恆星動力學 的英文怎麼說

中文拼音 [héngxīngdòngxué]
恆星動力學 英文
stellar dynamics
  • : Ⅰ形容詞1 (永久; 持久) permanent; lasting 2 (平常; 經常) usual; common; constant Ⅱ名詞1 (恆心...
  • : 名詞1 (夜晚天空中閃爍發光的天體) star 2 [天文學] (宇宙間能發射光或反射光的天體) heavenly body...
  • : Ⅰ名1 (力量; 能力) power; strength; ability; capacity 2 [物理學] (改變物體運動狀態的作用) forc...
  • : Ⅰ動詞1 (學習) study; learn 2 (模仿) imitate; mimic Ⅱ名詞1 (學問) learning; knowledge 2 (學...
  • 恆星 : [天文學] fixed star; star恆星大氣 stellar atmosphere; 恆星導航 star navigation; stellar guidance;...
  1. Many planets ( for example, ganymede, mercury, the earth, jupiter and saturn ) and stars ( for example, the sun ) possess intrinsic magnetic fields. the explanation for their existence and variation remains a great challenge to planetary scientists and astrophysicists. this article attempts to review some recent developments and difficulties in the study of magnetohydrodynamics for the electrically conducting fluid interiors of planets and stars. it is the fluid motions, usually driven by thermal convection, that generate and sustain magnetic fields through magnetohydrodynamic processes in planets and stars. in planets, the magnetohydrodynamic processes are strongly affected by the combined and inseparable effects of rotation, magnetic fields and spherical geometry. the key dynamics involves the interaction between the coriolis and lorentz forces. in the sun, it is the solar tachocline, a thin shear flow layer located at the base of the convection envelope, that plays an essential role in the solar magnetohydrodynamic processes which produce the 11 - year sunspot cycle. some results of a new nonlinear three - dimensional solar dynamo model are also presented

    許多行(如木衛三,水,地球,木和土)和(如太陽)具有內部磁場.對這些磁場的存在和變化的解釋對行家和天體物理家是一個巨大的挑戰.本文試圖總結行的導電流體內部磁流體研究的新近發展和困難.一般由熱對流驅的流通過磁流體過程產生並維持在行中的磁場.在行中磁流體過程強烈地受到轉,磁場和球幾何位型的綜合影響.其的關鍵方面涉及科里奧利和洛倫茲間的相互作用.在太陽中其流線,即處于對流層的薄的剪切流層在太陽的磁流體過程中扮演了一個基本的角色,並由之產生了11年的太陽黑子周期.本文也給出了一個新的非線性三維太陽發電機模型
  2. Topics include : planets, planet formation ; stars, the sun, " normal " stars, star formation ; stellar evolution, supernovae, compact objects ( white dwarfs, neutron stars, and black holes ), plusars, binary x - ray sources ; star clusters, globular and open clusters ; interstellar medium, gas, dust, magnetic fields, cosmic rays ; distance ladder ; galaxies, normal and active galaxies, jets ; gravitational lensing ; large scaling structure ; newtonian cosmology, dynamical expansion and thermal history of the universe ; cosmic microwave background radiation ; big - bang nucleosynthesis

    課程的主題包含了:行、行形成;、太陽、正常的形成;演化、超新、緻密天體(白矮、中子及黑洞) 、波霎、雙x -射線源;團、球狀及疏散團;際介質、氣體、塵埃、磁場、宇宙射線;距離階梯;系、正常及活躍系、噴流;重透鏡;大尺度結構;牛頓宇宙、宇宙的膨脹及溫度發展歷史;宇宙背景微波輻射;大霹靂核合成。
  3. Dynamic elongated clouds envelop bubbles of multimillion degree gas produced by high - velocity winds from dying stars

    伸長的雲團包裹著瀕死高速風造就的百萬度氣體泡。
  4. The evolution time in our calculation is chosen to be 12 gyr, which is the mean value of globular cluster ages in the galaxy

    蒸發對小質量球狀團的演化起著主導作用,大質量的演化、銀河系核球和盤的沖擊加熱以及磨擦則主要影響大質量球狀團的演化。
  5. Besides acting as powerful signposts of active star formation, the intense maser emission provides a unique tool to probe the physical conditions and kinematics of these regions on scales of 10 - 103 au

    際脈澤不僅是形成的一個及其重要的標志,而且也提供圍繞大質量尺度10 - 10 ~ 3au分子氣體的物理條件和結構的信息。
  6. Interstellar dynamics ; molecular outflows ; jet ; star formation

    際介質分子外向流噴流形成
  7. They are the stellar evaporation in the tidal field, the stellar evolution during the early evolutionary stage, the tidal shocks due to clusters passing through the bulge and disk, and the dynamical friction

    本文考慮的過程有四種,即:蒸發、早期大質量的演化、銀河系核球和盤的沖擊加熱以及磨擦。
  8. Black hole is the prediction of general relativity on the condition of great gravitation. as the research of x - ray astrophysics, the research of black hole has been made rapid progress, providing substantial basis for black hole physics and making exploring and researching black hole be front - line subjects

    黑洞是廣義相對論在強引條件下的預言, x射線天體物理的研究推級黑洞的研究,使理論推測的黑洞成了可實在搜尋和探索的天體;使黑洞物理建立在了堅實的基礎之上。
  9. We have analyised the observed results of low and high spatial resolution observations of molecular line emission toward regions of high - mass star formation which have contributed to the understanding of the physical conditions, morphologies, and dynamics of the molecular gas in the immediate vicinity of recently formed massive stars

    本文研究了來自大質量形成區的一些分子譜線的低解析度和高解析度觀測結果。這些結果有助於我們了解在最近形成的大質量附近分子氣體的物理條件,形態以及結構。
  10. Peter olson develops computer models to study the structure and dynamics of the interiors of planets and stars

    歐爾森藉由發展電腦模型,以研究行內部的結構和
分享友人