Download Wind Of Glory Part 2

Vestas Wind Systems, the Danish wind turbine company, keeps these vast installations spinning longer using a digital repository for faster, more accurate part production, as Stephen Holmes reports

Having completed its first commercial design in 1979, Denmark-based Vestas has focused exclusively on turbine production since 1989. It has designed, manufactured, installed and serviced more wind turbines across the globe than any other company.

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Similar issues are found with the lightning tip receptors that are added to each wind turbine, to help reduce lightning-strike damage. These receptors are machined from aluminium and as a result might take up to 12 weeks to be delivered.

In 2022, they hope to introduce on-demand gauge production at all manufacturing locations. The company has also partnered with Wrth to build an additive ecosystem and manage an inventory of spare parts made with the Markforged Digital Forge platform to support maintenance, repair and operations (MRO) for local field support and other suppliers.

The company is making it easier for staff with the right permissions to scan a part code or search for a part in its EAM and ERP systems, and have it automatically sent to the required 3D printer. It is hoped that this centralised control, managed using its Blacksmith and Eiger Fleet, will produce high-quality, high-performing tools and end-use parts, keeping Vestas turbines turning and green energy flowing.

The internet wasn't particularly kind to the rules but the figures, as are all figures from West Wind and Old Glory, are rotten with charm and character and this blog celebrates them every chance I get. This entry though is about my build of the fencing/gate portions. I built mine to be 12"x18" of fenced in area. Not big enough to even enclose all the mausoleums!

The wind is, of course, an important factor is sailing, and in Sails of Glory. In the basic game, the wind has a fixed direction, to make things easier for new Captains. To keep track of this direction, the players have at their disposal the wind indicator, placed on a side of the gaming table with its arrow indicating the direction of the wind. In the advanced rules, the wind may shift, allowing for more engaging and realistic battles!

After the ship has been moved, the maneuver card is placed back in your maneuver deck. During the game, you have to pay attention to your movements - If any part of a ship base exits the game field after a maneuver, the ship is eliminated and counts as surrendered.

The Morning Glory is often accompanied by sudden wind squalls, intense low-level wind shear, a rapid increase in the vertical displacement of air parcels, and a sharp pressure jump at the surface.[5] Cloud is continuously formed at the leading edge while being eroded at the trailing edge.[4] Showers or thunderstorms may develop in its wake. In the front of the cloud, there is strong vertical motion that transports air up through the cloud and creates the rolling appearance, while the air in the middle and rear of the cloud becomes turbulent and sinks. The cloud quickly dissipates over land where the air is drier.[3]

One of the main contributors for the formation of the morning glory clouds is the mesoscale circulations associated with a difference in sea breezes that develop over the Peninsula and the Gulf. On the large scale, Morning Glories are usually associated with frontal systems crossing central Australia and high pressure in northern Australia. Locals have noted that the Morning Glory is likely to occur when the humidity in the area is high, which provides moisture for the cloud to form, and when strong sea breezes have blown the preceding day.[8]

Local weather lore in the area suggests that when the fridges frost over and the caf tables' corners curl upwards at the Burketown Pub, there is enough moisture in the air for the clouds to form. Reportedly, all winds cease at ground level as the cloud passes over.[9]

Although the Morning Glory clouds over the southern part of the Gulf of Carpentaria are the most frequent and predictable, similar phenomena have occasionally been observed elsewhere, e.g., over central United States, in the English Channel, Munich,[4] Berlin, eastern Russia, and other maritime regions of Australia. There was one distinct and well formed roll cloud observed spanning from horizon to horizon (east to west), just prior to midnight on 22 October 2015 at 50.3044N, 96.9692W (about 35 km North of Winnipeg, Manitoba, Canada), followed up by a series of them (but much less distinctive) shortly after midnight on 24 October 2015.[citation needed] There was another rare roll cloud formation that was observed in Masury, Ohio, 41.211168N, -80.537849W, on 27 May 2012, at 2:30 pm EST. This rare cloud event was observed by a mother and daughter, who also reported that high winds accompanied this formation, immediately after it being observed. Considering the rarity of the event in this region, it is seen as a once in a lifetime occurrence.[citation needed]

To celebrate the release of The Glory, Part Two, on March 10, writer Kim Eun-sook, Director Ahn Gil-ho, plus actors Song Hye-kyo, Jung Sung-il, Cha Joo-young, Kim Hieora and Kim Gun-woo took part in a press conference, where they responded to questions about the first part of the series and what the second part might feature.

Actress Song Hye-kyo, who previously starred in That Winter The Wind Blows, Descendants of the Sun, Encounter and Now We Are Breaking Up, spoke about how nervous she was before the first part of the series was released and how long it has taken for the success of the series to sink in.

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Morning Glory is the name given to a spectacular cloud formation that occurs in the Gulf of Carpentaria region of northeastern Australia. It is composed of a low roll cloud or often a succession of roll clouds, sometimes stretching from horizon to horizon. The clouds are seen early in the morning, most frequently towards the end of the late dry season from early September to about mid-November. They are typically 1 or 2 km in width, 1 km deep, and may be 100 km or more long, with cloud bases often no more than 100 or 200 m high. Occasionally they are preceded over land by a shallow layer of fog that they rapidly disperse. They move rapidly across the sky at speeds of 10-15 m s-1, the most usual direction being toward the southwest, although cloud lines orientated approximately east-west and moving from the south are sometimes observed. The passage of each cloud overhead is usually accompanied by the onset of a sudden wind squall which, although normally of short duration (perhaps 5 to 10 minutes), have wind speeds comparable to the speed of the cloud. The disturbance brings about also an abrupt rise in surface pressure (sometimes more than 1 mb in a few minutes and a reversal in surface wind direction. The surface pressure may oscillate following the rise, but the increased mean pressure and change in wind direction frequently persist for at least several hours. Some examples are shown in Figure 1. A typical surface pressure trace is shown in Fig. 2.

Anthropologist Dr. Margaret Moore told us that the name of the phenomenon in the language of the Garrawa Aboriginal people who live near the south coast of the Gulf is "kangolgi" and it is credited with increasing the supply of bird life. This may reflect the fact that the morning glory occurs most frequently in October, just prior to the "wet" season, which is a harbinger of bounty for the Aborigines.

The earliest published description of the morning glory that we are aware of is in the Royal Australian Air Force (1942, Part 2, p. 25), where it is described as a "land breeze" coming out of the east about dawn with a squally onset and with one or several long straight lines of low cloud. Thirty years later, Clarke (1972) explored the possibility that the phenomenon could be interpreted as a propagating internal hydraulic jump, formed at a discontinuity in the slope of the ground, on a katabatic flow developing on Cape York Peninsula. Clarke's theory was inevitably tentative, since the only available data against which it could be compared were a series of autographic records of surface pressure, wind and temperature at the (now abandoned) weather station at Karumba. Moreover the theory did not take account of the strong heating contrasts between sea and land in the Gulf region. In fact, there appeared to be the possibility that local sea breeze circulations might be a more important influence than the katabatic flow.

A climatology of pressure jumps was presented also, showing frequencies of occurrence at the five stations in terms of time of day and month, and mean synoptic mean sea level isobaric charts for pressure jump days and for days free of jumps. The latter were classified according to whether surface winds were southeasterly or northeasterly in the southeast gulf area. However, the isobars for northeasterly days without jumps are virtually indistinguishable from those with jumps. In October 1978, Dr. Reg Clarke, a former research scientist with the then CSIRO Division of Atmospheric Physics, and his wife, Elsje, staged a small expedition to the gulf with a view to collecting more detailed surface data on morning glories as well as photographs and time-lapse movie film of the clouds. Ten days were spent in the field during which time four glories were observed, a frequency which, coincidentally, corresponded with the average frequency of presumed morning glories at Karumba in October, based on nine years of data (Neal et al. 1977: see below). Two of these four occurred before daybreak; one was cloud-free; two had five parallel cloud bands and the other three. All had marked wind and pressure jumps. One was followed by car over 35 km and its speed measured at 11 m s-1; another was photographed in time-lapse which revealed a rolling motion of the cloud band with upward motion at the leading edge and downward motion at the rear. In each case, measurements of surface pressure, temperature, humidity and wind were made during the passage of the disturbance. e24fc04721