LAMOST望远镜的大气色散校正

大气折射与大气色散会影响大视场多目标光纤光谱观测的质量和效率.一个焦距为20m,焦比为F5、位于北纬40.4°的LAMOST望远镜在中天和中天前后0.75小时产生的色散值,用模拟计算得到结果,并用数值计算得到验证.对校正色散可能用的几种色散棱镜进行了计算分析比较,确定了色散棱镜的型式,并分析了色散棱镜的二级光谱以及色散棱镜在望远镜跟踪过程中的残留色散,及色散棱镜的安装误差.     

Synchronization of perturbed non-linear Hamiltonians

We propose a new method based on Lie transformations for simplifying perturbed Hamiltonians in one degree of freedom. The method is most useful when the unperturbed part has solutions in non-elementary functions. A non-canonical Lie transformation is used to eliminate terms from the perturbation that are not of the same form as those in the main part. The system is thus transformed into a modified version of the principal part. In conjunction with a time transformation, the procedure synchronizes the motions of the perturbed system onto those of the unperturbed part.A specific algorithm is given for systems whose principal part consists of a kinetic energy plus an arbitrary potential which is polynomial in the coordinate; the perturbation applied to the principal part is a polynomial in the coordinate and possibly the momentum.We demonstrate the strategy by applying it in detail to a perturbed Duffing system. Our procedure allow us to avoid treating the system as a perturbed harmonic oscillator. In contrast to a canonical simplification, our method involves only polynomial manipulations in two variables. Only after the change of time do we start manipulating elliptic functions in an exhaustive discussion of the flows.     

Improvements for group delay fringe tracking

Group delay fringe tracking using spectrally dispersed fringes is suitable for stabilizing the optical path difference in ground-based astronomical optical interferometers in low light level situations. We discuss the performance of group delay tracking algorithms when the effects of atmospheric dispersion, high-frequency atmospheric temporal phase variations, non-ideal path modulation, non-ideal spectral sampling, and the detection artifacts introduced by electron-multiplying CCDs are taken into account, and we present ways in which the tracking capability can be optimized in the presence of these effects.     

Canonical planetary perturbation equations for velocity-dependent forces,and the Lense-Thirring precession

A form of planetary perturbation theory based on canonical equations of motion, rather than on the use of osculating orbital elements, is developed and applied to several problems of interest. It is proved that, with appropriately selected initial conditions on the orbital elements, the two forms of perturbation theory give rise to identical predictions for the observable coordinates and velocities, while the orbital elements themselves may be strikingly different. Differences between the canonical form of perturbation theory and the classical Lagrange planetary perturbation equations are discussed. The canonical form of perturbation theory in some cases has advantages when the perturbing forces are velocity-dependent, but the two forms of perturbation theory are equivalent if the perturbing forces are dependent only on position and not on velocity. The canonical form of the planetary perturbation equations are derived and applied to the Lense Thirring precession of a test body in a Keplerian orbit around a rotating mass source.     

Magnetic measurements of recent sediments from Big Moose Lake,Adirondack Mountains,N.Y., USA

Measurements of anhysteretic (ARM) and isothermal (IRM) remanences in cores 6 and 8 from Big Moose Lake reveal evidence for changes in magnetic mineralogy and grain size within and between the two cores. It is proposed that changes in the strength and demagnetization characterizations of the IRM reflect the accumulation of atmospherically deposited magnetic minerals resulting from industrial processes. The record of magnetite deposition especially in Core 6 parallels that for coal soot at the site. In both cores, the record of haematite deposition parallels that for several anthropogenic indicators.This is the fourth of a series of papers to be published by this journal which is a contribution of the Paleoecological Investigation of Recent Lake Acidification (PIRLA) project. Drs. D. F. Charles and D. R. Whitehead are guest editors for this series.     

2017年12月大气环流和天气分析

2017年12月大气环流的主要特征如下：北半球极涡呈偶极型分布,欧亚中高纬环流呈两槽一脊型;南支槽位于70°E 附近,较常年同期偏西,副热带高压位置偏西,不利于水汽向我国中东部地区输送。12月,全国平均降水量为5.9 mm,比常年同期（10.8 mm）偏少44.8%,我国北方大部分地区降水量较常年同期偏少4~8成。全国平均气温-2.2℃,较常年同期（-3.2℃）偏高1℃;受偏强东北低涡影响,东北地区和内蒙古中东部气温较常年同期偏低1~3℃。月内,冷空气活动频繁,但强度较弱,出现5次一般强度冷空气过程。受频繁冷空气影响,雾 霾天气较常年同期偏少,仅28—30日出现一次大范围持续性雾 霾天气。     

非洲地区大气气溶胶光学厚度时空变化及亚速尔高压对沙尘越大西洋传输的影响

研究了非洲地区大气气溶胶光学厚度（AOD）的时空变化及沙尘气溶胶越大西洋海区的传输。结果表明：1）源于撒哈拉沙漠的沙尘及其随赤道东风向西输送使得沙尘气溶胶成为非洲沙漠地区和紧邻的大西洋海区的主要气溶胶组分;AOD高值区和沙尘气溶胶光学厚度高值区在1—7月随赤道辐合带北移同步向北移动,而在8—12月则向南回撤。2）刚果盆地大气气溶胶主要为热带雨林和稀树草原排放的有机碳（OC）和黑碳（BC）气溶胶;其中与生物质燃烧源排放有关的OC、BC高值主要集中在干季（6—9月）的后半段（8—9月）;而生物源OC排放全年连续,其排放峰值出现于雨季开始时;生物质燃烧排放高值期与生物源排放高值期前后相继,形成干季（尤其是后半段）时期的OC、BC光学厚度高值。3）亚马逊河入海口地区主要气溶胶组分为海盐气溶胶,9—11月该区风力输送增强,风向由东南风转变为东风,海盐进入亚马逊河入海口处,形成AOD和海盐气溶胶光学厚度高值区。4）撒哈拉沙漠沙尘气溶胶向大西洋传输的偏北月份为7—9月、偏南月份为1—3月;2000—2016年海区沙尘气溶胶的传输路径存在向南移动的变化趋势,与同期亚速尔高压的增强和沙尘传输路径以北北风分量的增强以及赤道辐合带的移动一致。上述研究结果揭示了利用大气气溶胶时空变化特征反映区域大气环流和气候变化的可能性。     

气候变化背景下山东大气自净能力特征分析

利用山东22个基本（准）气象站小时气象观测资料,采用A值法计算了山东1961—2017年逐日大气自净能力指数（the atmospheric self-purification capacity index,ASPC）,分析了其气候空间分布特征和时间演变规律,利用MK检验（Mann-Kendall检验）和MT检验（Moving-t,滑动t检验）方法对历年ASPC进行了突变检验。结果表明：平均ASPC气候倾向率减小趋势极显著(P<0.01),除章丘和威海外,其他各地ASPC减小趋势均极显著(P<0.01);春季各月ASPC较大,历年各月ASPC随时间明显减小;年和四季ASPC空间分布基本一致,半岛地区较大,鲁南等内陆地区相对较小;年和春、夏、秋、冬季ASPC突变年份分别出现在2003年和2006年、2003年、2003年、2005年。济南、青岛地区ASPC分别从1999年、1993年开始显著减小,低ASPC日数历年变化大致与ASPC变化相反;济南和青岛历年各月ASPC变化差异明显。     

Atmospheric Response to Mesoscale Ocean Eddies over the South China Sea

The South China Sea(SCS) is an eddy-active area. Composite analyses based on 438 mesoscale ocean eddies during 2000–2012 revealed the status of the atmospheric boundary layer is influenced remarkably by such eddies. The results showed cold-core cyclonic(warm-core anticyclonic) eddies tend to cool(warm) the overlying atmosphere and cause surface winds to decelerate(accelerate). More than 5% of the total variance of turbulent heat fluxes, surface wind speed and evaporation rate are induced by mesoscale eddies. Furthermore, mesoscale eddies locally affect the columnar water vapor, cloud liquid water, and rain rate. Dynamical analyses indicated that both variations of atmospheric boundary layer stability and sea level pressure are responsible for atmospheric anomalies over mesoscale eddies. To reveal further details about the mechanisms of atmospheric responses to mesoscale eddies, atmospheric manifestations over a pair of cold and warm eddies in the southwestern SCS were simulated. Eddy-induced heat flux anomalies lead to changes in atmospheric stability. Thus, anomalous turbulence kinetic energy and friction velocity arise over the eddy dipole, which reduce(enhance) the vertical momentum transport over the cold(warm) eddy, resulting in the decrease(increase) of sea surface wind. Diagnoses of the model's momentum balance suggested that wind speed anomalies directly over the eddy dipole are dominated by vertical mixing terms within the atmospheric boundary layer, while wind anomalies on the edges of eddies are produced by atmospheric pressure gradient forces and atmospheric horizontal advection terms.     

集合预报最优ETKF初始扰动方法设计及其在暴雨中的应用

为改进集合转换卡尔曼滤波方法(Ensemble Transform Kalman Filter,ETKF)在初始扰动中离散度偏小的问题,考虑引入物理不确定性。使用初始时刻离散度检验两种ETKF初始扰动方案改进的程度,通过动力和水汽条件分析探求改进机制。利用WRF模式构建更新预报系统,选取2014年5月一次暴雨个例进行集合降水预报试验,通过ETKF方法设计两种不同的初始扰动方案。结果表明:在分析循环中引入多物理扰动的初始扰动方案(multi)相比单一物理过程的初始扰动方案(mono)在初始时刻离散度和模拟动力水汽条件以及降水评分上均有较大改进。初始扰动中multi的离散度相比mono整体更优,显然添加了多物理扰动方案的试验对结果有改进作用;在对两种方案的机理分析中,multi对于降水位置的明显改善主要取决于散度及水汽通量散度模拟能力的提高;在离散度分析中,multi方案在强对流区域的改进效果比在整个区域中的更好,而对各变量的离散度和均方根误差之比相当,说明集合预报系统的合理性;对各量级预报结果评分显示,multi方案均呈现较好表现能力。