色球
- Chromosphere;plage
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色球层在光球层气体的搅拌下不停地翻腾。
The chromosphere is a frothy layer churned up by gases in the photosphere .
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2004年6月8日金星凌日Hα色球观测
H α Chromospheric Observations of the Venus Transit on June 8,2004
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色球耀斑Hα逃逸光子的三维重构和演化分析
Three-dimensional Reconstruction of the Escape Photons of a Solar H α Flare
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色球耀斑Hα谱线轮廓不对称性研究进展
H α Line Profile Asymmetry in Chromospheric Flare
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1984年2月14日大角星色球活动的CaⅡH,K线观测
Chromospheric Activity of Arcturus Observed at Call H and K Lines on February 14 , 1984
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色球和日冕的MHD加热机制
MHD Mechanisms of Chromospheric and Coronal Heating
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类太阳色球活动星εEri磁场的观测研究
An observation study of the magnetic field on the solar-like chromosphere active star ε eri
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密度与除了低层色球辐射线OI(130.4nm)以外的其它所选太阳辐射流量之间的相关性都相当好。
The density correlates remarkably well with all the selected solar irradiances except the lower chromospheric O I ( 130.4 nm ) emission .
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利用色球Ha、TRACE/WL、SOHO/EITEUV单色像观测资料及SOHO/MDI光球磁场观测资料,对2003年10月22日太阳活动区AR0484内发生的日浪事件进行了研究。
By analyzing the YAO / Ha , TRACE / WL , SOHO / EIT EUV filtergrams and SOHO / MDI magnetograms , two surges occurring in NOAA AR 0484 on 2003 October 22 are investigated .
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他们说,这些酶素可抑制药物,可使抗生素更有效,甚至合成致命的超级病菌像是金黄色球状物耐甲氧西林或MRSA。
Drugs that inhibit these enzymes can make antibiotics much more potent , making even deadly superbugs like Methicillin-resistant Staphylococcus aureus or MRSA succumb , they said .
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自从1976年,Hall明确地提出RsCVn型双星的定义以来,密近双星的类太阳活动(也叫色球活动或磁活动)性质就引起众多天文工作者的极大兴趣。
Since RS CVn-type binary was defined by Hall in 1976 , the solar-type activity (" chromospheric activity " or " magnetic activity ") of contact binaries interests many astronomic researchers .
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ⅡPeg的色球活动很强烈,有明显的自转调制现象,在我们观测的每个自转周里都有耀斑事件发生,且这样的耀斑事件是贯穿整个色球层的。
The chromospheric activity of II Peg is very strong , and exhibits an obvious rotational modulation phenomenon . The optical flare is happened In every rotational period , and it is through each layer of the chromosphere .
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福建色球藻目(Chroococcales)新植物
New Chroococcales ( Cyanophyta ) from Fujian Province
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确定了色球底的位置;
The location of the chromospheric base has been determined .
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在两名教师的注视下,她打开了一个素色球。
As two teachers watched closely , she unwrapped a plain ball .
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基于色球蒸发的研究结果,我们进一步探究耀斑的加热过程。
Based on the results , we further explore the flare heating problem .
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太阳色球-日冕过渡层非共振加热的可能机制
A possible mechanism of nonresonant heating of the chromosphere - corona transition zone
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色球均匀摆放(分布)的问题描述和算法描述
Describing the Putting of Chromospheres Symmetrically and the Arithmetic
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广告打头的五位家长都抽到了素色球。
The first five parents selected plain wooden balls .
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拍摄实际的色球层很困难。
It is difficult to photograph the actual chromosphere .
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活动色球双星HR1099近红外分光光度观测
Infrared Spectrophotometry of the Chromospherically Active Binary HR 1099
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晚型矮星的色球活动
Chromospheric Activity of Late - type Dwarf Stars
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耀斑色球压缩区的传播与谱线的不对称性
The Propagation of Chromospheric Condensations and the Asymmetry of Spectral Lines in Solar Flares
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太阳色球细节放大像
A Method of Magnifying Solar Chromospheric Images
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太阳宁静区色球磁场观测
Chromospheric magnetic fields observation for quiet-Sun regions
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怎么知道你要打全色球还是带状球?
How do you know whether you should hit the solid or the striped one ?
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演化恒星的色球活动与恒星自转周期间存在很好的相关性。
The relation between stellar chromospheric activity and rotation of evolution stars have a good relativity .
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班半色球摆成水平,用低杆击球入袋,这时我们看看反旋转能维持多久。
Put the stripe horizontally and view how much backspin shows up when you hit low .
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云南天文台进口钙色球太阳滤光器原理和损坏元件分析及其修复
Analysis of the Principle and the Damaged Components of the Imported Solar K-Filter at Yunnan Observatory
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扼要地介绍了色球和日冕加热问题的研究历史。
The history of researches on the chromospheric and coronal heating is introduced briefly in this article .