M - magnetosphere 中文

magnetosphere n.【天文學】磁層。adj.-spheric

n. 【天文學】磁層。 adj. -spheric “asymmetric magnetosphere“ 中文翻譯：不對稱磁層“compressed magnetosphere“ 中文翻譯：受壓磁層“dawnside magnetosphere“ 中文翻譯：晨側磁層“dayside magnetosphere“ 中文翻譯：晝側磁層“earth magnetosphere“ 中文翻譯：地球磁層“helio magnetosphere“ 中文翻譯：日磁層“inner magnetosphere“ 中文翻譯：內磁層“jovian magnetosphere“ 中文翻譯：木星磁層“jupiter magnetosphere“ 中文翻譯：木星磁層“magnetosphere convection“ 中文翻譯：磁層對流“magnetosphere coupling“ 中文翻譯：磁性層耦合“magnetosphere explorer“ 中文翻譯：磁化層探查器“magnetosphere shape“ 中文翻譯：磁層形狀“magnetosphere sizes“ 中文翻譯：磁層大小“mercurian magnetosphere“ 中文翻譯：水星磁層“planetary magnetosphere“ 中文翻譯：行星磁層“box model of magnetosphere“ 中文翻譯：磁層的盒模型“pressure exerted by magnetosphere“ 中文翻譯：磁層施加的壓力“quiet-time magnetosphere“ 中文翻譯：寧靜磁層“magnetosonic wave“ 中文翻譯：磁聲波“magnetosome“ 中文翻譯：磁體“magnetosiren“ 中文翻譯：磁警報器“magnetosheath“ 中文翻譯：磁鞘“magnetoscope“ 中文翻譯： n. 驗磁器。

magnetostriction
On the basis of analyzing previous scientists ' work , aeromagnetic data from north china wee reprocessed with 3 - d magnetosphere inversion method and program quantitative buried depth of curie temperature interface was obtained ; seismogenesis and its re1atnhip with curie temperature interface were discussed in the light of results from deep seismic sounding and deep fluid 摘要在前人工作的基礎上，運用三維磁性層反演方法和程序，對華北地區航磁資料進行了再處理，得出了研究區內居里溫度面的定量埋深，結合人工地震測深和深部流體對地震成因及其與居里面的關系進行了討論。
Recent study of the kilohertz quasi - periodic oscillations ( qpos ) in low mass x - ray binaries ( lmxbs ) indicates that the radiation force , other than the magnetosphere and disk interaction and the general relativity ( gr ) effect setting the inner disk edge , serves as the disk truncation mechanism on shorter time scales . some results and discussions are presented in this paper 最近對低質量x射線雙星中的千赫茲準周期振動的研究表明,是輻射壓力,而不是盤和磁球的相互作用以及處于盤內邊界的廣義相對論效應在短時標的盤切斷機制上起作用.本文給出了一些研究結果及討論
Just as the passage of a supersonic jet through the atmosphere produces a shock wave , the encounter of the solar wind with the magnetosphere forms a shock wave ? known as the bow shock ? some 13 , 000 kilometers upstream ( that is , closer to the sun ) from the dayside magnetopause 就像超音速噴射機在大氣層飛行時會產生震波，當太陽風碰上地球磁層，也一樣會產生震波，我們稱之為弓形震波，產生位置約在晝側的磁層頂外13000公里處。
Besides directing compasses , the earth ' s magnetic field reaches out into space to direct the flow of the solar wind around the planet ? forming a structure called the magnetosphere ( depicted above ) 地球的磁場效應不僅能夠指引指南針，還能夠將其效應延伸至宇宙空間來指引地球四周的太陽風的流向，這樣就形成了一種稱為“磁氣圈”的結構（如上圖所示）。
The field forms a protective shell called magnetosphere that has a radius around 10 times that of the solid earth . but strong eruptions on the solar surface can seriously distort this shell , creating geomagnetic storms 地球磁場形成一個大小約地球直徑十倍稱為磁層的保護殼，當太陽表面出現猛烈的爆發，便會嚴重扭曲這個保護殼，形成磁暴。
These results show the expected increases in solar wind plasma density downstream of the bow - shock boundary , as well as significant solar wind plasma densities within mercury ' s magnetosphere close to the planet 這些調查結果表明，預計增幅在太陽風等離子體密度下游弓激波邊界，以及大量的太陽風等離子體密度與水星的磁層接近地球。
For other orientations of the imf , reconnection still happens , but it may be more localized in the higher latitudes , where the released energy mainly flows around the magnetosphere rather than into it 假如imf指向別的方向，磁力線重連仍能發生，但會比較局限在高緯度，釋放出的能量則主要流經磁層外圍，而非流入磁層內部。
The latter measurements provide definitive evidence that mercury ' s magnetosphere ? despite its small size ? is not a vacuum but hosts significant densities of heated solar wind plasma 后者測量提供確切的證據表明，水星的磁層-盡管它體積小-是不是一個真空，但東道主密度顯著激烈的太陽風等離子體。
Reconnection is most efficient when the imf has a component that is directed southward ? that is , opposite to the northward direction of the earth ' s magnetic field at the dayside of the magnetosphere 在磁層晝側，若imf有南向分量，也就是和北向的地球磁場方向相反，則磁力線重連的效率最高。
Under these circumstances , reconnection takes place along a wide equatorial belt , opening up nearly the entire outer boundary of the magnetosphere to the solar wind 在這種情況下，磁力線重連會在赤道面上寬廣的帶狀區域內發生，幾乎把整個磁層外圍邊界都打開，放太陽風進來。
They move under the influence of the dynamo currents in the earth ' s core , as well as electric currents flowing in the ionosphere , the radiation belts and the earth ' s magnetosphere 它們在地核內發電機流以及流動在電離層、輻射帶和地球磁氣圈內電流的影響下產生移動。
The finding is evidence of the complex interaction between saturn ' s moons , rings and magnetosphere . studying this interaction is one of cassini ' s objectives 這個發現是土星的月亮，環狀物和磁氣圈之間復雜交互感應的證明。這種交互感應的研究是卡西尼的主要目標之一。
Thus , this research could not say much about the effects of interplanetary charged particles , which cannot penetrate earth ' s magnetosphere 因此，對游走于行星之間，但是無法穿透地球磁層的帶電粒子所產生的效應，這項研究所透露的訊息不多。
The three st5 satellites , each no bigger than an average tv set , will help scientists to study magnetic fields in earth ' s magnetosphere 三個空間技術5號衛星(每個尺寸都不大于一臺普通的電視機)將幫助科學家研究地球磁氣圈的磁場。
Yet the actual long - term survival of active organisms , spores or complex organic molecules beyond earth ' s magnetosphere has never been tested 活性有機體、孢子或復雜的有機分子，在地球磁層之外能否長期幸存，則從未實地驗證過。
In other words , how can the wind overcome the barrier of the geomagnetic field and drive the motions of the plasma inside the magnetosphere 換言之，即太陽風是如何克服地球磁場的阻礙，進而驅動磁層里的電漿運動？
But in the magnetosphere , weather results from the interaction between the earth ' s magnetic field and the solar wind 但在磁層里，太空天氣卻是由地球磁場和太陽風的交互作用所造成。
This animation shows a conceptual sketch of mercury ' s magnetosphere at the time of the messenger flyby 這個動畫是信使號探測船探測水星磁層時的模擬圖。
The transfer of magnetic energy from the solar wind radically alters the shape of the magnetosphere 從太陽風傳來的磁場能量，徹底改變了磁層形狀。

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magnetosphere

magnetosphere n.【天文學】磁層。adj.-spheric

magnetostriction

Thus , this research could not say much about the effects of interplanetary charged particles , which cannot penetrate earth ' s magnetosphere 因此，對游走于行星之間，但是無法穿透地球磁層的帶電粒子所產生的效應，這項研究所透露的訊息不多。

The three st5 satellites , each no bigger than an average tv set , will help scientists to study magnetic fields in earth ' s magnetosphere 三個空間技術5號衛星(每個尺寸都不大于一臺普通的電視機)將幫助科學家研究地球磁氣圈的磁場。

Yet the actual long - term survival of active organisms , spores or complex organic molecules beyond earth ' s magnetosphere has never been tested 活性有機體、孢子或復雜的有機分子，在地球磁層之外能否長期幸存，則從未實地驗證過。

In other words , how can the wind overcome the barrier of the geomagnetic field and drive the motions of the plasma inside the magnetosphere 換言之，即太陽風是如何克服地球磁場的阻礙，進而驅動磁層里的電漿運動？

But in the magnetosphere , weather results from the interaction between the earth ' s magnetic field and the solar wind 但在磁層里，太空天氣卻是由地球磁場和太陽風的交互作用所造成。

This animation shows a conceptual sketch of mercury ' s magnetosphere at the time of the messenger flyby 這個動畫是信使號探測船探測水星磁層時的模擬圖。

The transfer of magnetic energy from the solar wind radically alters the shape of the magnetosphere 從太陽風傳來的磁場能量，徹底改變了磁層形狀。