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偏振亮度
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  polarization brightness
     The variation of the polarization brightness of coronal streamer in Carrington Rotations 1591-1592 is investigated.
     本文研究了卡林顿自转周1591 - 1592 中冕流偏振亮度的变化。
短句来源
     The distribution of the polarization brightness along streamer belts is inhomogeneous; the degree of the inhomogeneity is 10%-50%.
     冕流带偏振亮度的分布是不均匀的,不均匀度为10 % - 50 % 。
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  相似匹配句对
     POLARIZATION OF ACTIVE GALACTIC NUCLEI
     活动星系核的偏振
短句来源
     Showing- Colour Polarization
     显色偏振
短句来源
     The distribution of the polarization brightness along streamer belts is inhomogeneous; the degree of the inhomogeneity is 10%-50%.
     冕流带偏振亮度的分布是不均匀的,不均匀度为10 % - 50 % 。
短句来源
     2) lightness rectification;
     ②亮度矫正;
短句来源
     Through photometric measurement,the absolute brightness and polarization of the corona were obtained for the interval 1.1—3.5R_⊙.
     光度测量得到1.1—3.5R_⊙的日冕绝对亮度偏振;
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  polarization brightness
The rotation of the solar electron corona is determined for intervals when nearly periodic variations dominated the polarization brightness record during 1964-1976.
      
The effect of a propagating shock on the Hi Lα line and the polarization brightness in the inner solar wind region is investigated.
      
Density perturbations associated with the jet follow from empirical electron density models of the polar inter-plume and plume regions, as derived from the ground-based eclipse measurements of coronal polarization brightness.
      


The speed dependence of solar wind mass flux outputs, F, near the Sun (on the source surface, 2.5 solar radii) and in the heliosphere(at 1AU) was analyzed by combining observations of the interplanetary scintillation(IPS)and K─coronameter data during Carrington rotations(1643-1652) in 1976 and was compared with the photosphere magnetic field for the same period. The basic results are that: (1) the speed dependence of F is differen for various speed ranges and magnetic structures: the dependence first rises for<470...

The speed dependence of solar wind mass flux outputs, F, near the Sun (on the source surface, 2.5 solar radii) and in the heliosphere(at 1AU) was analyzed by combining observations of the interplanetary scintillation(IPS)and K─coronameter data during Carrington rotations(1643-1652) in 1976 and was compared with the photosphere magnetic field for the same period. The basic results are that: (1) the speed dependence of F is differen for various speed ranges and magnetic structures: the dependence first rises for<470 km/s; the dependence then decreases for 470-590 km/s; finally, the dependence is constant for>590 km/s; (2) these speed ranges basically correspond to different magnetic structured on the photosphere: strong magnetic field region, current sheet region, and polar corona region; (3) in particular, the polar corona region's mass flux is the lowest in the three different magnetic structure regions and is nearly constant in the range of 400-700 km/s.(4) the results mentioned above are similar both on source surface and in heliosphere and are also similar with the results in the descending phase of sloar activity.

以IPS速度、光球磁场、K─日冕偏振亮度和卫星实地观测数据为基础,综合生成处于太阳活动上升期的1976年10个太阳周(1643─1652卡林顿周)的源表面高度(R=2.5Rs,Rs为太阳半径)和日球空间中(IAU)太阳同质量流量速度谱。结果表明,速度谱存在与太阳活动上升期一致的"三段"结构,且各段分别与不同的磁结构区相对应。

The polarized character of coronal streamers in white light is investigated. It includes: the changes of typical polarized degree of coronal streamers with increasing radial distance;the distributions of white light brightness of coronal streamers along position angle in the same radius of solar disk, the polarized degree of coronal streamers in different solar latitudes, the inhomogenity of the distribution of polarization brightness in a coronal streamer.

研究了日冕白光冕流的偏振特性,包含:典型冕流的偏振度随日心距增大的变化;冕流白光亮度在同一日心距处沿日面位置角的分布;不同日面纬度处冕流的偏振度;冕流中偏振亮度分布的不均匀性.

The variation of the polarization brightness of coronal streamer in Carrington Rotations 1591-1592 is investigated. The distribution of the polarization brightness along streamer belts is inhomogeneous; the degree of the inhomogeneity is 10%-50%. In the absence of coronal mass ejection (CME) influence, the distribution of coronal streamers along the streamer belts can persist stable during nearly two Carrington Rotations. The rise velosity of the top of the cusp region in a coronal streamer may be more than...

The variation of the polarization brightness of coronal streamer in Carrington Rotations 1591-1592 is investigated. The distribution of the polarization brightness along streamer belts is inhomogeneous; the degree of the inhomogeneity is 10%-50%. In the absence of coronal mass ejection (CME) influence, the distribution of coronal streamers along the streamer belts can persist stable during nearly two Carrington Rotations. 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.

本文研究了卡林顿自转周1591 - 1592 中冕流偏振亮度的变化。冕流带偏振亮度的分布是不均匀的,不均匀度为10 % - 50 % 。无日冕物质抛射影响存在时,沿冕流带冕流的分布可持续稳定存在近两个太阳自转周。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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