Detection of a variable interstellar absorption component towards δ Orionis A

Observations of δ Ori A made with the UHRF in its highest resolution mode ( R ≈900 000) have revealed the presence of a cool ( T _k350 K) variable absorption component at a heliocentric velocity of +21.3 km s⁻¹. The component is detected in Na  i D₁, where clear hyperfine splitting is seen, and Ca  ii K. Comparison of our data with existing spectra suggests that the component has consistently increased in strength from 1966 to 1994, and subsequently reduced in intensity by 1999. Following a discussion of the possible origins of this component it is concluded that an interstellar, rather than circumstellar, origin is most likely. This is one of very few detections of variable interstellar absorption reported in the literature, and we suggest an origin within filamentary material associated with the expanding H  i shell surrounding the Orion–Eridanus superbubble.     

一种提高大高差短基线精度的方法

提出采用半参数模型解算大高差短基线,削弱残余对流层误差的影响。算例表明,与常规最小二乘法相比,采用半参数模型处理基线能很好地分离GPS残余对流层误差,提高基线解算精度。     

Letter to the Editor: The collisional broadening of carbon radio recombination lines

The density matrix equations of highly excited carbon are analytically solved as functions of line number and temperature. Allowing for the series of the impact approximation theory and quadrupole interaction potential, the line widths are found with the theoretical error less than 0.06 in the range of temperatures T _e = 25 − 100 K. To determine the medium temperature and density by using the experimental values of line widths, the Doppler, radiational and impact broadening are calculated for the lines with the principal quantum numbers n > 300. This revised version was published online in July 2006 with corrections to the Cover Date.     

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超新星在星际^26Al问题中的作用：星际^26Al的天体源泉问题之三

讨论了迄今超新星爆发现论中各种爆炸性核燃烧核合成＾２６Ａｌ的问题。评述了星际＾２６Ａｌ天体起源的ＳＮＩＩ＋ＳＮＩｂ模型的有利因素和不足之处。最后提出一种产生星＾２６Ａｌ的新途径和有关部分星际＾２６Ａｌ起源于ＳＮＩａ的初步设想。     

不同对流层天顶延迟模型在中国西北地区适应性研究

基于Fortran语言对GAMIT10.7软件进行二次开发,实现了Hopfield模型、Saastamoinen模型、Black模型、UNB3模型、EGNOS模型、GPT2w_1+ Saastamoinen模型和GPT2w_5+ Saastamoinen模型在中国西北地区的对流层延迟解算服务,并分析不同对流层延迟模型在...     

Tropospheric Ozone in a Global-Scale Three-Dimensional Lagrangian Model and Its Response to NOX Emission Controls

A three-dimensional Lagrangian tropospheric chemistry modelis used toinvestigate the impact of human activities on the tropospheric distributionofozone and hydroxyl radicals. The model describes the behaviour of 50 speciesincluding methane, carbon monoxide, oxides of nitrogen, sulphur dioxide andnineorganic compounds emitted from human activities and a range of other sources.Thechemical mechanism involves about 100 chemical reactions of which 16 arephotochemical reactions whose diurnal dependence is treated in full. The modelutilises a five minute chemistry time step and a three hour advection timestepfor the 50,000 air parcels. Meteorological data for the winds, temperatures,clouds and so on are taken from the UK Meteorological Office global model for1994 onwards. The impacts of a 50% reduction in European NO_Xemissions onglobal ozone concentrations are assessed. Surface ozoneconcentrations decrease in summertime and rise in wintertime, but to differentextents.     

基于GPT3模型的ZTD及PWV反演精度分析

使用亚洲区域18个IGS测站和中国区域内16个探空站2016~2018年的数据,研究GPT3模型反演天顶对流层延迟（ZTD）和大气可降水量（PWV）的精度,并与其他GPT系列模型进行对比。结果表明,GPT3-1模型估计的ZTD的bias均值和最大值均最小,分别为1.34 mm和14.06 mm;GPT3模型整体精度略优于GPT2w模型,优于GPT2模型。探空站处GPT3模型反演的PWV的bias和RMSE均表现出较强的季节性特征;由GPT3模型反演的PWV的月均值可知,GPT3-1模型比GPT3-5模型具有更高的精度和稳定性。     

测站间高差对短时段GPS基线解算的影响

基于美国CORS网数据,分别选取平均基线长度和站间高差均不相同的6个GPS实验网,使用GAMIT/GLOBK软件,从基线较差、基线重复性、NRMS值以及解算中误差等方面分析站间高差对短时段（4 h）GPS基线解算的影响及削弱这些影响的方法。结果得出,当测站间高差大于100 m时,如果不估计对流层参数,即使是短基线也会使解算基线在高程方向的偏差达到1 cm,而对平面分量影响很小。此时,必须通过估计天顶方向的对流层参数来削弱其影响,才能保证最终解算的基线结果在高程方向的误差小于1 cm。