1、

Characteristic analysis of auroral electrojet in Zhongshan station, Antarctic

南极中山站极光电集流分布特征分析

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2、

Geomagnetic responses to the convection field, field-aligned current and auroral electrojet

对流电场、场向电流和极光区电集流变化的地磁响应

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3、

To go mountaineering, or to visit the South Pole. CHARACTERISTIC ANALYSIS OF AURORAL ELECTROJET IN ZHONGSHAN STATION, ANTARCTIC

来南极登山,或者来南极观光。南极中山站极光电集流分布特征分析

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4、

The results from the synthetic analyses of geomagnetic data with 1-minute resolution along latitude and longitude chains indicate that the intensity and location of the auroral electrojet center vary frequently with UT and the local time sector.

对此纬度链和经度链上各站1min精度地磁资料的综合分析结果表明,极光区电集流中心的相对强度及其纬度位置是随世界时和地方时区不断变化的。

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5、

An international team of scientists have discovered that Saturn's ultraviolet auroral glow pulsates in time with its radio wave emissions, possibly signalling a ticking over of each Saturnian day.

近来有国际科学家小组发现,土星紫外极光频率与其射电脉冲频率一致,也许可以据此来确定土星一日的长短。

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6、

Storm-time Joule heating of auroral thermosphere and ionization depletion in the F-region ── eiscat radar observation

暴时极光区热层大气焦耳加热与F区电离耗空的EISCAT雷达观测

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7、

In contrast, variations of ion temperature are very different in the two regions, with little change in polar cap while strong enhancement in auroral oval, implying a difference in key mechanisms for the negative storms in the two regions.

但离子温度的变化在两个区域很不相同,在极光椭圆区大幅度升高,而在极盖区没有显著变化,反映出引起F区负暴的主要机制在两个区域不尽相同。

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8、

An all-Sky auroral video image analyzing system

极光全天空视频图像分析系统

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9、

Development of an all-sky auroral image processing and analyzing software

极光全天空图象处理和分析系统的软件开发

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10、

Direct for the stage. Today these particles lead to auroral displays.

为舞台演出进行指导。如今粒子导致极光出现。

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11、

A Representation of Form Features HISTORICAL PREAMBLE AND PRESENT STATE OF AURORAL SPECTROSCOPY

形状特征的表示极光光谱学发展史和现状

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12、

A simulation study on ionosphere affected by auroral particle precipitation in cusp region

极隙区极光粒子沉降对电离层影响的模拟研究

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13、

Two types of ionospheric disturbance in the auroral region

极光区电离层扰动的两种类型

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14、

Auroral particle precipitation and its spectra transport in the atmosphere in Antarctic region

极光粒子沉降研究:谱形式及其在极区大气中的传输

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15、
16、

Astronomers are now able to predict periods of high auroral activity by following solar events;

天文学家现在能通过追踪太阳的活动来预测极光现象的高峰期;

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17、

A study on the Zhongshan conjugate point location during auroral substorms

极光亚暴期间的南极中山站地磁共轭点位置研究

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18、

Today these particles lead to auroral displays.

如今粒子导致极光出现。

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20、

Auroral Kilometric Radiation and Auroral Hiss: DE-1 Observation Results

DE-1卫星对千米波辐射和极光嘶声的部分观测结果及分析

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