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ASCA相关的网络例句
与 ASCA 相关的网络例句 [注:此内容来源于网络,仅供参考]

During the long ASCA observation on NGC 4151 in 1995, Fe K line of NGC 4151 showed significiant varations despite of the relatively small amplitued varations in the X-ray continuum flux.

在1995年ASCA对NGC 151的观测中,铁线存在着显著的10〓秒尺度上的快速变化,而连续谱的变化幅度却很小。

Analysis of ASCA observation of the X-ray pulsar 1SAX J1324.4-6200, we get precise pulse period, and find that it is significantly larger than the pulse period determined from previous observations, agreed well with a linear spin-down of the pulsar.

对X射线脉冲星1SAX J1324.4-6200的ASCA观测作了分析,获得其准确的脉冲周期及周期的演化,指出它可能是一低质量X射线双星系统。

System volume flux was gained by loop integral the momentum equation. The simulation program was complied under the real-time simulation support system, ASCA.

在实时仿真支撑系统ASCA下编写了计算程序,通过改变程序运算速度达到实时的需要。

Upper limits to the pulsed component of these possible oscillations at the 3-sigma level inferred from the 1994 and 1999 ASCA data in 0.7-5 keV are 3.5x10^-14 erg/cm^2/sec and 1.9x10^-14 erg/cm^2/sec respectively, which are 12.4\% and 6.9\% of the source flux.

最后,依据不同的观测资料,对可能存在於中子星表面的波而言,我们给出3 倍标准差信心水准的能量通量上限:由1994、1999年ASCA的资料,得到3.5×10^-14 erg/cm^2/sec和1.9×10^-14 erg/cm^2/sec,分别为原来星体能量通量的12.4﹪和6.9﹪。

Apart from those characteristics already noticed in earlier ASCA observations on this object (Yaqoob et al. 1995): a broad and skewed profile, with a strong peak at about 6.4 kev and a large red wing extending to~4-5 keV, we also found a weak blue wing extending to about 8 keV.

除了较早的观测已经发现的特性(6.4keV的发射线峰以及延伸至约4.5keV的红翼,Yaqoob et al.1995)外,我们还发现了一个清晰的延伸至8keV的蓝翼。

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I didn't watch TV last night, because it .

昨晚我没有看电视,因为电视机坏了。

Since this year, in a lot of villages of Beijing, TV of elevator liquid crystal was removed.

今年以来,在北京的很多小区里,电梯液晶电视被撤了下来。

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我比喻得过头了。