LOS ANGELES - Most car dealers like to be as specific as possible when describing store location in their tiffany money clips, using lines such as: "We're situated where the 405 and 5 collide."

But for The Auto Gallery Audi in Canoga Park, Calif., it's more like: "Go in the back way at Neiman Marcus and hang a left at women's handbags. "

The Auto Gallery chose to locate its Audi showroom inside Westfield Topanga, an upscale shopping mall in the San Fernando Valley, until a permanent store is erected a mile away on Ventura Boulevard.

Both financially and logistically, that made better sense than working out of a double-wide trailer while construction equipment roared nearby. In fact, it has worked out so well since the store opened in December that Auto Gallery's principals are considering keeping the mall store as a satellite sales center after the $10 million Audi dealership opens in August.

"The facility we had was dreadful; people didn't even know it was an Audi dealership," said Tony Schwartz, co-Tiffany Money Clips of Auto Gallery, which also sells Porsche, Maserati, Ferrari and Lamborghini. "But we had been waiting seven years for permits [for a new dealership] . We had to find an alternative."

Schwartz, who is careful to refer to the mall location as "a showroom, not a facility," said the rent is not inexpensive but is cheaper than operating out of a trailer at a street location.

Breakfast at Audi?

Schwartz was wowed by the demographics of potential customers roaming the mall, where 14 million shoppers a year walk tiffany money clips the corridor of elite storefronts that include Tiffany, Cartier, Louis Vuitton and Salvatore Ferragamo.

The mall also brings more shoppers from outside the area than would normally visit a car dealership. The shopping center previously displayed Audis in its walkways. But the relationship expanded when prime retail space opened next to Neiman Marcus.

Usually, five or six Audis are displayed in the 5,700-square-foot showroom. The aim is to represent each Audi vehicle. But tiffany money clips Topanga has dedicated a big chunk of the covered parking structure to the rest of the vehicles in inventory, which are brought around by a porter for test drives.

"The showrooms make an exciting and progressive addition to the luxury wing of Westfield Topanga," said Erick Klaster, senior general manager of Westfield Topanga and Promenade.

The Auto Gallery Audi is a salesready environment, complete with an accessories area. The back door of the showroom leads shoppers to the valet parking circle, where cars are delivered for test drives. But the pitch is definitely lower-key than at a traditional dealership.

"People just trip over us here," said Lonnie Decker, chief marketing officer for The Auto Gallery. "We are planting seeds with people who haven't put Audi on their shopping list. They may not be in purchase mode now, but we can get their contact information now."

The Auto Gallery also has a Lamborghini showroom next door to Audi in the mall. The Lambo outlet, which is 3,800 tiffany money clips feet, will stay even if the Audi showroom doesn't.

"It will be a permanent location for at least the next several years," Schwartz said. "It's a destination showroom, and we don't have to pay for bricks and mortar."

Most visitors to the Lamborghini showroom just want to gawk, although Schwartz said the store has a slightly more liberal test-drive policy than most exotic dealerships. But for most people, the dealership is a place to purchase Lamborghini logo merchandise, such as backpacks, T-shirts and baseball caps.

Not that the Westfield Topanga Audi showroom isn't selling cars.

The store's previous Audi store, at the Ventura Boulevard location, typically sold 50 new vehicles and 20 used vehicles a month. In the shopping center it's more like 40 new and 20 used, but that's in a down economy. The new store on Ventura is expected to sell 70 to 80 new vehicles and 30 to 40 used ones.

Vince Scandone, Audi's Los Angeles area general manager, said the benefits outweigh the difficulties.

"It's not a traditional path" for car buyers, Scandone said. "You don't get die drive-by. You don't have a usedcar display. You don't have the curb appeal. But you do get the benefits of shoppers who wouldn't go into an Audi dealership, and die next thing you know Audi is now on their list."

Operating out of a mall makes for some logistical, storage and insurance issues. Scandone admits Audi would not approve the shopping center location as a long-term home. But as a temporary solution, it has worked.

An added benefit: The mall's parking lot provides an excellent gathering place for "Supercar Sunday," a get-together of Audi gearheads and their cars sponsored by the dealership. Some Sundays the event attracts as many as 1,000 people, many of whom then wander over to the showroom.

And if the rest of the family is bored, there are countless other stores where they can pass the time. Decker says: "They can make a day of it."

When the lid is lowered and momentum is not conserved, the stratospheric basic state, variability, planetary wave 1 structure, and the blocking frequency are all significantly altered. The stratospheric jet is twice as strong as when momentum is conserved and always has significant vertical shear in the lower stratosphere. The wave 1 amplitude is very large in the vicinity of the model lid, particularly over the polar cap. There is also a significant decrease in the blocking frequency in the Euro-Atlantic sector and a large increase in the Pacific sector, which are consistent with the tiffany bangles in the tropospheric planetary wave structure. The impact of a strong stratospheric jet and low model lid height on planetary waves and blocking had been reported by previous authors (Boville 1984, 1986; Boville and Cheng 1988). It is shown here, however, that momentum conservation has a large impact that is much larger than the model lid height. The wave propagation characteristics also change significantly when momentum is not conserved: the correlation coefficients for both the upwardand downward-propagating patterns increase significantly. There is much more coherent downward propagation of wave 1 in the low-lid nonconservative configuration than in either the low- or high-hd conservative configurations. The increased amount of wave reflection is confirmed by a large increase in negative wave 1 heat flux values at both 100 and 10 hPa. The lack of wave 1 damping near the lid leads to a much stronger stratospheric jet and results in an increase in wave reflection off the model lid. Finally, the stratosphere-troposphere coupling is dominated by wave-reflection-type coupling according to the time-lagged NAM correlations.

There is no downward progression of NAM anomalies. The time scale of the zonal wind SSW event is much faster and the Tiffany Bangles wind remains large even after the event. Nonconservation leads to a significant decrease in the number of SSW events (by a factor of 4). The NAM time scales in both the troposphere and stratosphere are larger than in the other model configurations, and the seasonal cycle in the troposphere has two maxima instead of one. Overall, the excess wave reflection in the low-lid nonconservative configuration negatively impacts the climate, leading to a very strong and more persistent stratospheric jet that is not easily perturbed and more reminiscent of the Southern Hemisphere jet.

Our analysis suggests the stratospheric model configuration of a climate model must conserve gravity wave momentum flux and have a high enough model lid (and vertical resolution) to properly model planetary waves and their interaction with the zonal-mean flow (both wave dissipation and wave reflection) in Northern Hemisphere winter. If the model lid of a climate model is placed too low, then it acts as a reflecting surface for the upward-propagating planetary waves. Both low-lid configurations examined here had an excess of wave reflection, which resulted in too much wave-tiffany bangles-type stratosphere-troposphere coupling. The coupling was improved through the act of conservation since it both reduced the strength of the mean flow and damped the planetary waves near the model lid leading to wave dissipation. In particular, when momentum was conserved in the low-lid model there was a significant improvement in the seasonal cycle of the NAM time scales. The models in the IPCC AR4, which are mostly low-lid models, do not capture the observed seasonal cycle of the NAM time scales (Gerber et al. 2008a). It is possible that nonconservation and poor vertical resolution in the stratosphere contribute to the biases in the NAM time scales. [The low-lid configuration has 20 vertical levels between 300 and 10 hPa, whereas only 3 of the 13 IPCC AR4 models have more than 15 vertical levels between 300 and 10 hPa (Cordero and Forster 2006).] If the model lid of a climate model is placed high enough, above 2 hPa for instance, then it is more likely to have a better representation of planetary wave structure and propagation (as compared to a low-lid climate model), in particular with regard to wave tiffany bangles.

PH03 showed that the reflecting surface in the real atmosphere develops above 10 hPa; however, there is no guarantee that the modeled jet will develop a reflecting surface and, furthermore, that it will have the proper variability. The jet in the high-lid configuration examined here did develop a reflecting surface but it did not have the proper variability. A high lid also does not guarantee the proper coupling to the troposphere: the NAM correlations and the seasonal cycle of the NAM time scale in the troposphere were biased in the high-lid conservative configuration examined here. (Note, however, that a high lid does significantly reduce the errors associated with nonconservation as discussed by S09.) Many chemistry-climate models that are high-lid models also have biases in the tropospheric time scales (Gerber et al. 2010). tiffany bangles how to improve models with deficiencies in wave reflection and its impact on tropospheric time scales requires a better understanding of the coupling between the mean flow and the upwardand downward-propagating planetary waves. The mean flow coupling to the parameterized gravity waves further complicates matters. Recent results by Harnik (2009) suggest that the time duration of the upward pulse of wave activity entering the stratosphere from the troposphere is an important factor determining whether the wave is reflected.

Our analysis focused on Northern Hemisphere winter where the observed structure and propagation characteristics of the planetary waves are well documented. In the Southern Hemisphere the situation is more complicated because a permanent reflecting surface develops toward late winter as part of the seasonal cycle (Harnik and Lindzen 2001). Thus, wave reflection contributes more to the coupling between the stratosphere and troposphere in that hemisphere, which may pose a challenge for the CMAM since it does not capture the reflection in the Northern Hemisphere. Extending the analysis to the Southern Hemisphere is work in progress.

Acknowledgments. This research has been supported by the Natural Sciences and Engineering Research Council of Canada through a Post Doctoral Fellowship to the first author. JP's contribution was funded by the NOAA Climate Program Office. The first author is grateful to Drs. Michael Sigmond and John Scinocca for performing the model simulations, to Drs. Ted Shepherd and Charles McLandress for many helpful discussions, to Dr. Mark Baldwin for providing his EOF code, and to Dr. Ed Gerber for providing his code to calculate the NAM time scales. The authors are also grateful to three anonymous reviewers for helping to improve the manuscript.

We have examined the impact of stratospheric model configuration on planetary wave structure, vertical propagation, and the resulting impact on stratospheretroposphere coupling in Northern Hemisphere winter using the CMAM. The CMAM configurations included a high-lid (0.001 hPa) and a low-lid (10 hPa) configuration that were each run with and tiffany necklaces conservation of parameterized gravity wave momentum flux.

The impact on planetary wave structure was examined using diagnostics of the stratospheric basic state, variability, wave 1 horizontal structure at 500 hPa, blocking frequency, and wave amplitude and phase at all vertical levels. The impact on planetary wave vertical propagation (both upward and downward) was examined using the SVD Tiffany Necklaces of PH03. The upward- and downwardpropagating signals were isolated as maxima of timelagged correlation coefficients of the temporal expansion coefficients of the first coupled mode between zonal wavenumber 1 geopotential data at 500 hPa and data from three different stratospheric levels (50, 30, and 10 hPa). The propagation characteristics were also investigated using histograms of the daily wave 1 heat flux at 100 and 10 hPa averaged between 40° and 9O0N. Finally, the impact on stratosphere-troposphere coupling was examined using time-lagged NAM correlations, SSW composites, and the seasonal cycle of the NAM time scale.

The stratospheric basic state, variability, and planetary wave 1 structure in the high-lid conservative configuration are in good agreement with reanalysis data. The blocking frequency, is biased in its position of the maximum frequency in the Euro-Atlantic sector and in its absolute frequency. The upward-propagating wave 1 pattern and its time scale of propagation are in reasonable agreement with the reanalysis. The high-lid conservative configuration, however, fails to accurately capture the downward propagation of wave 1: it underestimates the magnitude of the tiffany necklaces and the time scale of propagation. The histogram of the daily wave 1 heat flux at 100 and 10 hPa in JFM are in good agreement with the reanalysis. Both zonal-mean- and wave-reflectiontype stratosphere-troposphere coupling contribute to the time-lagged NAM correlations, which is in agreement with the reanalysis. The zonal-mean NAM anomalies take 15 days to reach the surface, which is longer than in the reanalysis. The SSW zonal wind event composite has a reasonable time scale and subsequent recovery. Finally, the seasonal cycle of the NAM time scales in the stratosphere is in good agreement with reanalysis; however, the NAM time scales in the troposphere maximizes in spring instead of winter. The reanalyses show a clear maximum in winter.

When the lid is lowered and momentum is conserved, the stratospheric basic state, variability, planetary wave 1 structure, and the tiffany necklaces frequency are not significantly altered. The upward propagation of wave 1 is also preserved; however, the downward propagation is damped such that no downward-propagation time scale can be estimated. The wave 1 damping arises from a wave 1 projection of the GWD at 10 hPa, which is out of phase with the wave 1 zonal wind pattern and twice as large as in the high-lid conservative configuration. The damping is a direct result of conserving momentum and results in a more compact wave 1 heat flux distribution at 10 hPa as compared to the high-lid conservative configuration. The wave 1 heat flux histogram at 100 hPa remains in good agreement with the reanalysis. There is more wavereflection-type coupling in the time-lagged NAM correlations than in the high-lid conservative configuration. The downward progression of the zonal-mean NAM tiffany necklaces takes 25 days to reach the surface, which is longer than in the high-lid conservative configuration and the reanalysis. The SSW zonal wind composite is in good agreement with both the high-lid conservative configuration and the reanalysis; however, the number of SSW events decreases by a factor of 2. The seasonal cycle of the NAM time scale in the stratosphere and troposphere are reasonable, but the time scales are too large. The maximum tropospheric time scale occurs in winter, which is consistent with the reanalysis.

The impact of the changes in the planetary waves on the stratosphere and troposphere coupling in the different CMAM configurations can be further illustrated by considering stratospheric sudden warming (SSW) events. Following Charlton and Polvani (2007) we define a SSW event as a reversal in sign of the zonal-mean zonal wind at 10 hPa and 600N from November to March. Figure 13 shows composites of the zonal wind at 10 hPa and 6O0N for SSW events in the reanalysis and the CMAM configurations. The reanalyses show a large and fast tiffany key rings-scale decrease in the zonal-mean zonal wind preceding the SSW event with a much slower timescale recovery following the event (Fig. 13 top left). The reanalysis composite is based on the 18 events that occurred during the 30-yr record. The SSW zonal wind composite for HIGH_C is in good agreement with the reanalysis (cf. Fig. 13 top left to top right). The composite is based on the 30 events that occurred in the 40-yr model run. The good agreement between the SSW events in the reanalysis and the CMAM model in its standard high-lid configuration was highlighted recently by McLandress and Shepherd (2009). When the lid is lowered and momentum is conserved, the zonal wind composite is slightly distorted (Fig. 13 bottom left). There is a suggestion that the time scale of recovery is decreased when the lid is lowered. The composite is based on only 15 events (the number of events is reduced by half when the lid is lowered).

When momentum is not conserved, the zonal wind SSW composite is completely distorted (Fig. 13 bottom right). There is a clear increase in the time scale of both the decrease in zonal wind preceding the event and its subsequent recovery. The faster time-scale recovery is consistent with the lack of downward progression of NAM Tiffany Key Rings (Fig. 12 bottom right). There is also no decrease in the zonal wind following the event, as seen in the reanalysis. It is possible that the SSW events in LOW_N involve the displacement of the stratospheric jet off the pole rather than the destruction of the jet and its subsequent recovery. There is also a further reduction in the number of SSW events when momentum is not conserved (there are only 8 events in LOW_N). Sassi et al. (2010) also noted a distortion in the time scale and number of SSW events in their low-lid mean sea level pressure SSW composite as compared to their high-lid composite; however, they did not state whether their model was conservative.

Finally, the seasonal cycle of the coupling, as measured by the seasonal cycle of the NAM time scale, in the reanalysis and the different CMAM configurations is shown in Fig. 14. Using reanalysis data from 1958 to 2002, Baldwin et al. (2003) showed that the observed lower-stratospheric and tropospheric NAM time-scale tiffany key rings are coincident in the Northern Hemisphere during December, January, and February (DJF), indicating strong stratosphere-troposphere coupling during that time. More recently, Gerber et al. (2008a) analyzed the Intergovernmental Panel on Climate Change (IPCC) Fourth Assessment Report (AR4) models and showed that they have large biases in the seasonal cycle of the NAM time scale in the troposphere in the Northern Hemisphere. The models in the IPCC AR4 are predominantly low-lid models (Cordero and Forster 2006). The observed seasonal cycle of the NAM time scale for 1979-2008 shows a maximum in the troposphere during DJF (Fig. 14 top left). The time scales are slightly different from Baldwin et al. (2003) and Gerber et al. (2008a), because we have excluded years before 1979 in the current analysis. The maximum time scale in the troposphere occurs in DJF and is approximately 13 days. The maximum time scale in the lower stratosphere also occurs in DJF and is 30 days. (The largest time scales in the stratosphere occur in summer; however, the variance in the NAM during that time is minimal.) The tiffany key rings configuration shows good agreement with the reanalysis in the stratosphere with a maximum time scale in the lower stratosphere in DJF of 30 days (Fig. 14 top right). The maximum time scale in the troposphere is larger than in the reanalysis and occurs in spring instead of winter.

Overall, the HIGH_C time scales lie within the range of uncertainty of the reanalysis time scales with the exception of the tropospheric maximum in spring.2 (Note that the seasonal cycle of the time scales in all the CMAM configurations are found to be robust when 20-yr subsamples are considered, however the magnitude of the time scales vary slightly.) When the lid is lowered and momentum is conserved, the maximum stratospheric time scale in winter increases slightly (Fig. 14 bottom left). In the troposphere the maximum time scale also increases and is shifted from spring to winter. Overall, LOW_C shows good agreement with the reanalysis in terms of the seasonal cycle in both the stratosphere and troposphere; however, the time scales are too large in winter. In particular, the tiffany key rings time scale in winter is outside the range of uncertainty of the reanalysis time scale. When momentum is not conserved the time scales are severely altered (Fig. 14 bottom right). The maximum stratospheric time scale increases by a factor of 3 and is more reminiscent of those observed for the southern annular mode (see Fig. IB from Baldwin et al. 2003). In the troposphere there are two maxima that occur in early winter and late winter/early spring, respectively. Both the tropospheric and stratospheric timescale maxima are outside the range of uncertainty of the reanalysis time scale. The increase in maximum time scale in the stratosphere in winter between LOW_C and LOW_N is consistent with the previous results: nonconservation results in a very strong stratospheric jet that is more persistent and hence not easily perturbed (i.e., there are fewer SSW events). Note that the differences in time scales between the CMAM configurations likely reflect differences in the interannual variability (Keeley et al. 2009) and stratosphere-troposphere coupling is one source of this variability.

Following Baldwin and Dunkerton (2001) and PH04 we calculate time-lagged correlations of the NAM signature time series at 10 hPa with all other levels for all years. The daily unfiltered NAM time series was calculated using the zonal-mean NAM according to Baldwin and Thompson (2009) for all JFM periods. The NAMs are in good tiffany earrings in the troposphere (not shown). In the stratosphere the NAMs are in good agreement, with the exception of LOW_N, which has much larger amplitude toward the pole (not shown) and is consistent with its stratospheric jet being much stronger than the jets in HIGH_C and LOW_C (see Fig. 1).

Figure 12 shows the correlation coefficient for the NAM signature time series at 10 hPa with all other levels for time lags between -40 and 40 days for the reanalysis and the different CMAM configurations. The reanalysis correlation shows a clear downward progression of a positive anomaly from the stratosphere that reaches the surface 10-30 days later (Fig. 12 top left). There are also high correlation values near lag zero in the stratosphere that do not extend into the troposphere and a clear vacillation of the correlation sign on an intraseasonal time scale. The results differ slightly from PH04 (see their Fig. 4a) because we have included seven more years of reanalysis data. PH04 found that years with strong zonal-mean-type coupling showed a clear downward progression of NAM Tiffany Earrings toward the surface, while years with strong wave-reflection-type coupling had no downward coupling and the correlations peaked near zero time lag. The reanalyses show features of both zonal-mean- and wave-reflection-type coupling, as noted by PH04.

The HIGH_C configuration shows a similar downward progression of NAM anomalies and high correlation values near lag zero (Fig. 12 top right). There is, however, a delay in the downward progression into the troposphere: the maximum surface correlation occurs between 20 and 40 days. HIGH_C also captures the vacillation in the stratosphere and the phase transition from negative to positive at the surface near zero lag seen in the reanalysis. When the lid is lowered and momentum is conserved, the downward progression seen in HIGH_C is distorted (Fig. 12 bottom left). The tiffany earrings correlation values occur near day zero and, while there is some downward progression of the positive anomaly, it reaches the surface later than in HIGH_C (approximately 10 days later). The vacillation in the stratosphere is also weaker and there is no longer a phase transition at the surface. The high correlation values near zero lag suggest that there is more wave-reflection-type coupling in LOW_C than in HIGH_C The wave-mean flow interaction processes that lead to the downward progression of the zonal-mean anomalies in HIGH-C are clearly altered by the low lid in combination with momentum conservation. When momentum is not conserved there are further changes to the coupling. In particular the correlations become very large near zero lag and there is no longer any indication of a downward progression on intraseasonal time scales (Fig. 12 bottom right). The tiffany earrings correlation values near zero lag and lack of downward progression suggest that the coupling in LOW_N is dominated by wave-reflection-type coupling, which is tiffany earrings with the analysis in previous sections. It is clear that while momentum conservation improves the coupling it cannot entirely eliminate the negative effects of a low lid on the planetary waves.

It's 3 P.M. on a gorgeous sunny day in Los Angeles, and Amanda Seyfried is sitting at an outdoor caf, wearing a light-blue long-sleeve button-down and shorts, her signature glamorously wavy blond hair peeking out from a mustard-yellow cable-knit cap that she made herself. In a bag on the shop for tiffany accessories table is a DIY dog-collar kit for Finn, her blue-eyed Australian shepherd who lies lazily at her feet. The actress isn't hiding under huge sunglasses, sitting in a dark corner, or ignoring the passersby who stop to pet her adorable pup. (In fact, she's chatting them up, making it difficult for anyone to get a word in edgewise.)

Amanda is the rare young star who has managed to continue to thrive in Hollywood despite having no background in anything remotely Disney or Nickelodeon, and in case you haven't noticed, she's having a moment. In the past year, the 24-year-old actress from Allentown, Pennsylvania, has hit a movie genre trifecta Dear John, a Nicholas Sparks tearjerker; Chloe, an indie thriller; and this month's rom-com Letters to Juliet. And beyond the occasional red carpet and the Oscars, where she presented alongside Miley Cyrus, the paparazzi have generally left her alone. The closest they've gotten are a few snaps of the actress with beau (and Mamma Mia! costar) shop for tiffany bracelets Dominic Cooper, although one guy was daring enough to follow Amanda and Finn on a recent six-mile hike.

I don't really care about paparazzi like, I'm not wearing makeup right now and I shop for tiffany necklaces should be but when someone follows me around on a day like that, a really wonderful, beautiful day . . . she trails off. Had I known he was there, I would have been really upset. Amanda's going to have to get used to it.

merchandise bags of paper or plastic, paper gift wrap bows, paper ribbons, bottle wrappers of cardboard or paper, plastic bubble packs for wrapping or packaging, sheets of cellulose for wrapping tiffany shopping food for household use, plastic film for wrapping food for household use, wrapping paper, gift wrapping paper, printed note books, printed paper envelopes for use when sending watches or jewelry for repair, paper tags, plastic-coated paper tags, price tags, printed timetables, transfers or decalcomanias, hat boxes of cardboard.

packaging material made of starches in the nature of a paper substitute for food, beverages and consumer products, pencil sharpeners, Charm bracelet stationery folders, posters, calendars, letter openers, writing cases, namely, pen and pencil cases; stands for pens and pencils, passport holders, blotters, pens, pencils, drawing sets consisting of drawing pencils and charcoal pencils, desk-mounted cabinets for stationery, stencil cases; pen cases, pencil cases, rubber erasers; drawing squares and drawing rulers; gummed tape for stationery use, covers of paper for flower pots, book covers, marking chalk, chaplets, modeling paste for stationery or household use

Unworked or semi-worked leather sold in bulk, animal fur-skins, luggage, handbags, shoulder bags, garment bags for travel, traveling bags, beach bags, clutch bags, all purpose sports bags, attach cases, school bags, tote bags, textile Bead bracelet shopping bags; card cases, namely, business card cases; vanity cases not fitted; keycases, knapsacks, rucksacks, briefcases, purses, wallets, pouches of leather for packaging; traveling trunks, suitcases, umbrellas, parasols, walking sticks; dog collars, whips

Electric vegetable slicing machines, electric food milling machines, electric coffee grinders for domestic and commercial use, electrically operated meat grinders, electric food mixers and electric food blenders for domestic use, centrifuges, electric whisks, electric graters, electric juicers for household use, electric fruit and vegetable peelers, electrically operated food processors; pasta rolling machines, pasta cutting silver necklaces machines; electric tin openers, ironing machines for industrial use, dry cleaning machines.

machines for removing all kinds of stains from any kind of fabric by the help of silver pendants steam and pressurized air clothes washing machines, dish washing machines, floor washing machines; electric trouser presses for industrial use, mangles being commercial clothes pressing machines, blades as parts of machines, tables specially adapted to hold powered machinery, electric vacuum cleaners; discs for cutting and burring metals and building materials as parts of machines, ploughs, wood sawing machines, clothes spin dryers, printing presses.

automatic looms, dip-dyeing machines, chemical fiber drying machines, harvest drying machines, sewing machines, knitting machines; machine lasts for making shoes. sand-blasting machines, wine presses silver rings being machines, tobacco processing machines, power-operated polishers, drilling heads being parts of machines, concrete smoothing machines, embossing machines, power-operated potters' wheels, machines for laying asphalt paving, bottle sealing machines for industrial purposes, tube coiling machines, glue scrapers being parts of machines.