outward pressure 中文意思是什麼

outward pressure 解釋
向外施力握
  • outward : adj 1 外頭的,外部的;外形的,表面的;皮毛的;明顯的;可見的;公開的。2 向外的,向外去的;外出的...
  • pressure : n 1 壓;按;擠;榨。2 【物理學】壓力,壓強;大氣壓力;電壓。3 精神壓力,政治[經濟、輿論等]壓力。4...
  1. The buildup of pressure would force gas outward at speeds far above escape velocity

    壓力的增加,將迫使氣體以遠高於脫離速度的速率向外逃逸。
  2. In contrast, in an area of high pressure, the air at low levels spreads outward and air descends from aloft

    相反,在高壓區內空氣往外擴散,逼使上面的空氣下沉。
  3. The afterflow represents a production of kinetic energy which becomes convered into a pressure wave when the outward flow of water is reversed.

    殘余塑性流動代表在外向水流返回時動能變為壓力波的一種結果。
  4. Special patent design , utilizes hydraulic full - automation systematic outward - turning type. the operator can regulate hydraulic pressure freely , and the operating space is not limited , exactly improves working efficiency and safety rate

    獨特的專利設計,採用液壓翻開式全自動系統方式,操作空間不受限制,可調液壓壓力,顯著提高了工作效率和安全生產率。
  5. Deep convulsions, combined with the pressure of radiation and other forces, heave the distended and loosely bound surface layers outward into space, creating a planetary nebula

    深層的擾動,結合輻射壓與其他作用力,將脹大而鬆散的表層高高舉起,向外拋入太空中,創造出行星狀星雲。
  6. Because of these two balancing forces the outward pressure and the inward gravitational attraction, the star is stable for a very long time from millions to billions of years

    最後向內的引力和向外的壓力會達致平衡,讓恆星可以長時間保持穩定由數百萬至數百億年不等。
  7. At some point, the density and temperature at the center of the cloud of gas will be high enough to ignite the nuclear fusion. the energy produced by the fusion will create two kinds of outward pressure to act against the gravitational attraction

    隨著恆星不斷收縮,核心氣體的溫度及密度亦不斷上升,直至燃點起熱核反應,所產生的能量會造成兩種向外的壓力,對抗向內的萬有引力。
  8. 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

    恆星內部所產生的高溫,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,令恆星保持穩定,進入主序星階段。
  9. A sufficiently large and dense core can overcome the outward force of gas pressure to collapse under its own weight

    夠廣大且夠緻密的雲核,會以自身的重量克服向外的氣體壓力而崩塌。
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