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491.
492.
Record ozone loss was observed in the Arctic stratosphere in spring 2020. This study aims to determine what caused the extreme Arctic ozone loss. Observations and simulation results are examined in order to show that the extreme Arctic ozone loss was likely caused by record-high sea surface temperatures(SSTs) in the North Pacific. It is found that the record Arctic ozone loss was associated with the extremely cold and persistent stratospheric polar vortex over February–April, and the extremely cold vortex was a result of anomalously weak planetary wave activity. Further analysis reveals that the weak wave activity can be traced to anomalously warm SSTs in the North Pacific. Both observations and simulations show that warm SST anomalies in the North Pacific could have caused the weakening of wavenumber-1 wave activity, colder Arctic vortex, and lower Arctic ozone. These results suggest that for the present-day level of ozone-depleting substances, severe Arctic ozone loss could form again, as long as certain dynamic conditions are satisfied. 相似文献
493.
494.
The high observation efficiency, scanning speed and observation frequency of the Fengyun-4A(FY-4A) satellite indicates the progress of Chinese geostationary meteorological satellites. The characteristics of FY-4A atmospheric motion vectors(AMVs) derived from the high-level water vapor(WV-High) channel, mid-level water vapor(WV-Mid) channel,and infrared(IR) channel of FY-4A are analyzed, and their corresponding observation errors estimated. Then, the impacts of single-channel and multi-channel FY... 相似文献
495.
T. V. Shabanova 《Monthly notices of the Royal Astronomical Society》2005,356(4):1435-1439
Three slow glitches in the rotation rate of the pulsar B1822−09 were revealed over the 1995–2004 interval. The slow glitches observed are characterized by a gradual increase in the rotation frequency with a long time-scale of several months, accompanied by a rapid decrease in the magnitude of the frequency first derivative by ∼1–2 per cent of the initial value and subsequent exponential increase back to its initial value on the same time-scale. The cumulative fractional increase in the pulsar rotation rate for the three glitches amounts to Δν/ν0 ∼ 7 × 10−8 . 相似文献
496.
本文介绍了TMS320C25高速接口电路的设计方法,并以高速A/D接口为例,说明接口电路设计中的一些技巧。这对充分利用TMS320C25的硬件资源有非常重要的意义。 相似文献
497.
用中国科学院大气物理研究所高分辨率、自由表面热带海洋环流模式对厄尼诺/南方涛动(El/SouthernOscillation)循环中另一重要位相La 事件进行了数值模拟研究。模式区域为南北纬30°之间的热带太平洋,经纬圈水平方向分辨率分别为2°和1°,垂直方向分为不等距的14层;模式中考虑了盐度并引入与洋流切变和层结稳定度有关的垂直扩散参数化方案。在观测到的海表风应力、热量和淡水通量(蒸发与降水之差)驱动下,所发展的模式从1984年积分到1989年。本文给出模式对近十几年来最强的1988年La事件进行数值模拟的结果,着重分析La期间热带太平洋海面起伏、流场和温度场时空演变,以及La和El期间变量场时空结构差别。文中还进行了模式结果和一些观测资料间的比较。 相似文献
498.
本文阐述了A村金矿点的地质环境及其金矿化特征和矿化类型,认为该金矿点是与花岗岩类岩石有关的金矿化类型。关在研究其成矿条件的基础上,提出了若干寻找同类型金矿的找矿标志。 相似文献
499.
卢伙胜 《广东海洋大学学报》1995,(2)
在假设手纲、空纲成直线状,浮纲、沉纲呈悬链线状的前提下,利用悬链线各因素与手纲冲角之间的相互制约关系,确立了计算单船底拖网作业手纲冲角近似值的逐步校正法。并推广应用于双船底拖网作业中的曳纲水平冲角、空纲的水平冲角、上袖端的内倾率、上片网衣在沉纲前上方的遮盖面积以及遮盖率等的近似值计算。 相似文献
500.
Rong-Feng Shen † Li-Ming Song Zhuo Li 《Monthly notices of the Royal Astronomical Society》2005,362(1):59-65
We compute the temporal profiles of the gamma-ray burst pulse in the four Burst and Transient Source Experiment (BATSE) Large Area Detector (LAD) discriminator energy channels, with the relativistic curvature effect of an expanding fireball being explicitly investigated. Assuming an intrinsic 'Band' shape spectrum and an intrinsic energy-independent emission profile, we show that merely the curvature effect can produce detectable spectral lags if the intrinsic pulse profile has a gradually decaying phase. We examine the spectral lag's dependences on some physical parameters, such as the Lorentz factor Γ, the low-energy spectral index, α, of the intrinsic spectrum, the duration of the intrinsic radiation t 'd and the fireball radius R . It is shown that approximately the lag ∝Γ−1 and ∝ t 'd , and a spectrum with a more extruded shape (a larger α) causes a larger lag. We find no dependence of the lag on R . Quantitatively, the lags produced from the curvature effect are marginally close to the observed ones, while larger lags require extreme physical parameter values, e.g. Γ < 50 , or α > −0.5 . The curvature effect causes an energy-dependent pulse width distribution but the energy dependence of the pulse width we obtained is much weaker than the observed W ∝ E −0.4 one. This indicates that some intrinsic mechanism(s), other than the curvature effect, dominates the pulse narrowing of gamma-ray bursts. 相似文献