coronal的例句大全

Observations on Coronal Mass Ejections and Its Associated Solar Activities

日冕物质抛射及相关太阳活动的观测研究

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Numerical simulation of coronal mass ejections between two coronal streamers

两冕流间物质抛射事件的数值模拟

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The Neutral Current Sheet and Its Radiation Pairs of Side Sources in Coronal Mass Ejections

日冕物质抛射的中性电流片及边源辐射对

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Radio Moving Type ⅳ Bursts and Coronal Mass Ejections

射电运动Ⅳ型爆发和日冕物质抛射

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Solar coronal mass ejections in space weather

日冕物质抛射&空间天气的扰动源

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Solar Atmospheric Responses to. Magnetic Flux Eruptions I. A Mechanism for Coronal Mass Ejections

磁通量喷发的大气响应Ⅰ.日冕物质喷射机制

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Solar Radio Meter Burst and Coronal Mass Ejections

太阳射电米波爆发与日冕物质喷射

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Coronal mass ejections and solar particle events

日冕物质抛射与太阳粒子事件

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At least in some flares, these twisted magnetic field loops must become coronal mass ejections.

至少在一些闪焰事件里，这些扭曲的磁场环圈会产生日冕团块喷射。

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The hydromagnetic nature of solar coronal mass ejections

太阳日冕物质抛射的磁流体力学性质

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One telescope aboard SOHO can provide three or four days' warning of major solar events by spotting coronal mass ejections.

通过观测日冕物质的喷发，SOHO上的一台望远镜能提前三到四天预报太阳的重大活动。

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Moreover, solar radio microwave bursts which accompany with coronal mass ejections during February 1999 to August 1999 are analyzed.

此外，分析讨论了1999年2月至1999年8月期间与CME共生的太阳微波爆发。

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An absence of sunspots also means an absence of solar flares and their more violent siblings, coronal mass ejections.

黑子的缺失还预示着太阳耀斑的缺席，同时，猛烈的日冕喷发也不会出现。

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Coronal mass ejections ( CMEs) belong to large-scale solar active phenomena and cause strong disturbances on the geospace environment, being a main source of disastrous space weather.

日冕物质抛射（CME）属于大尺度太阳活动现象，它能造成地球空间环境的剧烈扰动，是空间灾害天气的主要源头。

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Method: In 23 cases 28 ears with congenital atresia of external auditory meatus. A high resolution spiral CT is used to display the temporal bone by axial and direct coronal planes.

方法：23例（28耳）先天性外耳道闭锁、中耳畸形患者，经高分辨率螺旋CT轴位、冠状位颞骨扫描，应用仿真内镜软件行图像三维重建。

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The background field consists of a coronal streamer containing three closed bipolar fields and an open magnetic field with an equatorial current sheet.

背景磁场由含3个闭合双极场的冕流和带赤道中性电流片的开放场构成，磁绳位于中心双极场的下方，其特性由环向磁通和轴向磁通表征。

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The rise velosity of the top of the cusp region in a coronal streamer may be more than 2km/ s, if the longitude angular size is more than 27 ° associated with a CME occurence.

当一个日冕物质抛射伴随冕流产生时，冕流的经向角大小若大于27°，可导致冕流尖角区顶部上升速度大于2km／s。

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The results of observation show: For large scale region, polar coronal hole is unipolar open field; For enhanced magnetic structures of 48h time scale, open field is dominant, however, the mixing case of open field and closed field is also present;

观测结果表明t就极无涧大尺度范围来看，是单极开放场I就48h时标的加强磁结构来说，以开放场为主的情况下，有开放场与闭合场栩混杂的情况。

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A male patient presented with 2 rows of asymptomatic papules along the coronal margin for 10 years.

患者男，44岁。龟头冠状沟2行带状排列的皮色丘疹10年，大部分丘疹呈珍珠状，少数丘疹呈丝状疣样，长度>0.7cm。

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The effect of intracoronal bleaching on cervical periodontium of dogs

髓室内漂白对狗牙颈部牙周组织的影响

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