A velocity of 190 ± 60 km/s relative to the Milky Way was computed, which means Triangulum is moving towards Andromeda Galaxy and suggesting it may be a satellite of the larger galaxy (depending on their relative distances and margins of error).[8]
In 2004, evidence was announced of a clumpy stream of hydrogen gas linking the Andromeda Galaxy with Triangulum, suggesting that the two may have tidally interacted in the past. This discovery was confirmed in 2011.[33] A distance of less than 300 kiloparsecs between the two supports this hypothesis.[34]
The Pisces Dwarf (LGS 3), one of the small Local Group member galaxies, is located 2,022×103 ly (620 kpc) from the Sun. It is 20° from the Andromeda Galaxy and 11° from Triangulum. As LGS 3 lies at a distance of 913×103 ly (280 kpc) from both galaxies, it could be a satellite galaxy of either Andromeda or Triangulum. LGS 3 has a core radius of 483 ly (148 pc) and 2.6 × 107 solar masses.[35]
Pisces VII/Triangulum (Tri) III may be another satellite of Triangulum.[36]
Structure
Infrared image of M33 taken with the Spitzer Space Telescope
Ultraviolet image of M33 by GALEX observatory
In the French astronomer Gérard de Vaucouleurs' revised Hubble Sandage (VRHS) system of galaxy morphological classification, the Triangulum Galaxy is classified as type SA(s)cd. The S prefix indicates that it is a disk-shaped galaxy with prominent arms of gas and dust that spiral out from the nucleus—what is commonly known as a spiral galaxy. The A is assigned when the galactic nucleus lacks a bar-shaped structure, in contrast to SB class barred spiral galaxies. American astronomer Allan Sandage's "(s)" notation is used when the spiral arms emerge directly from the nucleus or central bar, rather than from an inner ring as with an (r)-type galaxy. Finally, the cd suffix represents a stage along the spiral sequence that describes the openness of the arms. A rating of cd indicates relatively loosely wound arms.[37]
This galaxy has an inclination of 54° to the line of sight from Earth, allowing the structure to be examined without significant obstruction by gas and dust.[38][39] The disk of the Triangulum Galaxy appears warped out to a radius of about 8 kpc. There may be a halo surrounding the galaxy, but there is no bulge at the nucleus.[40] This is an isolated galaxy and there are no indications of recent mergers or interactions with other galaxies,[39] and it lacks the dwarf spheroidals or tidal tails associated with the Milky Way.[41]
Triangulum is classified as unbarred, but an analysis of the galaxy's shape shows what may be a weak bar-like structure about the galactic nucleus. The radial extent of this structure is about 0.8 kpc.[42]
The nucleus of this galaxy is an H II region,[32] and it contains an ultraluminous X-ray source with an emission of 1.2 × 1039 erg s−1, which is the most luminous source of X-rays in the Local Group of galaxies. This source is modulated by 20% over a 106-day cycle.[43] However, the nucleus does not appear to contain a supermassive black hole, as an upper limit of 3,000 solar masses is placed on the mass of a central black hole based upon the velocity of stars in the core region.[44]
The inner part of the galaxy has two luminous spiral arms, along with multiple spurs that connect the inner to the outer spiral features.[38][39] The main arms are designated IN (north) and IS (south).[45]
Star formation
NGC 604, a star-forming region in the Triangulum Galaxy, as imaged by the Hubble Space Telescope.
In the central 4′ region of this galaxy, atomic gas is being efficiently converted to molecular gas, resulting in a strong spectral emission of CO. This effect occurs as giant molecular clouds condense out of the surrounding interstellar medium. A similar process is taking place outside the central 4′, but at a less efficient pace. About 10% of the gas content in this galaxy is in the molecular form.[38][39]
Star formation is taking place at a rate that is strongly correlated with local gas density, and the rate per unit area is higher than in the neighboring Andromeda Galaxy. (The rate of star formation is about 3.4 Gyr−1 pc−2 in the Triangulum Galaxy, compared to 0.74 in Andromeda.[46]) The total integrated rate of star formation in the Triangulum Galaxy is about 0.45 ± 0.1 solar masses per year. It is uncertain whether this net rate is currently decreasing or remaining constant.[38][39]
Based on analysis of the chemical composition of this galaxy, it appears to be divided into two distinct components with differing histories. The inner disk within a radius of 30×103 ly (9 kpc) has a typical composition gradient that decreases linearly from the core. Beyond this radius, out to about 82×103 ly (25 kpc), the gradient is much flatter. This suggests a different star formation history between the inner disk and the outer disk and halo, and may be explained by a scenario of "inside-out" galaxy formation.[40] This occurs when gas is accumulated at large radii later in a galaxy's life space, while the gas at the core becomes exhausted. The result is a decrease in the average age of stars with increasing radius from the galaxy core.[47]
Discrete features
Using infrared observations from the Spitzer Space Telescope, a total of 515 discrete candidate sources of 24 μm emission within the Triangulum Galaxy have been catalogued as of 2007. The brightest sources lie within the central region of the galaxy and along the spiral arms.
Many of the emission sources are associated with H II regions of star formation.[48] The four brightest HII regions are designated NGC 588, NGC 592, NGC 595, and NGC 604. These regions are associated with molecular clouds containing (1.2–4) × 105 solar masses. The brightest of these regions, NGC 604, may have undergone a discrete outburst of star formation about three million years ago.[49] This nebula is the second most luminous HII region within the Local Group of galaxies, at (4.5 ± 1.5) × 107 times the luminosity of the Sun.[46] Other prominent HII regions in Triangulum include IC 132, IC 133, and IK 53.[45]
The northern main spiral arm contains four large HII regions, while the southern arm has greater concentrations of young, hot stars.[45] The estimated rate of supernova explosions in the Triangulum Galaxy is 0.06 Type Ia and 0.62 Type Ib/Type II per century. This is equivalent to a supernova explosion every 147 years, on average.[50] As of 2008, a total of 100 supernova remnants have been identified in the Triangulum Galaxy,[51] the majority of which lies in the southern half of the spiral galaxy. Similar asymmetries exist for H I and H II regions, plus highly luminous concentrations of massive, O type stars. The center of the distribution of these features is offset about two arc minutes to the southwest.[45] M33 being a local galaxy, the Central Bureau for Astronomical Telegrams (CBAT) tracks novae in it along with M31 and M81.[52]
About 54 globular clusters have been identified in this galaxy, but the actual number may be 122 or more.[41] The confirmed clusters may be several billion years younger than globular clusters in the Milky Way, and cluster formation appears to have increased during the past 100 million years. This increase is correlated with an inflow of gas into the center of the galaxy. The ultraviolet emission of massive stars in this galaxy matches the level of similar stars in the Large Magellanic Cloud.[53]
In 2007, a black hole about 15.7 times the mass of the Sun was detected in this galaxy using data from the Chandra X-ray Observatory. The black hole, named M33 X-7, orbits a companion star which it eclipses every 3.5 days. It is the largest stellar mass black hole known.[54][55]
Unlike the Milky Way and Andromeda galaxies, the Triangulum Galaxy does not appear to have a supermassive black hole at its center. This may be because the mass of a galaxy's central supermassive black hole correlates with the size of the galaxy's central bulge, and unlike the Milky Way and Andromeda, the Triangulum Galaxy is a pure disk galaxy with no bulge.[56]
Relationship with the Andromeda Galaxy
Triangulum on the collision paths of the Milky Way and Andromeda galaxies.
As mentioned above, M33 is linked to M31 by several streams of neutral hydrogen[57] and stars,[57] which suggests that a past interaction between these two galaxies took place from 2 to 8 billion years ago,[58][59] and a more violent encounter will occur 2.5 billion years in the future.[57]
The fate of M33 was uncertain in 2009 beyond seeming to be linked to its larger neighbor M31. Suggested scenarios include being torn apart and absorbed by the greater companion, fueling the latter with hydrogen to form new stars; eventually exhausting all of its gas, and thus the ability to form new stars;[60] or participating in the collision between the Milky Way and M31, likely ending up orbiting the merger product and fusing with it much later. Two other possibilities are a collision with the Milky Way before the Andromeda Galaxy arrives or an ejection out of the Local Group.[61] Astrometric data from Gaia appears in 2019 to rule out the possibility that M33 and M31 are in orbit. If correct, M33 is on its first infall proper into the Andromeda Galaxy (M31).[62]
Planetary nebulae
Planetary nebulae are not only important contributors to the chemical enrichment of galaxies, but provide valuable information on single and binary stellar evolution. In addition, these objects seem to always produce very bright planetary nebulae with consistent luminosities, regardless of the galaxy's mass, age, or metallicity. This feature is very useful as a standard candle for distance measurements.
Large systematic research on this topic has been done by Rebeca Galera-Rosillo and co-authors in 2018.[63] This work benefited from the use of the INT and WHT telescopes located at La Palma island. As a result of this study, three new planetary nebulae were discovered.
Newly discovered PNe (2018), Rebeca named the PNe after her closest family members.
GCM 1 (Ovejisaurio),01:34:48.86+31:05:14.8
GCM 2, (Cuchilla Andante)01:33:45.20+30:21:22.0
GCM 3, (Sewi)01:33:52.30+30:21:12.0
Lawrence Livermore National Laboratory physicists, engineers, and computer scientists have developed a new computed tomography (CT, also known as computerized axial tomography or CAT) x-ray system to image nuclear weapon components removed temporarily from the stockpile for inspection. The Confined Large Optical Scintillator Screen and Imaging System (CoLOSSIS) consists of a scintillator (a material that emits light when struck by ionizing radiation); a pyramid-shaped central mirror; four turning mirrors; and four high-resolution, low-intensity visible-light charge-coupled-device (CCD) cameras. The system’s software assembles the collected digital radiographs into a large three-dimensional (3D) image that scientists can “walk through” to discover any problems or anomalies. CoLOSSIS has been installed at the Department of Energy's National Nuclear Security Administration’s Pantex Plant near Amarillo, Texas. [More information]
I made two of these, and they took about 40 hours each. They are 9.5" and they are art sculptures that do not move. I did not cut corners on any aspect of them. It is incredibly difficult to sculpt a 3-D character from a computerized cartoon image.
I am NOT interested in making any more, so sorry but there will only ever be two made by me :-)
The X-29, featuring one of the most unusual aircraft designs in aviation history, was flown as a technology demonstrator. The concepts and technologies explored were the use of advanced composites in aircraft construction; variable-camber wing surfaces; the unique forward-swept wing and its thin supercritical airfoil; strake flaps; and a computerized fly-by-wire flight control system that overcame the aircraft's instability. 1990-un-edited-Not part of my personal collection
Lawrence Livermore National Laboratory physicists, engineers, and computer scientists have developed a new computed tomography (CT, also known as computerized axial tomography or CAT) x-ray system to image nuclear weapon components removed temporarily from the stockpile for inspection. The Confined Large Optical Scintillator Screen and Imaging System (CoLOSSIS) consists of a scintillator (a material that emits light when struck by ionizing radiation); a pyramid-shaped central mirror; four turning mirrors; and four high-resolution, low-intensity visible-light charge-coupled-device (CCD) cameras. The system’s software assembles the collected digital radiographs into a large three-dimensional (3D) image that scientists can “walk through” to discover any problems or anomalies. CoLOSSIS has been installed at the Department of Energy's National Nuclear Security Administration’s Pantex Plant near Amarillo, Texas. [More information]
1. Aim Allan wake
2. I told people outloud, that i live in fever swamp by goosebumps and philly the movie, with will smith and bald guy, about isolation, gays, and aids, but everyone around me thinks I'm in hbos the wire.
3. Just how he computer7zed my internet to not help me, and only let disinterested people see my websites, he computerized 300 miles where i live, to all hate me, and all the hot girls only like the guys who hate me, and he gives the guys who help spread propaganda against me really hot pussy, and i could tell ppl 100percent the truth, and no one would care here in fever swamp, only if they going to suck a hot glitch, cause were there's100s roar the guys"the troops here " and I'm reserve, any guy here can get hot women, and there 1000s and I'm one guy, I'm the one with massive attention, and they are dumb....but in there biodome, they win, they all can have hot babes , i can not, there the troops, i signed up for army, I'm not, i getinsulted 24/7, while they score hot babes like rockstars
Hot tub lung is associated with exposure to Mycobacterium avium intracellulare complex (MAC) when present in aerosols from indoor hot tubs/spas as well as swimming pools, showers, humidifiers, and wind instruments.
High resolution computerized tomography (HRCT) findings are usually diffuse centrilobular nodules and/or ground glass opacities. Cavitary nodules have also been reported.
It is generally considered to be a form of hypersensitivity pneumonitis {HP), but since MAC has been cultured from lung tissue there is uncertainty as to whether it represents an infection, hypersensitivity, or a combination of both. Biopsy usually shows non-necrotizing granulomas which may be localized around airways; necrotizing granulomas are sometimes present. Granulomas are present in the lumens of small bronchioles as well as in the interstitium and airspaces. Airspace granulomas may also be seen in sarcoidosis, but they are not nearly as numerous and conspicuous as they are in hot tub lung. The granulomas are usually larger and more well-formed than those seen in non-mycobacterial HP. Organizing pneumonia is often present. AFB stains of granulomas are usually negative but may be positive. Lymphangitic distribution of granulomas and granulomatous vasculitis are characteristic features of sarcoidosis that are not seen in hot tub lung. Hot tub lung can be suspected, but not diagnosed, based on biopsy findings alone. In addition to histologic findings, definitive diagnosis requires a history of indoor hot tub use or exposure to aerosolized water contaminated with MAC.
Images contributed by Dr. Sam Albadri - @sam_albadri.
Released in September 2001 for the 2002 model year, Toyota released the Camry XV30 series as a larger sedan, but without a station wagon for the first time. The wagon's demise occurred due to its sales erosion to minivans and crossover SUVs.
Toyota redesigned this series from the ground up for the first time since the V30 and XV10. Through efficiency gains such as increased computerization, and by having the XV30 ride on the K platform introduced with the Toyota Highlander (XU20) of 2000, Toyota expedited the XV30 production development stage to 26 months, down from 36 months with the XV20. As a consequence, Toyota claimed the XV30 to have cost 30 percent less to design and develop than its predecessor. XV30 also had increased parts content over the XV20, but did not cost any more to manufacture.
Until the 2003 model year, the Camry Solara remained on the XV20 series chassis, and received only minor styling upgrades to the front and rear ends. However, the Solara did receive the same 2.4-liter 2AZ-FE I4 engine that was available on the Camry sedan. The US received three engine options, a 115 kW (154 hp) 2.4-liter inline-four, a 142 kW (190 hp) 3.0-liter V6, and a 157 kW (210 hp) 3.3-liter version of the same. The 3.3-liter was only available for the Camry's sportier "SE" model.
The white Camry here is undoubtedly a better car than any of the other designed this month. Faster, safer, more efficient, quieter. These are all the hallmarks of progress. The Camry's design, however, is the very definition of cautious.
In the future, no doubt, there will be some people who get misty eyed when they see one drive down the road. As mentioned, not a bad car, but not inspired either.
Using the computerized dietary-intake survey program that was developed and validated by U.S. Department of Agriculture (USDA) Agricultural Research Service (ARS) Beltsville Human Nutrition Research Center (BHNRC) scientists’ nutritionist Grace Omolewa-Tomobi uses serving-size aides to help a study participant to recall food portions and beverages she consumed while in the study on Feb. 29, 2012. USDA photo by Stephen Ausmus.
The tea containers were still absent when I was here the week prior: flic.kr/p/nk4Zvn, and may of been some of the very last things done to cap off this massive remodel/expansion. Maybe the shaved ice/slushie machine needs a software update to be operational!?? Looks like a very nice computer monitor on it, but a computerized slushie machine seems like a bit of overkill!
____________________________________
Kroger, 2004-built, Goodman Rd. at Getwell Rd., Southaven MS
The Postcard
A postcard that was published by P. Sander of Philadelphia and Atlantic City. The card was posted in Atlantic City on Tuesday the 7th. November 1922 to:
Miss Shoia Morse,
London Orphan School,
Stratford,
London,
England.
The message on the divided back of the card was as follows:
"Dearest Shoia,
Thanks for your letter.
I have just returned from
Philadelphia, been away
two weeks and had a
lovely time.
How are you getting on?
Hoping you are well.
With fond love from
Uncle and Auntie
xxxxxx"
Bally's Atlantic City
Bally's Atlantic City is a casino hotel on the Boardwalk in Atlantic City, New Jersey, owned and operated by the Bally's Corporation.
The Marlborough-Blenheim Hotel stood on the site before the casino was built. It is famous for its address of "Park Place and the Boardwalk", two locations popularized by the board game Monopoly. Bally's is one of the largest hotels on the boardwalk with nearly 1,169 rooms.
Its historic Dennis Tower was constructed in stages between 1906-1929.
In 1997, The Wild Wild West Casino was opened as an expansion of Bally's.
History of the Site
The site now occupied by Bally's was originally the location of two separate hotels - the Marlborough-Blenheim Hotel and the Dennis Hotel.
(a) The Marlborough-Blenheim Hotel
The Marlborough House was built in 1900 by Josiah White III in the Queen Anne style. White expanded the resort in 1905 with a new, separate wing, built entirely of concrete, which opened in 1906 as the Blenheim. The hotel was then renamed the Marlborough-Blenheim.
(b) The Dennis Hotel
The Dennis Hotel began as a pre-Civil War cottage built by William Dennis. After the war, it was acquired by Joseph H. Borton, who built a large addition in 1892, in the French chateau style.
The Dennis was sold to Walter Buzby just after the turn of the twentieth century who added a huge new six-story eastern wing, which was completed in 1906. It is the oldest portion still standing.
In 1910, the 1892 Michigan Avenue west wing was demolished and replaced with a larger six-storey wing.
In 1925, Buzby had Smedley design a huge ten-story rear wing, containing a new lobby and ballrooms, which would connect the eastern and western wings extending to the Boardwalk.
In 1929 Buzby hired a Philadelphia Quaker firm, Price and Walton, to design a seven-storey addition to the west wing, which extended it seventy feet toward the ocean, bringing it even with the 1906 wing. This gave the Dennis its current form.
In 1969, the Buzby family sold the Dennis for $4 million to Gary and Lewis Malamut. When they defaulted on the mortgage in 1975, the hotel was returned to the Buzby family. It was soon after foreclosed by the First National Bank of South Jersey.
Bally's Park Place (1979–2000)
In 1977, flamboyant art dealer Reese Palley and local attorney Martin Blatt purchased the Marlborough-Blenheim from the White family. They intended to spend $35 million on renovations, preserving the Blenheim wing, while razing the Marlborough to make way for a modern casino hotel.
Palley successfully got the Blenheim wing placed on the National Register of Historic Buildings. In June 1977, Bally Manufacturing, the world's largest producer of slot machines, leased the Marlborough-Blenheim from Palley and Blatt for 40 years, with an option for a further 100 years.
On the 17th. August 1977, Bally announced that it had purchased the neighboring Dennis Hotel for $4 million from the First National Bank of South Jersey. On the 25th. October 1977, Josiah White IV, grandson of the Marlborough-Blenheim's founder, presided over the closure of that hotel, locking its front door.
After Bally took control of the two properties, it announced plans to raze all three hotel buildings - the Marlborough, the Blenheim, and the Dennis, despite protests, to make way for the new "Bally's Park Place Casino and Hotel", an $83 million casino/hotel.
The new resort was to have a 39-storey, octagonal hotel tower and a huge three-level podium, containing a 75,000 square-foot casino, along with other resort and convention facilities. However, in an effort to offset costs and open the casino as soon as possible, the Dennis Hotel was retained to serve as the temporary hotel for Bally's until a new tower could be built.
In November 1978, Bally demolished the Marlborough-Blenheim and quickly cleared the land to begin building Bally's Park Place Casino. The casino opened on the 30th. December 1979, with the newly renovated Dennis serving as its hotel.
In 1989, Bally constructed a 750-room hotel tower in a modern style, with an exterior of light pink glass. On the 2nd. July 1997, The Wild Wild West Casino opened as the second casino at Bally's.
Bally's Atlantic City (2000–Present)
In 2000, Bally's Park Place changed its name and became Bally's Atlantic City. The adjacent Claridge Hotel and Casino was purchased and incorporated into Bally's in 2003, and was renamed the Claridge Tower. The casino in the Claridge Tower was named The Ridge. The casino was renovated in 2008 from a standard casino floor to an upscale lounge-casino.
In 2005, Harrah's Entertainment purchased Bally's. In 2008, Harrah's spent $38.5 million to purchase the row of shops between the Dennis Tower and the boardwalk, and then spent a further $23 million to demolish the shops and restore the open plaza, and to restore the facade of the Dennis Tower and renovate its rooms.
In 2012, The Ridge closed its gambling and food amenities. The tower's 500 hotel rooms continued to be used for Bally's guests until it was sold in 2013, to be reopened as the independent Claridge Hotel.
In October 2017, ownership of Bally's was transferred to Vici Properties. In April 2020, Twin River Worldwide Holdings (later Bally's Corporation) agreed to buy Bally's Atlantic City from Vici. The deal excluded the Wild Wild West Casino which contains a sports betting facility, and operations were transferred to Caesars Atlantic City.
Twin River also announced that they would acquire a license to give Bally's their own sports book, online sports betting, and I-Gaming. The sale was completed in November 2020.
Gaming
The casino at Bally's has over 83,569 sq ft (7,763.8 m2) of gaming space, with approximately 1500 slot machines. Table games include Blackjack, Baccarat, Craps, Roulette, Spanish 21, Let it Ride, and Pai Gow Tiles.
Specialty games and poker variations known as "Carnival Games" include Mississippi Stud, 3-Card Poker, 4-Card Poker, Heads Up Hold’em, High Card Flush, and Pai Gow Poker.
Recent developments include games which combine the features of live table games with those of slot machines: The multi-player Roulette automatically spins the ball, but the bet and payout function is mostly handled by computerized video terminals for each player.
A similar multi-player machine throws a pair of large craps dice. Bally's also has a FanDuel sportsbook which offers sports betting. As provided by local and state law, there are scattered areas where smoking is permitted, totaling 25% of the official gaming space. (Aside from this exception, smoking is banned by law throughout the rest of the casino and hotel).
Under New Jersey law, persons under 21 years of age are not permitted to gamble. They may only pass through the main aisles of the casino when accompanied by someone over 21 years old to cross between hotel areas and exits, and may not stop or slow down to observe the games.
Desmond 'Dizzy' de Villiers
So what else happened on the day that the card was posted?
Well, the 7th. November 1922 marked the birth of Desmond ‘Dizzy’ de Villiers.
Desmond was chief test pilot at de Havilland, and the world's first open-cockpit pilot to reach supersonic speed.
The Life of Desmond de Villiers
Desmond de Villiers was educated at Bedford Modern School. During World War II he was a Squadron Leader in the Royal Air Force, and was awarded the AFC. He principally flew Beaufighters in RAF Fighter Command and RAF Coastal Command.
In 1943, de Villiers was seconded to de Havilland where he became chief test pilot, and the world's first open-cockpit pilot to reach supersonic speed (albeit inadvertently, the cockpit canopy flew off mid-flight and landed in the garden of a house in Blundellsands near Southport).
He was also the second British pilot to exceed Mach 2.
Desmond was chief experimental test pilot on the English Electric Lightning programme (making more than 1,000 flights). During his test career, he flew more than 6,000 hours in 130 different aircraft.
In 1951, de Villiers flew the Mamba Marathon at the Farnborough Airshow.
Retirement and Death of Desmond de Villiers
De Villiers retired from test flying in 1967. He died on the 19th. June 1976 at the young age of 53.
Volume Rendering of an abdominal CT with oral contrast.
Bilateral duplex kidney with ureter duplex; kidney cysts.
Manual segmentation of ureters and bladders (to assign the yellow color).
Rendering done with a Carestream workstation.
Primera Iglesia Metodista Libre representatives receive their invoice from Community FoodBank of New Jersey Customer Service Specialist Maria Sylvia, for more than 2,000 pounds of commodities, on January 20, 2016, in Hillside, New Jersey. A computerized system summarizes warehouse data from checkout points to produce invoices for charitable organization representatives departing with their goods. Fresh foods will soon be used to produce meals at congregate feeding centers for those in need throughout the state. Other goods with longer shelf life will be used to support meals through the month.
U.S. Department of Agriculture (USDA) Food and Nutrition Service (FNS) partnered with the Community FoodBank of New Jersey, the New Jersey Department of Agriculture, and Emergency Support Function #11 partners to respond to the disaster nutrition needs of those most severely impacted by Hurricane Sandy. FoodBank packaged and delivered USDA Foods as part of a Disaster Household Distribution Program to communities in need throughout New Jersey. The FoodBank utilized the processes it already had in place for packaging Commodity Supplemental Food Program boxes and lessons learned from Hurricane Irene and Tropical Storm Lee to quickly serve 24,000 households affected by Hurricane Sandy. USDA FNS relies on strong partnerships with food banks, such as the Community FoodBank of New Jersey, and other organizations at the local, state, and federal levels to provide USDA Foods for disaster congregate and household feeding. USDA coordinated its disaster nutrition response efforts with the State under FEMA’s Emergency Support Function #11 - Agriculture and Natural Resources. At the Federal level, ESF #11 supports State, tribal, and local authorities and other Federal agency efforts to provide nutrition assistance to those most severely impacted by disasters. USDA Photo by Lance Cheung.
IMO Secretary-General Sekimizu has opened the second session of the Sub-Committee on Ship Design and Construction (SDC) (16-20 February), which is being chaired by Mrs Anneliese Jost (Germany). Items on the agenda include: revision of SOLAS chapter II-1 subdivision and damage stability regulations; development of second generation intact stability criteria; passenger ship matters including computerized stability support for the master in case of flooding and amendments to SOLAS in relation to the opening of passenger ship watertight doors; and revisions to the Interim Guidelines for wing-in-ground (WIG) craft.
Our cataloguing systems haven't really changed since 1960s, but indexing and searching has been computerized. Plus we invented subject headings somewhere along the line.
Times Square, New York City, New Years Eve Ball Drop, 2012 - 2013
The Times Square Ball is a time ball located atop the One Times Square building in New York City, primarily utilized as part of New Year's Eve celebrations held in Times Square. Yearly at 11:59 p.m. EST on December 31, the ball is lowered 77 feet (23 m) down a specially designed flagpole, resting on the midnight to signal the start of the new year. The first ball drop in Times Square took place on December 31, 1907, and has been held annually since (except in 1942 and 1943 in observance of wartime blackouts). The ball's design has also been updated over the years to reflect new advances in technologies—its original design utilized 100 incandescent light bulbs, iron, and wood in its construction, while its current incarnation features a computerized LED lighting system and an outer surface consisting of triangle-shaped crystal panels. As of 2009, the ball is also displayed atop One Times Square year-round and is removed only for general maintenance.
The Times Square ball drop is one of the best-known New Year's celebrations internationally, attended by at least one million spectators yearly, with an estimated global audience of at least 1 billion. The prevalence of the Times Square ball drop has also inspired other similar "drops" held locally in other cities and towns around the world.
“Dick Clark’s New Year’s Rockin’ Eve with Ryan Seacrest,” from American Idol as the host
Performers of the 2012 - 2013 celebration Carly Rae Jepsen, Neon Trees, Flo Rida, Pitbull, with Taylor Swift, in the headliner position just before midnight.
For more on New Years Eve in Times Square visit:
Photo
Times Square, New York City, USA, North America
12-31-2012
Art by Sherrie Thai of Shaireproductions.com
Medium: Traditional pen/ink and digital illustration, inspired by Edward Curtis photograph. The title is a collage with handwritten and computerized fonts.
The UP manifest on the right is actually coming at you, running long nose forward with 3 engines of light power. But, the crashed computerized signal system at the diamond isn't letting it through to Global 3. So, the conductor of the light power lets a "Z" train through first (with the DPU on the left), then flags the light power on the right to come through. Shot at the Rochelle, IL Railroad Park.
In 1985 the X-29A on display became the world's first forward-swept aircraft to fly supersonically. The X-29A program explored cutting-edge aircraft design features, including forward-swept wings, advanced materials, a forward-mounted elevator (or canard) and a computerized flight control system. It was managed by the U.S. Air Force and funded by DARPA (Defense Advanced Research Projects Agency), the USAF and NASA.
The museum’s aircraft is the first of two X-29As built by Grumman, and it made its first flight in December 1984. The second X-29A first flew in 1989 and continued to perform test flights into the early 1990s. After successfully completing the test program, the X-29A on display was retired to the museum in late 1994.
National Museum of the US Air Force
Wright-Patterson AFB
Dayton, OH
Cruise in comfort aboard Bali Bounty Cruises 600 passenger catamaran. With a cruising speed of up to 30 knots, you may sit back, relax and enjoy full staff service while reading the daily newspaper or viewing our onboard video entertainment. We sail from Bali every day.
Bounty Cruises is equipped with state of the art computerized stabilizer and meets with International Safety Standards. Complete with an executive standard of service, the Bounty Catamaran is three decks of pure luxury.
Day Cruise
Join our cruise for a full day of water activities above and below the sea from our 48 m pontoon at the beautiful crystal clear bay on Nusa Lembongan Island. Your day includes hotels transfers, morning and afternoon tea, snorkelling, surf ski, unlimited banana boat rides, 44 m waterslide, glass bottom boat rides, village tour and a scrumptious buffet lunch. Optional extras include diving with BIDP, surf bike and massages.
Please Visit our Official Website: www.bali-individually.com/tour-organizer/category/adventu.... If you have questions or need assistance with a reservation, please call or click to chat online or send us e-mail for inquiry, the best price and packages: sales@bali-individually.com | Telp. +62 - 361-7415637 | text message: +62-81338579071 | facebook: www.facebook.com/pages/Bali-Villa-Reservation/251116974245
Four Steps to Better Health Through Quality Chiropractic Care
If you decide to become a patient of a CBP doctor, there are four important steps we ask you to go through:
History of Injury and Examination,
Postural Analysis (some doctors utilize computerized methods such as the PosturePrint system)
Spinal X-rays (analyzed either by hand or with use of computer aided systems such as PostureRay),
Report of Findings - Where the doctor will explain your problems and if he/she can help through application of chiropractic services and the unique recommended plan for your case.
History of Injury and Examination
Our History of Injury is designed to determine whether your condition is within the realm of our care. Based upon the results, one of the doctors will make appropriate recommendations regarding an examination or referral to another doctor if your presenting problem is not a chiropractic condition. Most often, your condition will be treatable by our care.
A thorough spinal and musculo-skeletal examination will be performed in order to identify which structures of your body are injured and most likely causing your problem.
Computerized Postural Analysis
It has been known for years that body posture is like a “Window into the Shape of the Spinal Column”. Figure 1 shows that Abnormal Posture is always associated with an abnormal spine. Body Postural problems aid the doctor of chiropractic in identifying a variety of dysfunctions in the spinal column. Abnormal Postures can cause or relate to a number of health problems. Abnormal Posture causes increased force and pressure on the muscles, ligaments, and bones of your spinal column. These abnormal forces (caused by abnormal posture) lead to a break down of body tissues causing pain and damage.
Figure 2: Postural Decay as we age.
Posture Digitization: Postural photographs of you the patient can be obtained, in which a sophisticated computer program known as PosturePrint will objectively measure your postural distortions. These photographs enable the doctor to detect and measure abnormal positions of the human skull, shoulders, ribcage, pelvis, knees, and feet. In other words, he or she can show you how far out of alignment your posture is. This helps explain why you may be hurting as well as aid the doctor in prescribing corrective postural-based exercises unique to CBP rehabilitative methods.
(Click Here to download sample PosturePrint Report of Findings - This PosturePrint Examination is part of your initial patient workup)
Spinal X-rays
Many patients often ask if a chiropractor should take x-rays of their spines. The answer is simple. Properly taken spinal x-rays are like a blue print of your spine. With x-rays, the chiropractor can see how an individual spine deviates from normal alignment and we can clearly decide on appropriate treatment. Without an x-ray they would only be guessing. Would you want a mechanic to work on your car engine without looking under the hood?
For example, the figure below is a sample of common abnormal neck alignment subluxations (viewed from the side) with an estimate on average time needed to rehab such problems. It is clearly evident the further your neck is from the normal, then the longer you will need to perform rehabilitative measures. Please note that these are only generic estimates, as many factors dictate how fast a patient responds such as age, the length of time the problem has been there, amount spinal degeneration, etc.
Another important finding that properly taken x-rays will identify is spinal arthritis. Many people are not even aware that spinal disc disease and bone arthritis are developing in their spines. For many people this is a “time bomb” waiting to explode. Figure 6 below shows an abnormal neck (viewed from the side) with arthritis in the mid neck.
Figure 6: Side view showing arthritis in the Neck
Report of Findings
The report of findings is a very important part of communication in a CBP chiropractor's office. Before they decide if Chiropractic care is right for you, they will sit down with you (the patient) and explain the findings of the examination, posture analysis, and spinal x-rays. Many times patients tell the CBP chiropractor that other doctors never have shown them their spinal x-rays. This never happens at at a CBP practioner's office. We are confident that you will find that CBP trained chiropractors are very thorough in the search, identification and explanation of your spinal problem.
Once they have identified your particular spinal problem, the doctor will recommend an appropriate treatment plan specific to your condition.
+++ DISCLAIMER +++
Nothing you see here is real, even though the conversion or the presented background story might be based on historical facts. BEWARE!
Some background:
The North American A-5 Vigilante (Prior to 1962 unification of Navy and Air Force designations, it was designated the A3J) was an American carrier-based supersonic bomber designed and built by North American Aviation for the United States Navy. In 1953, North American Aviation began a private study for a carrier-based, long-range, all-weather strike bomber, capable of delivering nuclear weapons at supersonic speeds. This proposal, the North American General Purpose Attack Weapon (NAGPAW) concept, was accepted by the United States Navy, with some revisions, in 1955. A contract was awarded on 29 August 1956. Its first flight occurred two years later, on 31 August 1958 in Columbus, Ohio.
At the time of its introduction, the Vigilante was one of the largest and by far the most complex aircraft to operate from a Navy aircraft carrier. It had a high-mounted swept wing with a boundary-layer control system (blown flaps) to improve low-speed lift. It had no ailerons; roll control was provided by spoilers in conjunction with differential deflection of the all-moving tail surfaces. The use of aluminum-lithium alloy for wing skins and titanium for critical structures was also unusual. The A-5 had two widely spaced General Electric J79 turbojet engines, fed by inlets with variable intake ramps, and a single large all-moving vertical stabilizer. Preliminary design studies employed twin vertical fin/rudders, but this was eventually changed to a single tall but foldable fin. The wings and the nose radome folded for carrier stowage, too. The Vigilante had a crew of two seated in tandem, a pilot and a bombardier-navigator (BN) (reconnaissance/attack navigator (RAN) on later reconnaissance versions).
The Vigilante had advanced and complex electronics when it first entered service. It had one of the first "fly-by-wire" systems on an operational aircraft (with mechanical/hydraulic backup) and a computerized AN/ASB-12 nav/attack system incorporating a head-up display ("Pilot's Projected Display Indicator" (PPDI), one of the first), multi-mode radar, radar-equipped inertial navigation system (REINS, based on technologies developed for North American's Navaho missile), closed-circuit television camera under the nose, and an early digital computer known as "Versatile Digital Analyzer" (VERDAN) to run it all.
The aircraft replaced the subsonic Douglas A-3 Skywarrior as the Navy's primary nuclear-strike aircraft, but only briefly. Given its original design as a carrier-based, supersonic, nuclear heavy attack aircraft, the Vigilante’s main armament was carried in an unusual internal "linear bomb bay" between the engines in the rear fuselage, which allowed the bomb to be dropped at supersonic speeds. The single nuclear weapon, commonly the Mk 28 bomb, was attached to two disposable fuel tanks in the cylindrical bay in an assembly known as the "stores train". A set of extendable fins was attached to the aft end of the most rearward fuel tank. These fuel tanks were to be emptied during the flight to the target and then jettisoned with the bomb by an explosive drogue gun. The stores train was propelled rearward at about 50 feet (15 m) per second (30 knots) relative to the aircraft. It then followed a ballistic path.
The Vigilante originally had two wing pylons, intended primarily for drop tanks. The second Vigilante variant, the A3J-2 (A-5B), incorporated internal tanks for an additional 460 gallons of fuel, which added a pronounced dorsal "hump", along with two additional wing hardpoints, for a total of four. Other improvements included blown flaps on the leading edge of the wing, changes to the air intakes and stronger landing gear.
The reconnaissance version of the Vigilante, the RA-5C, was based on the A-5B airframe and had slightly greater wing area and added a long canoe-shaped fairing under the fuselage for a multi-sensor reconnaissance pack. This added an APD-7 side-looking airborne radar (SLAR), AAS-21 infrared line scanner, and camera packs, as well as improved electronic countermeasures. An AN/ALQ-61 electronic intelligence system could also be carried. The RA-5C retained the AN/ASB-12 bombing system, and could, in theory, carry weapons, although it never did in service. Later-built RA-5Cs had more powerful J79-10 engines with afterburning thrust of 17,900 lbf (80 kN), the same engines as the Navy’s F-4J Phantom IIs. The reconnaissance Vigilante weighed almost five tons more than the strike version with almost the same thrust and an only modestly enlarged wing. These changes reduced its acceleration and climb rate, though it remained fast in level flight and was still fully carrier-capable.
The last Vigilante version to be developed from 1964 on and to enter service in 1966 was the EA-5D, a dedicated electronic reconnaissance and electronic warfare version, again replacing respective A-3 Skywarrior variants. With the initial experience from the Vietnam conflict, the EA-5D was primarily conceived as a fast escort for supersonic strike aircraft – namely the USN’s F-4 Phantom IIs which progressively took over more strike missions and direly needed protection from SAMs that could keep up with them during their dangerous missions over enemy territory.
The EA-5D, which was unofficially nicknamed “Electric Vigilante”, “Eva” or simply “E-V” by its crews, was based on the late RA-5C’s airframe and was easily distinguishable through its fairing at the top of the fin which contained the electronics for a Bunker-Ramo AN/ALQ-86 ECM suite. It carried ECM gear in the linear bomb bay and a 16 feet (4.9 m) long canoe-shaped ventral fairing (looking like a shortened but deeper version of the RA-5C’s camera and SLAR installation), plus a heat exchanger, a non-jettisonable auxiliary tank and AN/ALE-41 chaff dispensers in an extended tail cone. The complete installation weighed some 6,000 pounds (2,700 kg). Receivers were installed in a fin-tip pod, or "football", like that of the contemporary EA-6A. This fin array caused some lateral instability, though, which could be compensated with a pair of fins under the rear fuselage.
Like the RA-5C, the EA-5D retained the AN/ASB-12 bombing system and was – in theory – like its recce sibling capable to carry out strike missions, but this never happened either. The EA-5Ds were furthermore equipped with an AN/APQ-129 fire control radar, making the aircraft capable of SEAD missions and of firing the AGM-45 “Shrike” anti-radiation missile, although they were apparently never used in that offensive role. Up to four ram-air turbine powered ALQ-76 countermeasures pods could be carried on the underwing hardpoints, augmenting the internal AN/ALQ-86 system’s bandwidth and jamming power. To improve survivability the EA-5D was furthermore outfitted with a pair of launch rails, mounted as sub-pylons on the outsides of the outer underwing hardpoints. Each could carry a single IR-guided AIM-9 Sidewinder AAM.
Despite the Vigilante's useful service as reconnaissance and ECM platform, it was expensive and complex to operate and occupied significant amounts of precious flight and hangar deck space aboard both conventional and nuclear-powered aircraft carriers at a time when carrier air wings, with the introduction of the F-14 Tomcat and S-3 Viking, were averaging 90 aircraft, many of which were larger than their predecessors. Moreover, the Vigilante did not end the career of the A-3 Skywarrior, which would carry on as photo reconnaissance aircraft, electronic warfare platforms, aerial refueling tankers, and executive transport aircraft designated as RA-3A/B, EA-3A/B, ERA-3B, EKA-3B, KA-3B, and VA-3B, into the early 1990s.
Only 28 EA-5Ds were built (two prototypes, 15 new-build, and 11 conversions from existing A-5A and RA-5C airframes) and the United States remained the only operator of the type. The EA-5D saw extensive use in Vietnam and seven machines were lost (four to SAMs, one to a VPAF MiG-21 and two through accidents), but after the end of hostilities and massive reductions of military expenses the EA-5D was quickly phased out from frontline service in the late 1970s, after an active career of just twelve years. In service it was replaced by the subsonic but much more potent EA-6B “Prowler”, which was based on the carrier-capable A-6 “Intruder” bomber, primarily to reduce the number of types in the USN’s arsenal and therewith operating costs and complexity. Since the EA-6B offered much higher ECM capabilities, the small EA-5D fleet was never upgraded, e. g. with the 2nd generation AGM-78 “Standard” ARM or the AN/ALQ-99 ECM pods.
However, a handful of “Electric Vigilantes” remained active with VAQ-137 (“Rooks”) until the late Eighties – long enough to receive the USN’s new tactical low-visibility paint scheme. These EA-5Ds were operated from land-bases only, not assigned to a Carrier Air Group, with a dedicated tail code (“KW”) to reflect this special status. They acted primarily as electronic aggressor aircraft but were also used to simulate supersonic cruise missiles like the contemporary Soviet Kh-20 (AS-3 “Kangaroo”) or Kh-22 (AS-4 “Kennel”) against land and sea targets during training and naval NATO maneuvers. Thanks to their size, speed and flight characteristics the aircraft were also employed as supersonic bomber aggressors, mimicking Soviet Tu-22s or Su-24s. Most of the Evas therefore received more or less authentic temporary Red Star decorations on their fins, which were, however, rarely overpainted after training missions and became part of the “standard markings”.
In 1987 the machines were finally retired, their airframes had reached their structural limit and maintenance costs of the complex aircraft had become prohibitive. They were in the electronic aggressor role eventually replaced with subsonic and much more economical EA-7L Corsair IIs.
General characteristics:
Crew: 2
Length: 76 ft 6 in (23.32 m)
Wingspan: 53 ft 0 in (16.16 m)
Height: 19 ft 5 in (5.91 m)
Wing area: 701 sq ft (65.1 m)
Empty weight: 32,783 lb (14,870 kg)
Gross weight: 47,631 lb (21,605 kg)
Max takeoff weight: 63,085 lb (28,615 kg)
Fuel capacity: 2,805 US gal (10,618 L; 2,336 imp gal) internal
or 19,074 lb (8,652 kg) of JP-5,
or 24,514 lb (11,119 kg) with 2 × 400 US gal external tanks
Powerplant:
2× General Electric J79-GE-10 after-burning turbojet engines,
10,900 lbf (48 kN) thrust each dry, 17,900 lbf (80 kN) with afterburner
Performance:
Maximum speed: 1,322 mph (Mach 2, 1,149 kn, 2,128 km/h) at 40,000 ft (12,000 m)
Combat range: 974 nmi (1,121 mi, 1,804 km)
Ferry range: 1,571 nmi (1,808 mi, 2,909 km)
Service ceiling: 52,100 ft (15,900 m)
g limits: +5
Rate of climb: 33,900 ft/min (172 m/s)
Wing loading: 80.4 lb/sq ft (393 kg/m2)
Thrust/weight: 0.72
Armament:
4x underwings pylons, each with a load capability of up to 2.000 lb (950 kg),
typically occupied with 400 US gal drop tanks or ALQ-76 Tactical Jamming System (TJS)
ECM pods. Other potential loads: AN/ALE-43(V)1&4 Bulk Chaff Dispensing System pod,
a single AN/AAQ-28(V) Litening targeting pod or AGM-45 Shrike anti-radar missiles
2x launch rails for defensive AIM-9 Sidewinder AAMs on the outer pylons
The kit and its assembly:
This what-if project had been lingering for a long time in the back of my mind, and I shoved it a side for years because of the model’s sheer size that eats up a lot of display space – even though I had the hardware already stashed away, collecting dust. While the build was rather inspired by its livery (see below) I wondered why the Vigilante, an elegant and impressive aircraft, had not been adapted to the ECM role? The concept of a supersonic penetrator/protector aircraft was realized by the USAF with the EF-111A Raven, but in the Vigilante’s time frame, the Vietnam War, esp. its end phase, an escort for fast USN attack aircraft might have made sense, so that I tried to mate the RA-5C with contemporary ECM technology and typical details – and the result became the fictional EA-5D.
With this idea the model became only a conversion of a basic airframe, not a spectacular kitbashing. Since I knew the Hasegawa RA-5C and its underwhelming quality/detail, I settled for the Trumpeter kit – a MUCH better but also a bit über-complicated offering. It is, however, better in any respect, even though you can ask why the cockpit has to consist of no less than thirty (!) parts (including seats and dashboard films), and the pylons as well as even the thin stabilizers and the fin have to consist of halves? One can also wonder why the kit comes with four(!) free-fall nukes but none of the RA-5C’s typical 400 gallon drop tanks? The kit features the type’s underwing flare dispensers, though. If there is something to criticize it’s the lack of air intake ducts – behind the wedge-shaped intakes and their ramps there is nothing inside the fuselage. Since I did not want to put too much effort into that flaw I simple blocked sight into the model’s body with a bulkhead made from black foamed styrene.
Everything goes together quite well, except for the fuselage halves which appear somewhat warped, and the rather massive plastic makes work easy. Despite this splendor of material, the sandwich leading and trailing edges are surprisingly thin and look pretty good.
While the RA-5C was at its core built OOB there were – naturally – some external mods to convey its ECM role. Most obvious detail is the fin top fairing, procured from a KiTech EA-6B, a shabby copy of the Hasegawa kit. This also provided the ECM pods and the pair of voluminous drop tanks.
The retrofitted Sidewinder launch rails on the outer pylons came from an Emhar FJ-4B, the then-state-of-the-art all-aspect AIM-9Ls came from a Hasegawa F-4 kit. To emphasize its electronic mission I added some antenna fairings around the hull. Beyond the fin pod, the EA-5D received sensor fairings along the flanks, inspired by the USAF F-105Gs’arrangement along the bomb bay, a shallow dorsal bulge behind the cockpits and some blister and blade antennae all around the hull.
The large ventral fairing that replaced the RA-5C’s “camera canoe” was scratched from a drop tank half, from a chunky Kangnam MiG-31, in an attempt to create something that the reminds of the EF-111’s arrangement. A ventral adapter for a display holder was integrated into the hull, too, for in-flight scenes.
A pair of long stabilizer fins was added under the rear fuselage, too, because I think that the large tail fin pod could somewhat hamper directional stability… The consist of rotor blades from a Matchbox SA.360 Dauphin helicopter.
The Vigilante’s tail cone, the former fairing for the linear bomb bay between the engines, was also heavily modified, with a thimble-shaped radome and a separate fairing for an internal chaff dispenser underneath, for a different look. To make the model look a bit more lively, esp. in its all-grey low-viz livery (see below) I mounted the flaps (all six are separate elements, and the inner pairs consist of lower and upper halves, too!) in lowered position.
Painting and markings:
The original reason to build this whiffy Vigilante was to see how the sleek and elegant aircraft would look in early USN low-viz colors! With this idea in mind the scheme was improvised and very simple: FS 36320 on the upper surfaces and FS 36375 underneath (Humbrol 128 and 127, respectively), on the flanks (with a relatively high waterline) and the fin. A slightly darker blue grey (FS 35237, Humbrol 145) was used for an anti-glare panel in front of the windshield. Most di-electric panels and the nose radome were painted in brownish light grey (RAL 7032, Revell 75), for low contrast but a significantly different color.
Inside, the landing gear as well as the air intakes were painted gloss white, the cockpit was painted in neutral grey (FS 36231) with dark grey ejection seats. The latter appears a bit tone-in-tone with the all-grey outside, but that was apparently the A-5’s interior design in real life.
To add some variety to the grey livery I painted the ordnance in “old” USN colors: the drop tanks became all-white and the ECM pods also received a white base. The AIM-9Ls on the extra launch rails (also painted white) received blue bodies as training missiles, with black seeker heads and white tail fins.
The wings’ leading edges (bare steel?) were masked and then painted with Revell 91 (iron metallic).
The whole model received a washing with thinned black ink to emphasize the many recessed rivets and panel lines, and then I added panel counter shading with lighter basic tones, also trying to create a slightly worn/weathered and not-so-uniform finish on the large grey surfaces, which underline the Vigilante’s elegant lines but also look quite boring, due to the sheer size/area, esp. from above.
The low-viz markings were improvised and puzzled together from various sources. The Red Stars on the fin were inspired by real-world aggressor markings, AFAIK some A-7Ls, EA-3Bs and A-4Fs carried such decorations, even paired with large bort numbers on the nose.
To improve the worn/grimy look I also treated the model’s surfaces with grinded graphite – only lightly, but I wanted to make the large grey areas to look even more diverse than just with the initial paint effects.