Introduction
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When it comes to vacuum gas cooling, various factors come into play. According to search results, "velocity appears to be more vital in enhancing the quenching efficiency of vacuum furnaces" than merely elevating the pressure alone. Our study compared the cooling rates of two differently sized High Pressure Gas Quenching (HPGQ) vacuum furnaces: a large 10-bar vacuum furnace equipped with a 600 HP blower motor versus a smaller 10-bar vacuum furnace equipped with a 300 HP motor. Both furnaces, one with a hot zone of 110 cubic feet and the other with 40 cubic feet, were exclusively engineered and manufactured by Solar Manufacturing located in Sellersville, PA.
High Pressure Gas Quenching in the heat treatment of metals has made remarkable progress over recent years. Varying gas pressures within the chamber have proven to be more manageable than their oil and water quenching counterparts. The primary benefit of gas cooling over liquid cooling remains the dimensional stability of the component being heat-treated. Additionally, using gas as a quench medium dramatically reduces the risk of crack initiation in a component due to temperature differentials during cooling. Gas quenching cools strictly by convection, while the three distinct phases of liquid quenching (vapor, vapor transport, and convection) impart undue stress into the part, causing more distortion (Figure 1).
Multiple variables are involved in optimizing gas cooling. These include furnace design, blower designs, heat exchanger efficiency, gas pressure, gas velocities, cooling water temperatures, the gas species used, and the surface area of the workpieces. When these variables remain constant, the relative gas cooling performance of a vacuum furnace typically increases as the furnace size decreases.
Solar Manufacturing has built multiple high-pressure gas quenching furnaces of varying sizes over the years, ranging from 2 to 20 bar pressure. We have learned that vacuum furnaces rated at 20 bar and above become restrictive in both cost constraints and diminishing cooling improvements. Therefore, Solar Manufacturing engineers began to study gas velocities to improve cooling rates. They determined that increasing the blower fan from 300 horsepower to 600 horsepower, along with other gas flow improvements, would substantially increase metallurgical cooling rates. The technology was reviewed and found to be sound. A 48" wide x 48" high x 96" deep HPGQ 10-bar furnace equipped with this newest technology was purchased by Solar Atmospheres of Western PA located in Hermitage, PA.
Once this new vacuum furnace was installed, a cooling test was immediately conducted. A heavy load was quenched at 10-bar nitrogen in an existing HL 50 sized furnace (36"x 36" x 48"). The same cycle was repeated in the newly designed vacuum furnace, almost three times its size! (See Pictures 1 and 2)
The load chosen for the experiment was 75 steel bars with a 3" OD x 17" OAL, weighing 34 pounds each. The basket and grid system supporting the load weighed 510 pounds. The total weight of the entire load was 3,060 pounds. Both test runs were identically thermocoupled at the four corners and in the load's center. All five thermocouples were deeply inserted (6" deep) into ¼" holes at the end of the bars (See Picture 3). Each load also contained two 1" OD x 6" OAL metallographic test specimens of H13 hot working tool steel. These specimens were placed near the center thermocouple to ensure the "worst case" in terms of quench rate severity. All tests were heated to 1850°F for one hour and 10-bar nitrogen quenched.
The comparative cooling curves between both HPGQ vacuum furnaces are shown in Chart 1. Table 1 reveals that in the critical span of 1850°F to 1250°F for H13 tool steel, the cooling rate in the larger furnace with more horsepower nearly matched the cooling rate of the furnace that was three times smaller in size.
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Micrographs of the H13 test specimens processed in each load were prepared (Pictures 4 & 5). The microstructure of each test specimen is characterized by a predominantly tempered martensitic microstructure with fine, undissolved carbides. The consistency of the microstructure across both trial loads further demonstrates that while the larger furnace utilized the higher horsepower, both resulted in a critical cooling rate sufficient to develop a fully martensitic microstructure.
These tests prove that the most significant impact on the cooling performance in a vacuum furnace is to increase the gas velocity within the chamber. This was primarily achieved by increasing the blower fan's horsepower. By doing this, the ultimate cost to the customer is significantly less than manufacturing a higher pressure coded vessel. This newly designed vacuum furnace has proven to be a game-changer.
Part II of this article will discuss real-life case studies and how both Solar and Solar's customers have mutually benefited from this newest technology.
Written by: Robert Hill, FASM, President, Solar Atmospheres of Western PA
Gregory Scheuring, Plant Metallurgist, Solar Atmospheres of Western PA
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