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天波时延
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  sky wave time delay
     Relationships Between the Variation of the Solar Constant and the Solar Soft x-ray Radiation and LF Sky Wave Time Delay
     太阳常数的变化与太阳软x射线辐射流量及低频天波时延的关系
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  “天波时延”译为未确定词的双语例句
     The measurements of the time delay of the 100 kHz one hop sky wave, transmittedfrom the Y station (26°13' N, 128°09' E) of Loran-C North-West Pacific Chain and received at Lintong (34°22' N, 109°13' E), and the solar 1 ~8 A x-ray flux measured bySMS-GOES are compared with the solar constant measured by SMM/ACRIM I.
     本文对1982年在陕西临潼接收的美国罗兰-C西北大平洋链Y台发射的100kHz低频一跳天波时延的实测资料及SMS-GOES测量的太阳1~8A软x射线的每日辐射流量与SMM/ACRIMI测量的太阳常数之间的关系进行了分析。
短句来源
     The comparisons and analyses show that the negative correlation exists between the solar 1~8Ax-ray flux and the solar constant, while the time delay of LF one hop sky wave is positively correlated with the solar constant.
     结果表明:太阳1~8A软x射线辐射流量与太阳常数之间存在较强的负相关; 低频一跳天波时延与太阳常数之间存在着较强的正相关。
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  相似匹配句对
     Accurate Measurement of the Loran-C LF Sky-wave Propagation Time-delay by an indirect Method
     罗兰—C天波传播时延的间接法精确测量
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     Stability of networked control systems with time-delay
     时延网络控制系统的稳定性
短句来源
     Delay Characteristics for the Asynchronous Tranfer Mode
     异步传送模式的时延特性
短句来源
     (3) Thereare no obvious changes for the LF sky wave signals during the initial phase of the magmetic storms ;
     (3)在磁暴初相时,低频天波信号的时延、场强无明显的变化;
短句来源
     Review and Description of the Sky Wave Over The Horizon Radar
     天波超视距雷达评述
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The analyses on the relationship between the variation of LF sky-wave signal and thegeomagnetic activities are conducted based on the data of geomagnetic activities and themeasuremants of the 100kHz one hop sky wave, transmitted from the Y station (26°36'N,128°09'E) of Loran-C North West Pacific Chain and received at Lintong (34°22'N, 109°13'E). The results show that: (1 ) The variations of the time delay and field strength of thelow frequency sky wave signal are usually obvious when the daily average index...

The analyses on the relationship between the variation of LF sky-wave signal and thegeomagnetic activities are conducted based on the data of geomagnetic activities and themeasuremants of the 100kHz one hop sky wave, transmitted from the Y station (26°36'N,128°09'E) of Loran-C North West Pacific Chain and received at Lintong (34°22'N, 109°13'E). The results show that: (1 ) The variations of the time delay and field strength of thelow frequency sky wave signal are usually obvious when the daily average index of the geomagnetic disturbance,AP, is high; (2) On the days when the magnetic storms reach themain phase, the LF sky wave signals mostly changed. Usually, the variations of the signals are larger if the geomagnetic storms reach main phaSe at night, while the those of thesignal are smaIler if the geomagnetic storms reach main phase during daytime; (3) Thereare no obvious changes for the LF sky wave signals during the initial phase of the magmetic storms ; (4)The varlation of the time delay of low frequency one hop sky wave, is positively correlated with the H value, the maximum of the horizontal component of thegeomagnetic field for the main phase of magnetic storm. These results are discussed in thepaper.

基于临潼(34°22'N,109°13'E)对来自冲绳(26°36'N,128°09'E)的100kHz低频一跳天波的时延及场强的实测,并利用相应的地磁扰动等资料、进行了有关低频天波信号变化与地磁活动的关系的分析研究。结果表明:(1)当地磁扰动的日平均指数较高时,低频天波信号的时延、场强的变化也较为明显;(2)磁暴达主相的当日,低频天波信号的时延、场强大多有明显变化,并且对延、场强的变化还与低频天线反射点处于白天还是夜晚有关,若处于夜晚,天演变化较大。若处于白天,变化较小;(3)在磁暴初相时,低频天波信号的时延、场强无明显的变化;(4)低频一跳天渡时延变化值与磁暴主相最大变幅H值有较好的正相关。

The measurements of the time delay of the 100 kHz one hop sky wave, transmittedfrom the Y station (26°13' N, 128°09' E) of Loran-C North-West Pacific Chain and received at Lintong (34°22' N, 109°13' E), and the solar 1 ~8 A x-ray flux measured bySMS-GOES are compared with the solar constant measured by SMM/ACRIM I. The comparisons and analyses show that the negative correlation exists between the solar 1~8Ax-ray flux and the solar constant, while the time delay of LF one hop sky wave is positively correlated...

The measurements of the time delay of the 100 kHz one hop sky wave, transmittedfrom the Y station (26°13' N, 128°09' E) of Loran-C North-West Pacific Chain and received at Lintong (34°22' N, 109°13' E), and the solar 1 ~8 A x-ray flux measured bySMS-GOES are compared with the solar constant measured by SMM/ACRIM I. The comparisons and analyses show that the negative correlation exists between the solar 1~8Ax-ray flux and the solar constant, while the time delay of LF one hop sky wave is positively correlated with the solar constant. These results are discussed in the paper.

本文对1982年在陕西临潼接收的美国罗兰-C西北大平洋链Y台发射的100kHz低频一跳天波时延的实测资料及SMS-GOES测量的太阳1~8A软x射线的每日辐射流量与SMM/ACRIMI测量的太阳常数之间的关系进行了分析。结果表明:太阳1~8A软x射线辐射流量与太阳常数之间存在较强的负相关;低频一跳天波时延与太阳常数之间存在着较强的正相关。并对此进行了讨论。

 
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