| 研究生: |
張家豪 Chang, Chia-Hao |
|---|---|
| 論文名稱: |
沃斯田鐵系不銹鋼於CO-H2-H2O氣氛中之金屬塵化現象研究 Metal Dusting Behavior of Austenitic Stainless Steels in CO-H2-H2O Mixed Gases |
| 指導教授: |
蔡文達
Tsai, Wen-Ta |
| 學位類別: |
博士 Doctor |
| 系所名稱: |
工學院 - 材料科學及工程學系 Department of Materials Science and Engineering |
| 論文出版年: | 2011 |
| 畢業學年度: | 99 |
| 語文別: | 中文 |
| 論文頁數: | 113 |
| 中文關鍵詞: | 塵化 、不銹鋼 |
| 外文關鍵詞: | metal dusting, stainless steel |
| 相關次數: | 點閱:91 下載:2 |
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金屬塵化是一種高溫腐蝕現象,主要發生在400~800 ℃的溫度範圍、且含有高碳勢的氣氛環境中,屬於碳化反應的範疇。塵化反應會造成材料發生分解的現象,產生顆粒狀的金屬粉末、氧化物、碳化物及積碳等混合物,在合金表面形成蝕孔。
本研究主要探討多種不銹鋼(304L、310、321及347 SS)於600℃之35 % CO + 60 % H2 + 5 % H2O氣氛環境中,經過長時間曝露試驗後之塵化現象。不銹鋼經過500小時塵化試驗後,試片表面皆可觀察到塵化蝕孔的生成。利用掃瞄式電子顯微鏡(SEM)和穿透式電子顯微鏡(TEM),同時搭配能量質譜分析儀(EDS)進行試片所生成蝕孔之表面及橫截面的微觀組織觀察。蝕孔下方基材區域存在著多種的形貌,最外層為具有石磨結構的積碳區域並有鐵/鎳金屬顆粒鑲嵌其中;而位於基材最上端區域則存在一層以氧化鉻為主的多孔性氧化物層,而緊鄰著此氧化層下方則為沒有析出物存在的鉻缺乏區,在鉻缺乏區當中靠近氧化鉻層的那一端可以觀察到許多因選擇性氧化反應而形成次微米級孔洞,更往基材內部的區域觀察時,則可以在基材中觀察到大量碳化物析出。
304L及347不銹鋼經過600 ℃之35%CO-60%H2-5%H2O混合氣氛之長時間曝露試驗後,304L不銹鋼試片的蝕孔之最大深度與半徑的比值為1:3.44,而347不銹鋼試片的比值為1:5.71,主要是因為347不銹鋼中的合金元素鈮能夠有效地減緩塵化反應的發生速度,以致造成這樣的差異。
321不銹鋼於600 ℃之35%CO-60%H2-5%H2O 氣氛中,經過500及1000小時的曝露試驗之後,試片的邊緣(edge)及角隅(corner)為蝕孔優先成核位置,歸因於試片邊緣及角隅位置的氧化鉻鈍化膜在生成過程中受幾何因素的影響而容易生成裂縫,進而成為塵化反應的起始位置。321不銹鋼試片因塵化反應形成的金屬顆粒,基本上具有鐵/鎳富集的化學組成。而蝕孔下方基材中的碳化物析出區域大小,隨著曝露時間的增加而有增大的趨勢,經過TEM的分析得知,化學組態Cr7C3的碳化鉻主要生成於高碳濃度的基材外層區域,而化學組態Cr23C6的碳化鉻則存在於碳濃度較低的基材內部區域。
310不銹鋼於於600 ℃之35%CO-60%H2-5%H2O混合氣氛中進行500及1000小時的曝露試驗之後,試片表面的蝕孔呈現出花瓣般縐折的形貌,且蝕孔底部呈現出凹凸起伏的不平整表面,可歸因於表面所生成的鉻/錳氧化物及鉻/錳/鐵氧化物兩者的保護性和二次蝕孔於蝕孔底部的成核成長有關。
Metal dusting is a high temperature corrosion phenomenon which mainly occurs in high carbon-activity atmospheres in the temperature ranging of 400 to 800 ℃. Metal dusting process would disintegrate metal materials into a mixture of powdery metal, oxide, carbide and carbon deposits.
The metal dusting behavior of Type 304L, 310, 321 and 347 stainless steels (SSs) in a flowing CO/H2/H2O mixed gas stream at 600 ℃ was investigated. After a long-term exposure(500-hr) in a 35 % CO + 60 % H2 + 5 % H2O gas, large pits were formed on steel surfaces. The microstructures and chemical compositions of the reaction products and the substrates under the pits were examined using a scanning electron microscope (SEM) and a transmission electron microscope (TEM), each combined with an energy dispersive spectrometer (EDS). At the bottom of the pits, a thick layer of coke consisting of carbon and disintegrated Fe/Ni particles was found. A thin layer of oxide was observed below this outer layer, and a Cr-depleted precipitate-free zone contained voids just beneath this layer which resulted from the selective oxidation of stainless steels. Massive matrix carbide precipitation occurred below the Cr-depleted zone. Moving toward the interior of the substrate, Massive carbide and intergranular carbides were formed in the inner most portions of the scales beneath the substrate.
The aspect ratio of the pits formed in 304L SS was higher than that formed in 347 SS. The experimental results showed that niobium (Nb) could delay the ingress of carbon and retard the metal dusting reaction.
According to the results, the edges and corners of 321 SS were the most sensitive sites for pitting attack. The relatively high tendency for oxide passive film to breakdown at the edges and corners was responsible for the initiation of metal dusting. The composition of the metal particles dislodged from 321 SS surface was basically the Fe/Ni metallic phase, which might be either enriched with Ni or Fe. The carbide precipitation zone under the pit increased with increasing the exposure time in the high carbon-activity gas-environment. Matrix carbide in the form of Cr7C3 was observed in the outer zone close to the pit bottom, while grain boundary carbide in the form Cr23C6 was observed in the area far below the pit bottom.
After a long-term exposure (500-hr) of 310 SS, the coalescence of small pits would cause the formation of pit with a petal-like feature. The cracks at the substrate under the pit were the preferential sites for carbon inward diffusion and led to metal dusting attack. Secondary pit nucleation at the bottom of the primary pit would lead to the development of irregular appearance of the bottom surface. The relatively high tendency for oxide passive film to breakdown at the Cr/Mn/Fe oxide covered area was responsible for the enlargement of pit size.
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