太阳-日冕物质抛射(CME),Sun: Coronal Mass Ejection (CME)英语短句,例句大全

太阳-日冕物质抛射(CME),Sun: Coronal Mass Ejection (CME)
1)Sun: Coronal Mass Ejection (CME)太阳-日冕物质抛射(CME)
2)coronal mass ejection (CME)/flare日冕物质抛射(CME)/耀斑
3)coronal mass ejections太阳日冕物质抛射
1.The hydromagnetic nature of solar coronal mass ejections;太阳日冕物质抛射的磁流体力学性质
4)Sun: coronal mass ejections太阳-日冕物质抛射
5)coronal mass ejection日冕物质抛射
1.Classified prediction of geomagnetic disturbance caused by coronal mass ejection;日冕物质抛射引起地磁扰动的分类预报
2.The relationships between the coronal mass ejections (CMEs), interplane tary disturbances and geomagnetic storms are studied, involving the solar source distribution of geoeffective halo CMEs, the periodicity of CMEs, X-ray flares a nd geomagnetic disturbances, the threshold of interplanetary parameters in causi ng geomagnetic storms, etc.根据SOHO飞船上的LASCO和EIT探测器和GOES卫星的关于太阳活动的观测资料以及ACE和Wind飞船在地球轨道附近关于太阳风等离子体和行星际磁场的观测数据 ,分析了日冕物质抛射(CME)、行星际磁云和地磁暴的相关性。

英文短句/例句

1.THE MONITOR OF THE CME IN MARCH 1991 BY COSMIC RAYS银河宇宙线对1991年3月日冕物质抛射的监测
2.Studies on the Prediction Method for Geomagnetic Disturbances Caused by Coronal Mass Ejections;日冕物质抛射引起的地磁扰动预报方法研究
3.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
4.We show that both the preevent corona and the driving mechanism are important in the formation and evolution of CMEs.结果表明,初态日冕和驱动机制对日冕物质抛射的形成及演化都有重要影响.
5.These results may interpret the formation of plasmoid type CME.这些结果可用于解释等离子体团型日冕物质抛射的形成。
6.Characteristics of the Propagation and Evolution of Interplanetary Coronal Mass Ejections in the Heliosphere;行星际日冕物质抛射在行星际空间的传播和演化规律
7.A Bright Mass Ejection On the Solar Disk on 1980 October 141980年10月14日太阳视圆面上的明亮物质抛射
8.On the other hand, all the material in the transversal sheet comes from the corona and produces a high-temperature coronal loop.横向电流片的物质则全部来自日冕,从而形成高温日冕环。
9.quiet coronal X-ray emissio宁静日冕Ｘ射线辐射
10.Simulation of Atomic Coefficient and Radiation Losses of Impurity Using Non-coronal Model on HL-2A;HL-2A杂质原子参数和非日冕辐射的模拟
11.Projectivity of Hyperboloids of One or Two Sheets;双曲抛物面与单叶双曲面的射影性质
12.The Heat-Engine Effect of the Material Exchange in Solar Super Atmosphere--The Model of the Chromosphere-Corona Transition Region太阳高层大气物质交换的热机效应——色球-日冕过渡区模型
13.Horn parabolic reflector antenna喇叭抛物反射面天线
14.the parabolic reflector of a searchlight探照灯的抛物面反射镜
15.The Observational Evidence of Microwave Pulsations with Very Long Periods in the Corona日冕微波辐射甚长周期脉动的观测证据
16.Solar Radio Type Ⅱ Burst in the Corona and Interplanetary Medium日冕和行星际空间中的太阳射电Ⅱ型爆发
17.Stray light analysis of internally occulted mirror coronagraph反射式内掩日冕仪的光学设计与杂散光分析
18.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。

相关短句/例句

coronal mass ejection (CME)/flare日冕物质抛射(CME)/耀斑
3)coronal mass ejections太阳日冕物质抛射
1.The hydromagnetic nature of solar coronal mass ejections;太阳日冕物质抛射的磁流体力学性质
4)Sun: coronal mass ejections太阳-日冕物质抛射
5)coronal mass ejection日冕物质抛射
1.Classified prediction of geomagnetic disturbance caused by coronal mass ejection;日冕物质抛射引起地磁扰动的分类预报
2.The relationships between the coronal mass ejections (CMEs), interplane tary disturbances and geomagnetic storms are studied, involving the solar source distribution of geoeffective halo CMEs, the periodicity of CMEs, X-ray flares a nd geomagnetic disturbances, the threshold of interplanetary parameters in causi ng geomagnetic storms, etc.根据SOHO飞船上的LASCO和EIT探测器和GOES卫星的关于太阳活动的观测资料以及ACE和Wind飞船在地球轨道附近关于太阳风等离子体和行星际磁场的观测数据 ,分析了日冕物质抛射(CME)、行星际磁云和地磁暴的相关性。
6)CME日冕物质抛射
1.THE MONITOR OF THE CME IN MARCH 1991 BY COSMIC RAYS;银河宇宙线对1991年3月日冕物质抛射的监测
2.With the background structure,two tube models containing spiral magnetic field lines with a small length-scale can move in the computational domain step by step,interact afterward and trigger a Coronal Mass Ejection(CME)finally.在这种背景结构下,两个较小尺度的磁螺旋线管模型能够连续浮入到计算域,在计算域内相互作用,触发了日冕物质抛射(CME)。
3.The influence of a streamer background with nested close magnetic structures on the properties of CME initiated from its bottom is investigated in a solar meridian plane.在子午面内,研究具有嵌套闭磁场结构冕流背景对触发日冕物质抛射(CME)特征的影响。