solar magnetic field

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

太阳磁场是指分布于太阳大气中的磁场。

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

有关太阳磁场的无力场模型及计算方法研究

A Research on Observation of Solar Magnetic Field

太阳磁场观测研究

Progress in the Studies on a Relic Solar Magnetic Field

太阳剩余磁场研究进展

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

太阳磁场演变的起因之一&太阳的回磁效应

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

在太阳磁场大气中FeIλ5324.19（？）谱线的形成深度

Application of LCT in Solar Magnetic Field Observation

局部相关跟踪算法在太阳磁场观测中的应用

The KD P modulator in the solar magnetic field telescope

太阳磁场望远镜中KD~P电光调制器

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

太阳磁场和宇宙线实验规律初探

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

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

It is believed that this is the response of the globe marine temperature field to the periodic changes of 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。

Some Perspective views and complements on the paper [ 3 ] are made , which may improve our understanding the computation problem of solar magnetic field .

对关于太阳线性无力场评注和快速傅氏分析法的应用的评论一文，提出一些看法和补充，以增进对无力场计算太阳磁场问题的进一步的认识。

The measurement of solar magnetic field and the non-potential characteristic of solar activity are important to explain the physical mechanism and dynamical process of solar activity .

因此，太阳活动区磁场测量和非势特征的研究对理解太阳表面上各种活动现象的物理机制和动力学过程有着十分重要的意义。

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

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）

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

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。

In this paper , we introduce a recently finished image-processing system for the high-resolution observation of solar magnetic field in the Huairou Solar Observing Station ( HSOS ) .

文章介绍了怀柔太阳观测基地最近完成的一套实时高分辨太阳磁场观测系统。

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 .

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。

Results from spectral analysis on time sequences show that the reddish-grey rhythmic deposits were controlled by decade-or century-level climatic periods which might be related to several astronomic cycles , such as sunspot or solar magnetic field .

经频谱分析等时序分析法的估算可知该红灰韵律层是受十年级与百年级主周期的控制，可能与太阳黑子或太阳磁场活动等天文周期有关。

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 .

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 upper level abnormal changes of climate in the stratosphere have a marked period of 22 years , which is considered as the response of atmosphere temperature field to abnormal changes of solar magnetic field with a period of 22 years . The variance contribution rate exceeds 9 % .

平流层高空气候异常变化还具有显著的22年变化周期，分析认为是大气温度场对太阳磁场磁性周期22年异常变化的响应，其方差贡献率超过9%。

In the process of observation of solar magnetic field , the sun itself enters into the telescope and the effective amount of light related to the magnetic field is very limited . In order to improve SNR ( Signal to Noise Ratio ), the captured images must be overlapped .

在太阳磁场观测中，太阳本身进入望远镜的与磁场有关的有效光量是有限的，为了提高信噪比，需要将采集到的图像进行多帧叠加。

Research on Fast Algorithms and Their Application to Solar Force-free Magnetic Field

有关太阳无力磁场的快速算法应用研究

A Synthesized Method for Determining the Azimuth of Solar Transverse Magnetic Field

确定太阳横向磁场方位角的综合方法

Amongst these , one of the most important problem is to solve the boundary value problem for the solar force-free magnetic field equation .

这其中最重要的一个问题就是通过数值方法求解太阳无力磁场方程的边值问题。

A MHD model of 2-D structure of solar wind and magnetic field output on source surface

太阳等离子体和磁场输出源表面结构的一种MHD模型

Some comments are made on the computation of solar active region magnetic field in the last thirty years , especially on some errors in linear force-free field representations .

首先对30年来用无力场计算太阳活动区磁场方法作了一些评注，特别研究了线性无力场解中的几个误区。

The Primary Results of Research on Solar Oscillations by Using Magnetic Field Telescope

用磁场望远镜研究太阳振荡的初步结果

On the energy storage in the solar atmosphere by twisting magnetic field

太阳大气中磁场的扭转储能

Visit mercury , and you will be visiting the only other planet in the inner solar system with a magnetic field .

访问水星，你就是访问仅有的另一个在太阳系内部有磁场屏障的形星。

In the space solar telescope ( SST ), the image integration method is used to increase signal-to-noise ratio ( SNR ) of the solar magnetic field images .

空间太阳望远镜（SST）系统采用图像积分方法提高太阳矢量磁图的信噪比（SNR）。