活动太阳

Ap指数在2004也显示出54天周期，这样一来，地磁活动和太阳活动一起影响密度变化中的54天周期。

The Ap index also shows 54-day periodicities in 2004 , and magnetic activity , together with solar irradiance , affects the 54-day variation in density significantly .

地磁活动与太阳活动对环电流离子成分与位置的影响

Effect of geomagnetic activity and Solar-cycle variation on the ring current ions

太阳活动和太阳全辐射热之间的相关

The relativity between solar activity and total solar radiation

磁暴活动与太阳黑子的相关性

On magnetic storm coincided with sunspot activity

辽西地震活动与太阳黑子活动的相关性分析

The correlation discussion of seismicity in the west of Liaoning Province and the sunspots activity

你只不过看到了激烈活动的太阳上数千个年轻的耀斑之一。

You are envisioning just one of thousands of young spicules on the active Sun .

质子活动与太阳黑子群

Proton Activities and Sunspot Groups

相对于地磁活动，太阳活动对闪烁活动的影响相对不明显。

Compared with the geomagnetic activity , the solar activity did not evidently affect the scintillation occurrence .

本论文首先概述了太阳活动、太阳射电研究历史及现状、射电辐射理论等相关背景知识；

Of this dissertation , we introduce the background of solar activity , solar radio research and radio emission theory . In Chap.

从而，建立起反映太阳活动的太阳10.7cm辐射流量与卫星轨道摄动的关系模型。

Then the relation model between satellite orbit perturbation and 10.7 cm solar radio flux , which reflects solar activity , is established .

四月份的群马地区春寒料峭，然而活动当天太阳却露出笑脸，天气显得出奇地暖和。

Springtime in Gunma is usually chilly , but on that day , the sun appeared with a cheerful smile and made the weather comfortably warm .

但是，把时钟调快一个钟头，相对于人类的其他活动，太阳似乎能晚点升起也晚点下山。

But , by moving the clocks forward an hour , compared to all other human activity , the sun will seem to both rise and set later .

太阳活动由太阳大气中的电磁过程引起，时强时弱，平均以11年为周期，活动剧烈期的太阳活动有太阳黑子和耀斑。而现在我们本应该处于一个太阳活动极大期。

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

双极黑子活动区中太阳射电SVC辐射

Solar radio SVC radiation in an active region of bipolar sunspot

本文着重讨论了已往大气中~（14）C浓度的长期、中期和短期变化，以及这些变化与地球磁场的变化、人为活动因素、太阳活动和气候变化等的密切关系。

In this paper , we discuss the long , medium and shortterm changes of 14C concentration in the atmosphere in the past , and their relations with the fluctuations of the earth 's magnetic dipole moment , human activities , solar activities and the change of climate .

太阳活动低年太阳风的空间结构

Spatial structure of solar wind during minimum phase of solar activity

来自6538活动区的太阳射电米波事件

Solar Radio Metric Wave Events From Active Region 6538

对试图解释太阳活动起源的太阳发电机理论作了综合评述。

The Theories of various solar dynamos to explain the origin of solar activity are reviewed .

太阳黑子的出现周期是每11年一次，这个周期性活动同时改变太阳的磁场。

The11-year solar cycle , which governs the appearance of sunspots , also changes the sun 's magnetic field .

在某种意义上说，活动区是太阳活动的基本单位，也是太阳磁性最持久的和看得见的表现形式。

Active regions are in a sense the fundamental unit of solar activity and the most persistent and visible manifestation of solar magnetism .

它利用普遍存在于自然界和人类活动中的太阳光为能量，不需要接入公共电网。

Without accessing to public power grid , Solar lighting system uses sunlight that common exist in nature and human activities as its energy .

特大风暴潮的形成不仅与台风和天文大潮密切相关，而且还与太阳活动（如太阳黑子的变化）有关。

Their occurring are closely linked with not only the appearance of typhoon and highest astronomical tide , but also solar activity like sunspot burst .

然而，这些研究只是向我们展示了很短一段时间内的太阳活动情况，太阳在我们的研究所覆盖的这3年内的活动可能是一种反常现象。

However , they only show us a snapshot of the Sun 's activity and its behavior over the three years of our study could be an anomaly .

用模式识别方法研究了大地震的发生时间与中等地震活动性、太阳活动水平、地球自转之间的关系。

A pattern recognition algorithm has been used to correlate the occurrence time of a large earthquake to intermediate-size earthquake activity , to the level of sunspot activity and the rotation of the earth .

本文综述了太阳活动周期、太阳活动延伸周、太阳活动预报和太阳活动在日面上分布等有关太阳长期活动规律的理论研究；

We Summarize the theoretical studies of long-term solar activity on sunspot cycle , extended cycle , the prediction of solar activity and the asymmetric distribution of solar activity on the hemisphere and present the results of our studies on the long-term solar activity .

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 .

探索太阳活动的规律、太阳耀斑及其伴随CME的先兆、触发过程及能量传播机制等等，从理论上推动了等离子体天体物理、磁流体力学等诸多基础理论的发展，有着重要的理论意义；

Theoretical researches on solar activity , solar flare and CME were involved in many fields of foundational physics such as plasma astrophysics , magnetohydrodynamics ( MHD ) and so on .

太阳活动越剧烈，太阳风越强烈。

The more active the Sun , the stronger the solar wind .

太阳活动区参量与太阳耀斑和太阳质子事件的相关性统计分析

Statistic Analysis on Solar Activity Parameters with Solar Flare and Solar Proton Event

研究结果表明，太阳活动所引起的太阳辐射、地磁指数等的变化，与对流层大气所出现的异常降水事件有一定的对应。

The results show that variations of solar radiation and geomagnetic index correspond to the abnormal precipitation events in troposphere .