太阳磁场

太阳磁场望远镜中KD~P电光调制器

The KD P modulator in the solar magnetic field telescope

太阳磁场是指分布于太阳大气中的磁场。

Solar magnetic field means the magnetic field in the solar atmosphere .

CCD在太阳磁场测量中的应用

CCD is sun magnetic field measurement

在太阳磁场大气中FeIλ5324.19（？）谱线的形成深度

Fel λ 5324.19 (?) Line Depth of Formation in the Solar Magnetic Field

本文最后还对红外CCD、紫外CCD、弱光CCD在太阳磁场测量和太阳恒星磁场观测的应用进行了介绍。

In the end , the applications of infrared CCD , ultraviolet CCD and weak-light CCD in the observation of sun magnetic field and sun stellar magnetic field are introduced .

这段时期被称作”蒙德极小期”（“MaunderMinimum”），这个时期的出现被认为与一个长期的太阳磁场活动完全停滞的太阳周期紧密相连。

This period is known as the " Maunder Minimum ," and it is thought to be tied into a long-term cycle where the sun 's magnetic activity shuts down .

本文以线性无力场模式下边界元法（BEM）为基础，根据Carrington1733&1742周的光球磁场观测数据，计算出相应各Carrington周日冕高度（2.5R＿⊙）全日面的太阳磁场。

In this paper we calculated the global coronal ( at 2.5 R ⊙) magnetic field of Carrington rotations 1733-1742 using the boundary element method ( BEM ) under the linear force-free field model , based on photospheric magnetic field observations .

太阳磁场演变的起因之一&太阳的回磁效应

A Cause of Evolution of Solar Magnetic Field & Solar Gyromagnetic Effect

太阳磁场的红外研究

The study of solar magnetic fields in infrared spectral region

局部相关跟踪算法在太阳磁场观测中的应用

Application of LCT in Solar Magnetic Field Observation

有关太阳磁场的无力场模型及计算方法研究

The Research of Force-free Field Models and Computational Methods for the Solar Magnetic Field

太阳磁场望远镜的进展

The progress of the solar telescope - magnetograph

太阳磁场观测研究

A Research on Observation of Solar Magnetic Field

太阳磁场和宇宙线实验规律初探

Laboratory ; The Preliminary Study on the Experimental Regularity between Solar Magnetic Field and Cosmic Ray

由于大气抖动和望远镜自身精度的原因，太阳磁场望远镜在进行图像叠加时会出现误差。

However , because of atmospheric agitation and telescope accuracy , there are errors during overlapping all images .

与此同时，有些研究者利用磁光效应来研究太阳磁场。

At the same time , some researcher study the magnetic of sun on the basis of magneto-optic effect .

结束语对我国的红外太阳磁场研究提出一些建议。

In the conclusion some suggestions are proposed for the infrared study of solar magnetic fields in our country .

太阳磁场磁性指数异常变化对南北半球中纬度气候的影响

Influence of magnetic index abnormal change in the solar magnetic field on climate at the middle latitudes of North Hemisphere

文章作者认为，是缠绕的太阳磁场提供了足够的能量，使这些日冕物质可以克服恒星的重力以及周边磁场的束缚抛射出来；

We believe that it is the twisted magnetic field that stores enough free magnetic energy for a CME to erupt .

地球磁场像太阳磁场一样由发电机的作用而产生，这包括两个过程。

The Earth 's field , like the sun 's , is produced by dynamo action , which involves two processes .

一旦到达太阳磁场强烈的日冕处，这些轴子又会转变为光子。

Once at the solar corona , where the sun 's magnetic field is strong , the axions would convert back into photons .

法拉第效应对利用怀柔磁场望远镜观测的矢量磁场计算电流螺度的影响。太阳磁场的观测（英文）

The effect of Faraday rotation on the helicity computation using observations from the Solar Magnetic Field Telescope at the Huairou Solar Observing Station .

本文介绍了用于观测太阳磁场的天文望远镜系统的高速高精度局部级联式多阈值A/D转换器。

A high-speed high-accuracy partially-cascaded A / D converter is developed , which is used with the telescope for observing the solar magnetic field .

分析认为，这是地球海洋温度场对太阳磁场周期性变化的响应。

It is believed that this is the response of the globe marine temperature field to the periodic changes of the solar magnetic field .

本文综述了与恒星磁场测量有关的、太阳磁场若干观测特征。

In this paper , we have reviewed the observational characteristics of solar magnetic fields in these aspects which are relevant to stellar magnetic field measurements .

在太阳磁场观测系统中通过使用相关跟踪算法发现并消除原始图像间的抖动错位，提高磁场观测数据的空间分辨率。

Correlation tracking method is applied in the solar observing system in order to find the displacements among image series and improve the spatial resolution of the magnetogram .

每隔11年，太阳磁场活动便会加强，有时更会变得狂暴形成巨大的太阳黑子及强烈的太阳风暴。而此时此刻我们应该是出于太阳磁场活动最高峰的阶段。

Every 11 years , the sun 's magnetic activity ramps up , sometimes to a frenzy , causing large sunspots and strong flares . Right now we should be in the middle of such a solar maximum .

系统采用局部相关跟踪算法来提高磁场观测数据的空间分辨率，同时对相关跟踪算法的实现程序进行了优化以满足常规太阳磁场观测的要求。

The Correlation Tracking ( CT ) method is used in this system to improve the spatial resolution , and the algorithm of CT is optimized to improve the temporal resolution for the purpose of routine observation of solar magnetic field .

简要回顾了螺度引入太阳磁场研究中的历史过程，从物理角度讨论了相对磁螺度这个新的可观测量，并指出其在理论和观测中存在的问题；

This paper reviews the history of magnetic helicity studies and its concepts introduced into solar physics . With the physical discussions on a new measurable quantity ( relative magnetic helicity ), some problems in both theory and observations are pointed out .

太阳磁场磁性周期变化趋势略有超前，分析认为，这是南半球对流层大气气候系统对太阳磁场周期性变化的响应。

The periodic variation of solar magnetic field leads in phase slightly . Based on analysis it is known that this is the response of the atmosphere climate system of the troposphere in the Southern Hemisphere to the periodic variations of the solar magnetic field .