磁層暴 的英文怎麼說

中文拼音 [céngbào]
磁層暴 英文
magnetospheric storm
  • : 名詞1. [物理學] (磁性; 能吸引鐵、鎳等的性質) magnetism 2. (瓷) porcelain; china
  • : i 量詞1 (用於重疊、積累的東西 如樓層、階層、地層) storey; tier; stratum 2 (用於可以分項分步的...
  • : Ⅰ形容詞1 (突然而且猛烈) sudden and violent 2 (兇狠; 殘酷) harsh and tyrannical; cruel; fierce...
  1. The global ionospheric response to the geomagnetic storm eventduring may

    1998年5月事件期間全球電離響應形態與機制的研究
  2. 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

    地球場形成一個大小約地球直徑十倍稱為的保護殼,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
  3. Performance analysis of ionospheric grid model during storm for wide area augmentation system

    期間增強系統電離網格模型性能分析
  4. In addition, the study shows that the cmes " traveling direction is also an important factor, which influence the intensity of the geomagnetic storms. we also analyzed gcrs data from beijing super - neutron - monitor ( snm ) by using fft and power spectrum method

    我們對cme運動方向與強弱的關系進行了初步的研究,研究表明,同樣條件下,正對頂的cme形成的更強,即cme的運動方向是影響強弱的一個重要因素。
  5. Several influence factors to result plasma drift in hainan were analyzed. in this paper the characteristics of ionospheric parameters variation were analyzed systematically and some new results in storm - time such as seasonal behaviors were obtained ; it is the first time to investigate the ionospheric drift behavior in hainan and some new results was obtained, the relationships between each two plasma drift velocity components in storm time in hainan were found and the electric filed variation in hainan ionosphere also was obtained ; the results also show that there are big differences of the ionosphere parameters bo and bl obtained from the data with that obtained from the iri - 2001 applied for hainan ; a new phenomena was found during a strong magnetic storm, that a layer with very strong electron density and density grad was found during the recovery phase of the storm, its horizontal scale is beyond 100km and temporal scale is about 2 hours, this phenomena repeated 3 times continuously. a type of negative disturbance in high and low latitude but positive disturbance in east - asia also has been found

    本文較為系統地給出了海南地區電離的參數變化特徵,特別是得到了一些時與以往不同的季節特性;第一次給出了海南地區的電離等離子體漂移特徵,發現等離子體漂移時擾動在三個方向上有內在的聯系,得到了電場變化曲線;研究結果還表明海南電離的半厚指數和形狀參數等與國際參考電離iri - 2001存在很大差別;通過對強擾動事件期間的參數變化特性分析發現,在恢復相期間海南地區電離底部存在一個電子密度非常大的高密度區,高密度區底部電子密度梯度隨高度急劇增加,該區域的水平尺度可達100公里以上時間尺度約為2小時,連續出現過三次,這是一個在海南從來未發現的新現象;研究還發現了時東亞地區電離擾動會出現高低緯負相而中緯正相的現象。
  6. Increased radiation from the sun and occurrence of geomagnetic storms i. e. severe distortion of geomagnetic field of the earth may cause disturbances such as increases in density in the earth s upper atmosphere. these result in a greater drag on the movement of satellites and spacecraft, causing a slow - down or even a change in orbit

    輻射的增加及地即地球場急速變形的出現,會導致地球上大氣的擾動,例如空氣密度的上升,從而使衛星和太空船在航行時受到的阻力大增,航行速度因而減慢,甚至軌道亦會改變。
  7. Increased radiation from the sun and occurrence of geomagnetic storms ( i. e. severe distortion of geomagnetic field of the earth ) may cause disturbances such as increases in density in the earth s upper atmosphere. these result in a greater drag on the movement of satellites and spacecraft, causing a slow - down or even a change in orbit

    輻射的增加及地(即地球場急速變形)的出現,會導致地球上大氣的擾動,例如空氣密度的上升,從而使衛星和太空船在航行時受到的阻力大增,航行速度因而減慢,甚至軌道亦會改變。
  8. Solar wind flows out from the corona the sun s outer atmosphere into interplanetary space at speed of between 300 and 900 km per second. it causes fluctuation to the earth s magnetic field, which we call magnetic storm. such event will cause deflection of compass needles

    而太陽風則以每秒300至900千米的速度由日冕太陽外大氣向外拋射,進入行星際空間,對地球場造成擾動而產生,導致指南針指針偏移,嚴重的話更會導致電力受阻和電話線路中斷。
  9. Characteristics of variation and disturbances in low - latitude ionosphere were investigated based on the data observed in hainan under different magnetic activities and solar activities including variations and disturbances of parameters in different ionospheric layers, behaviors of plasma drift and a comparison with other low - latitude ionospheric station. the disturbance propagations from high to low latitude region during magnetic storm time are also investigated with analyzing the data obtained from the east - asian high - middle latitude stations

    本文在觀測數據分析的基礎上研究了不同地活動和太陽活動條件下低緯電離的變化和擾動特性,包括海南電離各分的參數變化和擾動特性,電離漂移的變化特性,並與低緯度地區其他臺站進行了對比分析,還對時東亞地區高中緯度地區臺站的觀測資料進行了分析,研究了電離擾動從高緯到低緯的響應過程。
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