高溫保溫階段 的英文怎麼說

中文拼音 [gāowēnbǎowēnjiēduàn]
高溫保溫階段 英文
soaking period
  • : Ⅰ形容詞1 (從下向上距離大; 離地面遠) tall; high 2 (在一般標準或平均程度之上; 等級在上的) above...
  • : Ⅰ形容詞(不冷不熱) warm; lukewarm; hot; gentle; mild Ⅱ名詞1 (溫度) temperature 2 (瘟) acute ...
  • : Ⅰ動詞1 (保衛; 保護) defend; protect 2 (保持) keep; preserve; maintain in good condition 3 (...
  • : 名詞1. (臺階) steps; stairs 2. (等級) rank 3. [醫學] (耳蝸的三個螺旋管的任一個) scala 4. [數學] order 5. [地質學] stage
  • : Ⅰ量詞(部分) section; segment; part; paragraph; passage Ⅱ名詞(姓氏) a surname
  • 高溫 : high temperature; elevated temperature; hyperthermia; megatemperature; inferno
  • 階段 : stage; phase; period; gradation; bench
  1. Therefore both non - intensive temperature procedure and shorter treatment time ( especially in the period when moisture content is still high for xero - labile materials ) applied in processing are suggested to enhance quality retention

    因此為持乾燥后產品的質量,常採用較和的乾燥條件,以及減少物料在含水率的乾燥時間。
  2. The following results were found, i. e., the water ratio affects obviously the acoustic wave velocity of rock sample ; the wave velocity is higher in saturated rock samples than in unsaturated ones ; and it decreases gradually with the strain of samples during uniaxial compression ; and also with the lengthening holding time at 160 ; when heating the samples the acoustic wave velocity increases slightly in initial stage and comes to the peak value at 60, then decreases gradually with increasing temperature ; meantime, there is a certain temperature effect on rock samples size

    實驗發現含水率對波速影響比較大,飽和巖樣的聲波傳播速度於不飽和巖樣的聲波傳播速度;人工預制裂紋對聲波傳播速度影響不大;單軸壓縮條件下,聲波傳播速度隨應變增加逐漸降低;在同一度( 160 )下,波速隨時間的增加而逐漸降低;在對巖樣逐漸加熱情況下,初始加熱波速略有升,當度達到60時,巖樣波速達到峰值,之後隨著度繼續升其波速逐漸下降;波速隨度變化具有一定的尺寸效應。
  3. Today, the house build in our country is staying at the period from meeting basic needs to making good life and from quantity to quality. there ' s more and more attentions paid to protect and improve the dwelling quality of the middle - low income people

    目前我國住宅建設正處于從「飽型」向「小康型」 ,由「數量型」向「質量型」轉變的重要,特別是證和提大多數中低收入家庭居住生活的質量越來越受到重視。
  4. Particles in the star move around rapidly due to high temperature creating a high gas pressure. together with the radiation pressure generated by the photons, they exert pressure pushing outward to balance gravity s inward pull. then, a star becomes stable and now enters the main sequence phase

    恆星內部所產生的,會令粒子急劇運動,產生向外的氣體壓力,再加上光子的輻射壓力抵消掉向內的引力,令恆星持穩定,進入主序星
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