COILS
High strength alloy and smaller diameter tubes spell ‘success’
Copper tubes withstand very high pressures in R744 gas coolers and here, Frank Gao, OEM team leader, International Copper Association and Yoram Shabtay, president, Heat Transfer Technologies explain why.
T
here is no doubt that the Earth’s atmosphere would benefi t from ecofriendly refrigeration and air-conditioning
technology. One technology that is poised to grow in the coming years is the use of carbon dioxide as a refrigerant. This technology has been under development for decades and is now commercially feasible as the technology advances for various components, such as compressors, refrigerant lines and gas coolers. A major diff erence between carbon dioxide (R744) and other refrigerants has to do with the very high pressure and relatively high temperatures of the R744 refrigeration cycle. For transcritical refrigeration cycles, operating pressures of 12 MPa (1740 psi) or more are typical. Considering that 0.10 MPa = 0.987 atm = 14.5 psi, a pressure of 12 MPa is about 118 times atmospheric pressure, a very high pressure indeed. By comparison, the discharge pressure for a typical R410A refrigeration cycle is less than one-quarter as high. Furthermore, the transcritical cycle could
involve cooling the CO2 in the gas cooler from well above 100°C down to about 31°C (i.e., from well above 212°F to about 88°F). The critical point for CO2
is 31°C (88°F) and 7.4 MPa (1071 psi).
Above that point, CO2 behaves as a supercritical fl uid (SCF), which has properties between a gas and a liquid. It is very dense, which permits high mass fl ow rates; it also has a very low viscosity, which reduces the inside-the-tube pressure drop.
Compact Coils Since the pressures are 20 September 2019
very much higher for R744 in a gas cooler than for a conventional refrigerant in an air-cooled condenser, special measures are required to withstand these very high pressures. First, copper tubes with small diameters are preferred in gas coolers. As a fi rst approximation for thin-walled tubes, the ‘hoop stress’ equals the internal pressure times the radius of the tube divided by the tube wall thickness. Hence, a 3/8 inch (9.525 mm) tube diameter is large for an R744 gas cooler. Tube diameters of 5/16 inch (7.9375 mm) or 1/4 inch (6.25 mm) are more common.
The hoop stress in the tube drops in the ratio of 6 to 5 to 4 as the diameter is reduced from 6/16 to 5/16 to 4/16 inches, respectively – that is, from 9.525 mm to 7.9375 mm to 6.350 mm. Some coil manufacturers are using copper tube diameters of only 5 mm since such smaller diameter tubes can withstand high internal pressures with thinner walls.
Secondly, tubes made from a high strength copper alloy can withstand higher pressures. Some coil makers successfully use this approach to increase the pressure rating of the coil itself. More commonly, system designers use a high strength copper alloy for the refrigerant lines that run to-and-from the gas cooler. The copper-iron alloy UNS C19400, which contains a small amount of iron, has a yield strength that is more than fi fty percent higher than UNS C12200 copper.
Finally, another way to increase the pressure rating is to increase the tube wall thickness. Doubling the thickness roughly halves the stress in the wall of a tube for a given internal pressure. Conversely, either of the fi rst two approaches – using a smaller diameter tube or a high strength copper alloy – allows one to use thinner tube wall thicknesses. Thin walled tubes of course decrease the cost and the weight of heat exchangers.
www.acr-news.com
Page 1 |
Page 2 |
Page 3 |
Page 4 |
Page 5 |
Page 6 |
Page 7 |
Page 8 |
Page 9 |
Page 10 |
Page 11 |
Page 12 |
Page 13 |
Page 14 |
Page 15 |
Page 16 |
Page 17 |
Page 18 |
Page 19 |
Page 20 |
Page 21 |
Page 22 |
Page 23 |
Page 24 |
Page 25 |
Page 26 |
Page 27 |
Page 28 |
Page 29 |
Page 30 |
Page 31 |
Page 32 |
Page 33 |
Page 34 |
Page 35 |
Page 36 |
Page 37 |
Page 38 |
Page 39 |
Page 40 |
Page 41 |
Page 42 |
Page 43 |
Page 44 |
Page 45 |
Page 46 |
Page 47 |
Page 48 |
Page 49 |
Page 50 |
Page 51 |
Page 52 |
Page 53 |
Page 54 |
Page 55 |
Page 56