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interplanetary shock in Chinese

Pronunciation:
How to pronounce "interplanetary shock""interplanetary shock" in a sentence

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  • 行星際激波

Examples

  • This paper presents three - dimensional , global numerical simulations of the dynamic response of the earth ' s ionosphere to interplanetary shocks
    摘要本文就地球電離層對行星際激波的動力學(xué)響應(yīng)進行三維全球數(shù)值模擬研究。
  • Such a response depends on the strength of the interplanetary shock : for a stronger shock , the new region current gets stronger , extends for a longer distance towards the equator , and reaches a lower latitude
    這一響應(yīng)過程和行星際激波強度有關(guān):激波強度越強,新生的區(qū)場向電流也越強,它向赤道方向延伸的距離也越大,能到達的緯度也越低。
  • The background interplanetary magnetic field is spiral with a vanishing south - north component , the initial ionosphere is dominated by the region field - aligned current ( fac ) and the corresponding dawn - dusk electric field , and the interplanetary shock collides with the earth along the sun - earth line
    背景行星際磁場為螺旋場,南北分量為零;初始電離層由區(qū)場向電流和相應(yīng)的晨昏電場所主導(dǎo);行星際激波沿日地連線方向撞擊地球。
  • In order to predict the arrival time at 1au of interplanetary shocks , a simple model called disturbance model is established here . in this model , the travel time is assumed to be a function of energy that is released from solar explosives , and input pulse longitudinal width , input pulse duration , the interaction of interplanetary shock and background solar wind are also taken into account
    本論文考慮了激波爆發(fā)源角寬度、能量、驅(qū)動時間、激波速度及其與背景太陽風(fēng)之間的相互作用,利用流體力學(xué)擾動方程建立起一個激波擾動傳播模型,用于研究激波從太陽傳播到地球軌道附近( 1au處)所需要的時間問題。
  • In order to verify the prediction efficiency , 27 interplanetary shock events from january 1979 to june 1982 and 68 interplanetary shock events from february 1997 to january 2000 are used for testing . comparing the results of our disturbance model to those obtained by stoa and ispm , we find that our disturbance model is as good as the other two models , and in some cases even better
    為印證擾動傳播模型的適用性,利用79年到82年間的27個激波事件,以及97年2月到2000年1月間的68個激波事件,對激波到達地球軌道附近的傳播時間進行了預(yù)測,并將結(jié)果與目前流行的行星際激波事件到達地球軌道時間的stoa和ispm預(yù)報模型所得結(jié)果進行了比較。
  • The prediction of disastrous space weather is a hot topi c among solar - terrestrial physics and high technological fields . we propose that the future forecasting of the physical conditions that the violent solar disturb ance causes at the earth by propagating in solar wind depends heavily on the num erical method . this paper analyses the existing problems we are facing in the num erical prediction of disastrous disturbance events in solar - terrestrial space , an d then gives some suggestions for future study . for such a purpose , a six step sol ution method is developed to deal with one - dimensional symmetric interplanetary shock dynamics . it should be point out that that initialization of fully self - con sistent 3 - d mhd codes considering the solar - interplanetary - geomagnetic coupled r elations with initial - boundary values at 1r of the global output of solar pl asma and magnetic field using available solar observations is an essential requi rement in space weather operational codes for forecasting purposes
    空間災(zāi)害性天氣的預(yù)報是日地物理學(xué)界及高科技領(lǐng)域的熱門話題.未來預(yù)測太陽劇烈擾動所造成的行星際風(fēng)暴到達地球空間的狀態(tài)勢必借助于數(shù)值方法.淺析了空間災(zāi)害性擾動事件數(shù)值預(yù)報存在的問題及未來設(shè)想,針對這一目的對一維球?qū)ΨQ問題提出了處理行星際激波的6步求解方法,指出未來空間災(zāi)害性擾動事件預(yù)報模式應(yīng)是一個基于三維的以真實太陽風(fēng)為背景自洽建立起來的、以太陽等離子體輸出及磁場全球結(jié)構(gòu)為初邊值、太陽、行星際、地磁因果耦合模式

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