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    Meter Wavelength Characteristics of a Solar Active Region in August 1972
    1972年8月太阳活动区的米波特征
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    SOME CHARACTERISTICS OF SOLAR X-RAY FLARE ACTIVE REGION
    太阳X射线耀斑活动区的一些特征
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    PRELIMINARY STUDY OF ACTIVE STRUCTURE OF THE 1830 CIXIAN STRONG EARTHQUAKE AREA IN HEBEI PROVINCE
    1830年河北磁县强震区活动构造初步研究
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    Research on Relations Between Active Conjugate Tectonics and Earthquake in Linfen Area
    临汾地区共轭活动构造与地震关系的研究
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    GEOTHERMAL INFORMATION OBSERVATIONS IN NORTH TIANSHAN SEISMIC ACTIVE ZONES
    北天山地震活动区地热信息的观测与研究
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  the active
    The Study on the Active Faults in Hainan Island by Way of Fractal Theory
    用分形理论研究海南岛的活动断裂
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    Research on the relationship based on GIS between the distribution of the active faults and the seismicity in Jiangxi
    基于GIS的江西活动断裂分布与地震活动关系研究
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    STUDY ON NEW ACTIVITY CHARACTERISTICS OF THE ACTIVE FAULTS IN YINING BASIN OF XINJIANG
    新疆伊宁盆地活动断裂新活动特征研究
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    The Detection and the Study of the Active Faults in Zhangbei Earthquake Area
    河北张北地震区活动断裂的探测与研究
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    The II International Workshop of the Active Geophysical Monitoring of the Earth Lithosphere Held in Russian
    第二届国际地球岩石圈活动的地球物理监测研讨会在俄罗斯举行
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    The Corotating Variation of Heliospheric Quantities (I) -Average Features in the 20th Solar Cycle
    日球参数的卡林顿共转变化(Ⅰ)——第20太阳活动周的平均特性
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    Three Dimensional Propagation Characteristics of the Flare-Associated Interplanetary Shock Wave During 1978-1981
    太阳活动高年期间(1978—1981)耀斑-行星际激波传播的三维平均特性——日本行星际闪烁(IPS)观测的初步分析
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    The Corotating Variation of Heliospheric Quantities (II)——Evolutions in the Solar Cycle 20
    日球参数的卡林顿共转变化(Ⅱ)——在第20太阳活动周中的演变
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    THE PERIODICITY OF AR5395 EVOLUTION
    AR5395活动区演化的周期性
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    THE HEIGHT OF O+-H+ TRANSITION IN THE TOPSIDE IONOSPHERE AT SOLAR MAXIMUM
    太阳活动高年上电离层中O~+—H~+离子过渡高度的特征
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  active
The Design and Synthesis of a Novel, Orally Active, Selective ETA Antagonist
      
The pharmacokinetics of α- and β-diastereomers of Arteether, a well-known antimalarial drug and its active metabolite dihydroartemisinin (DHA) were studied in Sprague-Dawley rats, Rhesus monkeys and human volunteers.
      
The same compounds were studied using CoMFA for which the molecules were first aligned to a template molecule, which was most active in the series.
      
Among these compounds, 6-benzo[1,3]dioxol-5-yl-4-oxo-hex-5-enoic acid (3) was the most active one.
      
Only 15.33% of the cells was metabolically active at 200 μg/ml methanol extract while 23.57% of the cells was active at 200 μg/ml berberine.
      
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The 'active' compounds, which reduced growth of cancer cells to ca.
      
The resulting data were analyzed and suitable models were developed after identification of the active ranges.
      
Resulting data were analyzed and suitable models were developed after identification of the active ranges.
      
The active site and crystal nucleus are formed due to the comprehensive effect of electricity, thermodynamics and chemistry.
      
The active power P and the reactive power Q are obtained through the PQ transformation of the stator currents.
      
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本文为譜斑与地磁扰动对比关系的初步小結。文中对1942—1943年,1952—1953年重現性譜斑与磁扰进行了初步分析,可以看出,在太阳活动下降分支上譜斑为重現磁扰主要的来源,但不是唯一的来源,并由此推測粒子流速度为每秒300—500公里。

~~

本文根据农作物根系活动层的深度及农作物对土壤湿度的要求,以及土壤湿度与地下水位之間关系,論述水网或河网地区,利用河沟水位和地下水位变化,通过土壤毛管作用达到均匀湿潤土壤进行地下浸潤灌溉。分析連續浸潤灌溉时均匀湿潤土壤应具的河网水位地下水位及相应的間距,间歇浸润灌漑时河沟应抬高水位和地下水位以及充水日期和相应的間距等問題。

Flares of importance≥Ⅱ~+ are grouped according to their heliographic position and magnetic class of the active regions. By means of superposed-epoch method, we have calculated the mean daily frequency of Kp≥6 under different conditions. It is found that, for the magnetic group βγ+γ+β_f solar flares in northern hemisphere produce stronger corpulscular effect than those in southern hemisphere, but for the flares in β_p+β regions no such hemispheric asymmetry is found. Also, in southern hemisphere the western flares...

Flares of importance≥Ⅱ~+ are grouped according to their heliographic position and magnetic class of the active regions. By means of superposed-epoch method, we have calculated the mean daily frequency of Kp≥6 under different conditions. It is found that, for the magnetic group βγ+γ+β_f solar flares in northern hemisphere produce stronger corpulscular effect than those in southern hemisphere, but for the flares in β_p+β regions no such hemispheric asymmetry is found. Also, in southern hemisphere the western flares have stronger effect than the central and eastern ones, but in northern hemisphere only those flares in β_p+β regions have this E—W asymmetry. Those asymmetrical relations appear in all of the last three solar cycles, and it is especially conspicuous during equinoxes.

本文探討了耀斑日面位置与磁扰关系的不对称性。經分析研究,得到(βγ+γ+β_f)型活动区耀斑的磁扰效应有明显的南北不对称性,但(β_p+β)型活动区耀斑却无此南北不对称效应。在太阳南半球,不論那种磁場类型活动区,发生在西边的耀斑要比东西或中心子午线附近耀斑的影响强,而在北半球只有(β_p+β)型活动区耀斑才有这种东西不对称性效应。在最近三个太阳黑子周內,这些不对称是經常存在的,而在春秋季表現最为明显。

 
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