太阳物理

海水太阳池物理模型

Physical Model of Seawater Solar Pond

传统上，光谱观测是太阳大气物理参数诊断的主要方法。

Traditionally the primary means to measure the parameters of the solar atmosphere is via spectroscopic observations .

宇宙线强度随时间的变化，是宇宙线物理、太阳地球物理和天体物理等交叉学科中的重要问题之一。

The time variation of the cosmic ray flux is one of crucial problems in the field of cosmic ray physics , solar geophysics and astrophysics , etc.

本文概略地评述了近年来太阳耀斑物理预报和有关的太阳耀斑理论的进展，也介绍了这些理论在太阳预报中应用的可能性。

In this paper we briefly review the progress in the physical forecast of solar flares and related theories in recent years . Possible applications of these theories to solar flare forecast are also given .

根据低频夭波实测资料和实验结果的分析表明：引起低频夭波信号的幅度与相位产生突然异常的原因，与太阳地球物理现象有关。

It is shown from the analyses of the observed data of LF skywaves and the experimental results that the reason why the amplitude and phase of the LF skywaves become suddenly abnormal is related to the solar-geophysical phenomenon .

现在常用白光日冕仪的观测来研究日冕物质抛射的传输和演化过程，因而如何恰当地理解白光日冕仪中的CME的观测特征对太阳和空间物理领域的许多相关研究至关重要。

Observations of white-light coronagraphs are widely used to study the propagation and evolution of CMEs , and thus how to properly understand CMEs viewed in white-light coronagraphs is crucial to many relative researches in solar and space physics .

电化掺杂制作太阳电池的物理机理

Physical basis of solar cell fabricating by electrochemical doping of impurities

太阳耀斑的物理预报

The Physical Forecast of Solar Flares

太阳-地球物理特别委员会

Special Commission on Solar-Terrestrial Physics

挠性太阳帆板为物理仿真部分，用来产生扰动力矩。

Flexible solar panels device consist of the part of loop simulation , which is used to generate disturbing moment .

太阳和天体物理吸积盘中的磁场是一种空间间歇的磁流。

It is shown that magnetic fields in the Sun and astrophysical accretion disks are of a spatially intermittent nature .

建立了海水太阳池的物理模型，分析了太阳池内的基本热平衡模型，双对流扩散模型和湍流卷吸运动模型。

The model of seawater solar pond was build up , and the basic heat balance model , double-diffusive process model and turbulent entrainment model were analyzed .

为了进一步探索太阳对流区的物理性质，我们利用高精度N的日震观测数据来研究太阳内部扰动磁场对低阶太阳P模振动的影响。

To investigate the physical nature of solar convective zone , we employ the observed frequency shifts of solar oscillations to study the influence of magnetic perturbation inside the Sun on the low solar p mode oscillations .

总结了非晶硅太阳电池在器件物理、制造工艺、大规模生产和应用方面所取得的重大进展。文章分析了非晶硅太阳电池作为空间能源系统技术上的主要优势；

The great progresses on device physics , manufacturing process , mass production and application on amorphous silicon solar cells were summarized .

通过模式不同版本之间的相互比较研究，可以发现模式中太阳辐射日变化物理过程的引入明显地改善了表面空气温度的模拟，尤其是在中低纬度的陆地上。

Through intercomparisons among different versions of the model , it can be clearly seen that the incorporation of the diurnal cycle of solar radiation apparently improves the simulation of SAT , especially in the low and middle latitudes over land .

本论文针对海水非对流型盐梯度太阳池主要做了如下的工作：1.建立了海水太阳池的物理模型，分析了太阳池内的基本热平衡模型，双对流扩散模型和湍流卷吸运动模型。

This thesis has carried out the following work about the seawater solar pond : 1.The model of seawater solar pond was build up , and the basic heat balance model , double-diffusive process model and turbulent entrainment model were analyzed .