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1.
L. Kristensen 《Boundary-Layer Meteorology》1979,16(2):145-153
It is demonstrated that the longitudinal spectral coherence differs significantly from the transversal spectral coherence
in its dependence on displacement and frequency. An expression for the longitudinal coherence is derived and it is shown how
the scale of turbulence, the displacement between observation sites and the turbulence intensity influence the results. The
limitations of the theory are discussed. 相似文献
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运动质点的多普勒效应使它们散射的雷达信号呈现为一种随机过程,对这随机过程的统计特性进行分析就能够推断云和降水的微物理或运动学的状况。本文由这种观点讨论了雷达气象的几种测量原理,它能够比较清楚地阐明每种方法的实质,也便于对各种方法的优缺点进行对比。文中还讨论了脉冲波列的谱分析问题,涉及了如何根据雷达测量结果去推断云和降水的微物理或运动学状况的问题。 相似文献
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V. Hisdal 《Theoretical and Applied Climatology》1959,10(1):59-68
Summary Spectral intensities of the scattered radiation from the zenith sky were measured using a filter monochromator. The monochromator was calibrated by means of a tungsten-filament lamp with known spectral energy distribution. The intensities of the individual wave-bands were referred to the total radiation intensity in the wave range considered, i. e. all spectral distributions were adjusted so as to give a constant total radiation. The relative intensity distributions obtained in this way are discussed. The results indicate that the relative intensity in a wave-band around 460 m is to a large extent independent of the atmospheric scattering conditions.
With 4 Figures 相似文献
Zusammenfassung Die spektrale Intensität der gestreuten Himmelsstrahlung des Zenithimmels wurde mit einem Filtermonochromator gemessen; der Monochromator wurde mittels einer Wolframbandlampe mit bekannter Energieverteilung geeicht. Die Intensität der einzelnen Wellenlängenbereiche ist auf die totale Strahlungsintensität des untersuchten Bereichs bezogen, d. h. alle spektralen Verteilungen wurden so umgerechnet, daß sie eine konstante Gesamtstrahlung ergaben; die in dieser Weise erhaltenen relativen Intensitätsverteilungen werden diskutiert. Die Resultate lassen erkennen, daß die relative Intensität in einem Wellenbereich um 460 m in hohem Maße von den Verhältnissen der atmosphärischen Streuung unabhängig ist.
Résumé On mesure l'intensité spectrale de la lumière diffuse du ciel provenant du zénith à l'aide d'un monochromateur à filtre étalonné au moyen d'une lampe au wolfram à spectre énergétique connu. L'intensité des diverses régions spectrales est rapportée à l'intensité totale du domaine étudié, c'està-dire que toutes les distributions spectrales ont été calculées de façon à donner un rayonnement total constant. Les distributions relatives ainsi obtenues front l'objet d'une discussion qui montre que, dans un domaine centré sur 460 m, l'intensité relative est dans une large mesure indépendante des conditions de la dispersion atmosphérique.
With 4 Figures 相似文献
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Martin Claussen 《Boundary-Layer Meteorology》1985,33(3):233-243
From measured one-dimensional spectra of velocity and temperature variance, the universal functions of the Monin-Obukhov similarity theory are calculated for the range –2 z/L + 2. The calculations show good agreement with observations with the exception of a range –1 z/L 0 in which the function
m
, i.e., the nondimensional mean shear, is overestimated. This overestimation is shown to be caused by neglecting the spectral divergence of a vertical transport of turbulent kinetic energy. The integral of the spectral divergence over the entire wave number space is suggested to be negligibly small in comparison with production and dissipation of turbulent kinetic energy.Notation a,b,c
contants (see Equations (–4))
- Ci
constants i=u, v, w, (see Equation (5)
- kme,kmT
peak wave numbers of 3-d moel spectra of turbulent kinetic energy and of temperature variance, respectively
- kmi
peak wave numbers of 1-d spectra of velocity components i=u, v, w and of temperature fluctuations i=
- ksb, kc
characteristics wave numbers of energy-feeding by mechanical effects being modified by mean buoyancy, and of convective energy feeding, respectively
- L
Monin-Obukhov length
- % MathType!MTEF!2!1!+-% feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn% hiov2DGi1BTfMBaeXafv3ySLgzGmvETj2BSbqefm0B1jxALjhiov2D% aebbfv3ySLgzGueE0jxyaibaiiYdd9qrFfea0dXdf9vqai-hEir8Ve% ea0de9qq-hbrpepeea0db9q8as0-LqLs-Jirpepeea0-as0Fb9pgea% 0lrP0xe9Fve9Fve9qapdbaqaaeGacaGaaiaabeqaamaabaabcaGcba% Gabeivayaaraaaaa!3C5B!\[{\rm{\bar T}}\]
difference of mean temperature and mean potential temperature
- T*
Monin-Obukhov temperature scale
-
velocity of mean flow in positive x-direction
- u*
friction velocity
- u, v, w
components of velocity fluctuations
- z
height above ground
-
von Kármanán constant
-
temperature fluctuation
- m
nondimensional mean shear
- H
nondimensional mean temperature gradient
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nondimensional rate of lolecular dissipation of turbulent kinetic energy
- D
nondimensional divergence of vertical transports of turbulent linetic energy 相似文献
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I. Matyasovszky 《Theoretical and Applied Climatology》2010,101(3-4):281-287
The paper discusses a methodology able to estimate both the discrete and continuous spectra without any assumption on the shape of spectral densities. The approach to estimate the spectral density is based on a robust smoothing of the periodogram. Bandwidth, a quantity similar to the width of spectral windows traditionally used in spectral analysis, is estimated locally in contrast to intuitively chosen global window lengths. Detection and estimation of frequencies forming discrete spectra are also addressed. The procedure is applied to Central England temperature (CEt), North Atlantic Oscillation (NAO) index and Oxygen Isotope of North Greenland Ice Core Project (δ18O of NGRIP) data. Annual and half annual cycles were detected in CEt data, whilst 118.2- and 41.7-ky cycles were found in δ18O of NGRIP. This latter periodicity is almost as intense as the dominant longer cycle. Several local peaks of spectral densities were recognised in each time series that mostly cover earlier results. However, a few previous findings at low frequencies have not been reinforced by the present method. Identification of modest local peaks or discrete amplitudes at low frequencies is an extremely challenging task as climatic data generally have spectral densities rising to low frequencies. 相似文献
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1/f noise in the UV solar spectral irradiance 总被引：1，自引：1，他引：0
Costas A. Varotsos Irina Melnikova Maria N. Efstathiou Chris Tzanis 《Theoretical and Applied Climatology》2013,111(3-4):641-648
The investigation of the intrinsic properties of the solar spectral irradiance as a function of the ultraviolet (UV) wavelength is attempted by exploiting rare observations performed at the Villard St. Pancrace station of the Lille University of Sciences and Technology ranging from 278 to 400 nm with a step of 0.05 nm every half an hour from nearly sunrise to sunset. To achieve this goal, the modern method of the detrended fluctuation analysis was applied on the solar spectral irradiance values versus wavelength. This analysis revealed that the solar incident flux at the top of the atmosphere and the solar spectral irradiance at the ground during two overcast sky days fluctuate with the UV wavelength exhibiting persistent long-range power-law behavior. More interestingly, the exponent of the power-law relationship between the fluctuations of the solar spectral irradiance versus UV wavelength at both the top of the atmosphere and the ground is consistently close to unity (of 1/f-type) throughout the day. This 1/f behavior has been detected in many complex dynamical systems, but despite much effort to derive a theory for its widespread occurrence in nature, it remains unexplained so far. According to the above-mentioned findings we speculate that the 1/f property of the incident solar UV flux at the top of the atmosphere could probably drive both the 1/f behavior depicted in the atmospheric components and the solar UV irradiance at the Earth's surface. The latter could influence the UV-sensitive biological ecosystems, giving rise to a 1/f-type variability in the biosphere, which has already been proven by recent observational data. We finally propose that Wien approximation could be multiplied by a 1/f function of wavelength (e.g., of the type of the fractional Brownian motion) in order to reproduce the aforementioned 1/f feature of the solar UV flux. 相似文献
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Klaus Hasselmann 《Boundary-Layer Meteorology》1974,6(1-2):107-127
Summary The effect of white capping on the spectral energy balance of surface waves is investigated by expressing the white-cap interactions in terms of an equivalent ensemble of random pressure pulses. It is shown first that the source function for any non-expansible interaction process which is weak-in-the-mean is quasi-linear. In the case of white capping, the damping coefficient is then shown to be proportional to the square of the frequency, provided the wave scales are large compared with the white-cap dimensions. The remaining free factor is determined indirectly from consideration of the spectral energy balance. The proposed white-capping dissipation function is consistent with the structure of the energy balance derived from JONSWAP, and the existence of a
–5 spectrum governed by a non-local energy balance between the atmospheric input, the nonlinear energy transfer and dissipation. However, closure of the energy balance involves hypotheses regarding the structure of the atmospheric input function which need to be tested by further measurements. The proposed set of source functions may nevertheless be useful for numerical wave-prediction. According to the model, nearly all the momentum transferred across the air-sea interface enters the wave field. For fetchlimited and fully developed spectra in a stationary, uniform wind field, the drag coefficient remains approximately constant. However, for more general wind conditions, this will not be the case and the wave spectrum should be included in an accurate parameterisation of the air-sea momentum transfer.Contribution from the Sonderforschungsbereich Meeresforschung Hamburg of the Deutsche Forschungsgemeinschaft. 相似文献
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Parameterizations of different hydrometeor spectral relative dispersion in the convective clouds 
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下载免费PDF全文 Qinyao Zou Lei Zhu Chunsong Lu Guang J. Zhang Xiaoqi Xu Qian Chen Dan Li 《大气和海洋科学快报》2022,15(3):100141
Spectral relative dispersion of different hydrometeors is vital to accurately describe sedimentation. Here, the Weather Research and Forecasting model with spectral bin microphysics is used to simulate convective clouds in Shouxian of Anhui province in China to study the spectral relative dispersion of different hydrometeors. Firstly, regardless of clean or polluted conditions, the relative dispersion of ice crystal spectra and its volume-mean diameter are negatively correlated, while the relative dispersion of other hydrometeor spectra is positively related to their respective volume-mean diameter. The correlations for cloud droplets and raindrops are affected by the process of collision–coalescence; the correlations for ice crystals, graupel particles, and snow particles could be affected by the deposition, riming, and aggregation processes, respectively. Secondly, relative dispersion parameterizations are developed based on a comprehensive consideration of the relationships between the relative dispersion and volume-mean diameter under both polluted and clean conditions. Finally, the relative dispersion parameterizations are applied to terminal velocity parameterizations. The results show that for cloud droplets, ice crystals, graupel particles, and snow particles, assuming the shape parameter in the Gamma distribution is equal to 0 underestimates the shape parameter and overestimates the relative dispersion; and for raindrops, assuming the shape parameter is equal to 0 is close to the relative dispersion parameterizations. The most appropriate constant shape parameters are recommended for different hydrometeors. The relative dispersion parameterizations developed here shed new light for further optimizing the terminal velocity parameterizations in models.摘要离散度的诊断对模式中沉降过程的准确描述至关重要. 本文利用WRF模式结合谱分档方案模拟安徽寿县地区的对流云, 研究不同水成物的离散度. 首先, 无论在清洁还是污染条件下, 除冰晶谱的离散度与体积平均直径间呈现负相关关系外, 云滴, 雨滴, 霰粒子与雪粒子谱离散度与体积平均直径呈现正相关关系; 云滴和雨滴受碰并过程影响, 冰晶, 霰粒子和雪粒子分别受凝华过程, 淞附过程和聚并增长影响. 其次, 综合考虑污染与清洁条件下离散度和体积平均直径之间的相关关系, 建立了离散度的参数化方案. 最后, 把该离散度方案应用到下落末速度的参数化方案中, 结果表明, 对于云滴, 冰晶, 霰粒子和雪粒子, 在Gamma分布中假设谱形参数等于0会低估谱形参数而高估离散度. 对于雨滴而言, 假设谱形参数等于0与参数化方案结果接近. 针对不同的水成物, 给出了最合适的谱形参数定值. 本文发展的离散度方案为进一步优化模式中下落末速度参数化方案提供参考. 相似文献
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Summary A sun photometer fitted with 9 narrowband interference filters from 368 nm to 1024 nm was used to determine the aerosol optical depth at 8 measuring stations in Europe. Of the 9 filters, 4 were not included in the standard equipment of the sun photometer. Given the temporal instabilities of the calibration factors of these 4 filters, meaningful results for the aerosol optical depth can be achieved only if calibration and measurements follow each other closely. Calibration was performed using the Langley plot method. For wavelengths < 500 nm, the measured aerosol optical depths were compared with the results of a high resolution spectrometer. Broadband aerosol optical depths, centred at 427 nm, were determined with an actinometer and were also used for comparison. Generally, there was good agreement of the results. To characterize the aerosol optical depths, the Ångström parameters and were used. The individual measuring stations showed a clustered distribution of and values.With 6 Figures 相似文献
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T.-Y. Koh B. C. Bhatt K. K. W. Cheung C. K. Teo Y. H. Lee Matthias Roth Purnawirman 《Meteorology and Atmospheric Physics》2012,115(1-2):35-45
This study evaluates the spectral scaling of a heavy rainfall event and assesses the performance of the Coupled Ocean/Atmosphere Mesoscale Prediction System (COAMPS) model in terms of the multiscale variability of rainfall in the temporal spectral domain. The event occurred over southern Malay Peninsula on 18 December 2006 and was simulated at high resolutions. 10, 5 and 1?min aggregate rainfall data from rain gauge stations in Singapore and simulated rainfall sampled at different evaluation points on 0.9, 0.3 and 0.1?km grids were utilized. The simulated and observed rain rates were compared via Fourier and wavelet analyses. A scaling regime was noted in the observed rainfall spectra in the timescales between 60?min and 2?min. The scaling exponent obtained from the observed spectra has a value of about 2, which may be indicative of the physics of turbulence and raindrop coalescence and might suggest the predominance of a characteristic raindrop size. At 0.9?km resolution, the model rainfall spectra showed similar scaling to the observed down to about 10?min, below which a fall-off in variance was noted as compared to observations. Higher spatial resolution of up to 0.1?km was crucial to improve the ability of the model to resolve the shorter timescale variability. We suggest that the evaluation of dynamical models in the spectral domain is a crucial step in the validation of quantitative precipitation forecasts and assessing the minimal grid resolution necessary to capture rainfall variability for certain short timescales may be important for hydrological predictions. 相似文献
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Summary This work presents a statistical study of the wind power potential of three stations in the Catalonia area (Spain) over the 1973–1982 period. These stations correspond to three airports (Barcelona, Palma de Mallorca and Girona), which obviously do not present a high wind power potential and are not the suitable locations for wind power utilization, but which have been chosen for the long record of data stored (10 years). The aim of this work is to provide a model of wind potential in terms of the speed and wind direction, which may be applied to other sites. The wind speed has been modelled by a Weibull distribution function and the wind direction by a normal two-dimensional function. A spectral analysis of both variables has also been carried out. The present study provides an evaluation of the local wind power in the geographic area of Catalonia.With 10 Figures 相似文献
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The radiation budget at the top of the atmosphere plays a critical role in climate research. Compared to the broadband flux, the spectrally resolved outgoing longwave radiation or flux(OLR), with rich atmospheric information in different bands,has obvious advantages in the evaluation of GCMs. Unlike methods that need auxiliary measurements and information, here we take atmospheric infrared sounder(AIRS) observations as an example to build a self-consistent algorithm by an angular distribution model(ADM), based solely on radiance observations, to estimate clear-sky spectrally resolved fluxes over tropical oceans. As the key step for such an ADM, scene type estimations are obtained from radiance and brightness temperature in selected AIRS channels. Then, broadband OLR as well as synthetic spectral fluxes are derived by the spectral ADM and validated using both synthetic spectra and CERES(Clouds and the Earth's Radiant Energy System) observations. In most situations, the mean OLR differences between the spectral ADM products and the CERES observations are within ±2 W m~(-2), which is less than 1% of the typical mean clear-sky OLR over tropical oceans. The whole algorithm described in this study can be easily extended to other similar hyperspectral radiance measurements. 相似文献
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The equation of turbulent diffusion is solved for a vertical area source within the planetary boundary layer. The traditional Gaussian-plume approach is compared with the spectral solution of the diffusion equation used together with the barotropic boundary-layer model of Lettau and Dabberdt (1970). The results of the numerical computations are presented and the differences between the solutions are discussed. 相似文献