暗条

暗条类似于太阳耀斑，亦或是某种磁结构。

The filaments may be analogous to solar flares or could be magnetic structures of some sort .

重连和蒸发的现象和过程可简述如下。Hα活动暗条上升并逐渐消失。

The processes could be described as follows : An active H α filament ascended and disappeared gradually .

而暗条F2一部分先消失，其余部分出现水平的轴向运动，最后F2整体爆发。

As for F2 , it partially disappeared and then the rest showed horizontal axial motion , and eventually erupted wholly . ( 2 ) The eruptive mechanisms of the two filaments are different .

综述了近年来人们对磁浮现与耀斑，暗条，CME等太阳表面磁活动的相关关系的研究进展。

The paper mainly overviews the recent years progress on the relationship between flux emergence and solar surface activity phenomenon , such as flares , prominence , coronal mass ejections ( CMEs ) .

结果表明：（1）1986年2月4日的3B／X3耀斑可能是由暗条电流环之间的合并不稳定性所致；（2）电阻撕裂模不稳定性是一种有效的耀斑前预热机制；

The results show that ( 1 ) The 3B / X3 flare on Feb.4 , 1986 was possibly caused by the current loop coalescence instability between two filament current loop s : ( 2 ) The resistive tearing instability is an efficient Pre-heating mechanism of pre-flare phase ;

黑子暗条旋转速度的轴向分布

The Axial Distribution of the Rotational Velocity of a Sunspot Filament

直流电场采油矿场试验暗条上升运动与电场直接加速

The Ascending Motion of the Filament and the Direct Electric Field Acceleration

暗条电流演化和耀斑储能

The evolution of filament current and sources of flare energy

一般回路形式下的暗条电流平衡高度

The Balance Altitude of the Filament Current Within A General Current Circuit

两个活动区电流暗条的平衡

The Balance of the Current Filament in the Two Solar Active Regions

太阳暗条激活与爆发的观测研究

The Observational Study of Activations and Eruptions of Solar Filament

暗条模型中暗条电流纵向分量的考虑

Investigation of the vertical component of the filament current circuit in filament models

该暗条爆发伴随有一个明显的双带耀斑。

The filament eruption was accompanied by a C9.6 X-ray class two-ribbon flare .

活动区新浮磁流和暗条的激活

Emergent magnetic flux and filament activation in active regions

导致太阳耀斑爆发的暗条扭绞

Twisting of a filament resulted in a solar flare

AR5572中一个宁静暗条的缠绕运动与磁场的关系

The Relation Between the Twisting Motion of a Quiescent Filament and the Magnetic Field

用三维运动学模式研究太阳暗条消失与行星际扰动太阳暗条活动的周期性研究

Relationship between filament disappearance events and interplanetary disturbances studied by a 3-D kinematic method

这表明螺旋磁场在扰动暗条中的存在可能是普遍的。

The fact suggests that twisted magnetic field may commonly exist in disturbed filament .

在耀斑开始很早以前，耀斑附近的暗条就变得活动起来。

The filament near the flare became active long before the start of the flare .

太阳暗条活动的周期性研究

Periodicities in Solar Filament Activity

耀斑具有双带结构，活动暗条被耀斑的双带包围在中间。

The flare has the two-ribbon structure , and the active filaments arc surrounded by the two ribbons .

暗条扰动与暗条通道中的光球运动和光球磁场变化有密切联系。

The filament disturbances are closely associated with photospheric displacement and changes of photospheric magnetic field in filament channel .

在一个左旋爆发暗条中，我们首次认证了其螺旋结构是左旋的。

For the first time , we identify that the helical structure appeared in an eruptive sinistral filament was left-helical one .

气孔的诞生和运动、黑子的挤压和剪切以及磁流的浮现和对消都可对暗条的失稳有贡献。

The pore birth and movement , the sunspots squeeze and shear , the magnetic flux emergence and cancellation may be all contributed to loss of filament stability .

而较长的宁静型暗条可能存在着缠绕结构，其运动较为复杂，旋转方向沿轴向发生变化。

And the winding structure of a longer quiet filament may exist , the motion of the filament is comparatively complex and the rotational direction alters along the axis .

本文对最近几年来暗条结构、动力学和磁场位形在观测和理论上的研究进展进行了回顾；

In the present paper , the observational and theoretical progresses in the more recent study of the structure , dynamics and magnetic field configuration of the filament are introduced .

本文给出了六个不同黑子暗条的旋转角速度、整体平移速度和它们的半径沿暗条轴的分布。

The distribution of the rotational angular velocities , the integral translational velocities and the radii along the filamentary axes of six different sunspot filaments are given in this paper .

本文根据无黑子双带耀斑发生前暗条周围色球纤维形态的观测特征，讨论了这类耀斑的储能过程。

In this paper , the energy storage for a spotless two ribbon flare is discussed from the morphology of chromospheric fibrils in the surrounding of filament prior to the flare .

浮现磁流、冲浪、暗条爆发和耀斑开始&1981年5月16日大耀斑的初相

The Emerging Magnetic Flux , the Surge , the Eruption of Filament and the Onset of Flare & The Initial Phase of the Great Two-Ribbon Proton Flare of May 16 , 1981

我们详细研究了几个扰动暗条的位形和动力学演化、相关的光球磁场和日冕结构的变化；以及相联系的耀斑发展。

It is studied for the detailed morphological and dynamic evolution of several disturbed filaments , the relevant changes of photospheric magnetic field and coronal structure , as well as the development of associated flares .