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31.
The analytical solutions of the continuous accretion rate equation are compared regarding two different size distributions for cloud and rain water, two hail terminal velocities for different turbulent regimes and two solution types. The Khrgian-Mazin and Marshall-Palmer size distributions are assumed for rain water fraction, while the Khrgian-Mazin and monodisperse ones are applied to cloud water. In all cases the exponential-type size distribution for hail is used. In the calculation procedure for hail terminal velocity we take into consideration that the drag coefficient may be fixed or dependent on Reynolds number. Both approximate and exact solutions of the accretion rate under the same other conditions are also compared.Results show that the Khrgian-Mazin size distribution makes the approximate accretion rate between hail and rain considerably higher compared to its former parameterization for both hail terminal velocity assumptions. On the other side, the new treatment of hail terminal velocity with a variable drag coefficient produces lower accretion rates compared to the fixed drag coefficient case for all size distributions used. The approximate solution of the accretion rate equation is mainly lower than the exact one. Only in the case of raindrops-cloud droplets interaction it is much higher than the exact one with the Khrgian-Mazin size distribution used. 相似文献
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In this paper, we discuss known discrepancies between theoretically derived and empirically measured relations between the radio surface brightness Σ and the diameter D of supernova remnants (SNRs): these relations are commonly known as the Σ–D relations. We argue that these discrepancies may be at least partially explained by taking into account thermal emission at radio frequencies from SNRs at particular evolutionary stages and located in particular environments. The major contributions of this paper may be summarized as follows: (i) we consider thermal emission at radio frequencies from SNRs in the following scenarios: a relatively young SNR evolving in a dense molecular cloud environment (n 100–1000 cm−3) and an extremely evolved SNR expanding in a dense warm medium (n 1–10 cm−3). Both of these SNRs are assumed to be in the adiabatic phase of evolution. We develop models of the radio emission from both of these types of SNRs and each of these models demonstrate that through the thermal bremsstrahlung process significant thermal emission at radio frequencies is expected from both types of SNR. Based on a literature search, we claim that thermal absorption or emission at radio frequencies has been detected for one evolved Galactic SNR and four young Galactic SNRs with similar properties to our modelled evolved and young SNRs. (ii) We construct artificial radio spectra for both of these two types of SNRs: in particular, we discuss our simulated spectrum for the evolved Galactic SNR OA 184. By including thermal emission in our simulated spectra, we obtain different slopes in Σ–D relations: these new slopes are in closer agreement to empirically obtained relations than the theoretically derived relations which do not take thermal emission into account. (iii) Lastly, we present an additional modification to the theoretical Σ–D relation for SNRs in the adiabatic expansion phase. This modification is based on the convolution of the synchrotron emissivity with the emissivity derived in this paper for thermal bremsstrahlung emission from an ionized gas cloud (that is, a theoretical construct of an SNR). 相似文献
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Dejan Vinkovi&#; &#;eljko Ivezi&#; Anatoly S. Miroshnichenko Moshe Elitzur 《Monthly notices of the Royal Astronomical Society》2003,346(4):1151-1161
We study the infrared (IR) emission from flared discs with and without additional optically thin haloes. Flux calculations of a flared disc in vacuum can be considered a special case of the more general family of models in which the disc is imbedded in an optically thin halo. In the absence of such a halo, flux measurements can never rule out its existence because the disc flaring surface defines a mathematically equivalent halo that produces the exact same flux at all IR wavelengths. When a flared disc with height H at its outer radius R is imbedded in a halo whose optical depth at visual wavelengths is τhalo , the system IR flux is dominated by the halo whenever τhalo > (1/4) H / R . Even when its optical depth is much smaller, the halo can still have a significant effect on the disc temperature profile. Imaging is the only way to rule out the existence of a potential halo, and we identify a decisive test that extracts a signature unique to flared discs from imaging observations. 相似文献
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A Global Approach to the Spatial Diversity and Dynamics of Internet Domains 总被引：1，自引：0，他引：1 
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下载免费PDF全文 Krzysztof Janc 《Geographical review》2016,106(4):567-587
The objective of this paper is to describe the place of individual countries in digital space through the lens of Internet domains and specific websites. We will discuss the global geography of domains in reference to states and other entities of spatial organization, and changes in the positions of individual websites. These issues will be approached with an awareness of the significant changes taking place in the functioning of the Web, particularly cyberbalkanization. This study mainly used data from Alexa rankings, the best free source of information available on the behavior of Internet users. One conclusion is the clear U.S. dominance over other countries in relation to number of most popular domains. Despite the clear U.S. dominance, the BRIC countries—Brazil, Russia, India, and China—play an increasingly significant role in the geography of domains. The trends discussed in this article are related to the so‐called balkanization of the Internet. Regulations of its functioning and the growing importance of national websites and search engines have contributed to deepening the differences between Internet users in different countries. 相似文献
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Abstract A kinematic model is applied to graupel growth. The vertical velocity and ther‐modynamic field data are taken from the forced 1‐D time‐dependent model of Cb cloud developed by Curie and Jane (1988). The graupel embryo pocket was released at the height of the — 10°C isotherm. The influence of the forced lifting on further graupel growth and its trajectory is analysed by sensitivity experiments based on the amplitude of the forced lifting, and initial graupel radius, density and cloud droplet concentration for the forced lifting initiation time derived from the model and the forced lifting duration time that agreed with observations. In particular, the sensitivity analysis was carried out for the forced lifting initiation and duration times. It is shown that for large values of the forced lifting amplitudes, the residence time of the graupel within cloud and the final graupel radius may be significantly larger compared with those in the non‐forced case. The residence time in a cloud can also be significantly larger for the smallest amplitude, whereas the final radius is rather insensitive owing to oscillations around the melting level. For some cases the forced lifting causes recycling inside the updraft, contrary to the results of previous non‐forced numerical models. The recycling mechanism is sensitive to the forced lifting duration time and the time interval between the graupel pocket injection in cloud and the initiation of the forced lifting. Initially the observed recycling mechanism is a consequence of the periodic forced lifting mechanism, but then combines with recycling of the Pflaum type (1980). 相似文献
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Vertical vorticity characteristics within individual cumulonimbus (Cb) cloud moving over complex terrain are investigated by cloud-resolving mesoscale model. Orography impact on vorticity is recognized by comparison of its characteristics within the storm moving over flat terrain under the same other conditions. In present study, two cases are considered: complex terrain case (referred to as CT case) and flat terrain case (referred to as FT case). A sensitivity study shows that orographical effects on vorticity are important. Main findings are:
- – For CT case vortices produced by convective tilting of horizontal vortices are closer to each other and more stretched in form owing to valley configuration. The vortex with positive vorticity is mainly stronger in magnitude compared to its negative counterpart.
- – Magnitudes of vorticities for CT case are greater at lowest levels and initial time intervals compared to those for FT case.
- – For CT case the vortices with opposite signs of vorticity produced by precipitation appear later than in FT case. Their duration is shorter and they are weaker in intensity compared to those formed within a cloud over flat terrain.
- – Complex terrain intensifies the splitting of simulated cloud.
Keywords: Mesoscale model; Vertical vorticity; Orography effects; Vortices 相似文献
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Cloud seeding projects may have the time scale of half a century and cover the planetary-scale surface. Such activities among the positive also have negative consequences that include environmental pollution. Year after year cloud seeding over certain areas could produce large amounts of seeding agents washed out in precipitation. The sampling of these deposits is therefore important, but not applied in large space and time scales due to a high cost. As an alternative, the cloud seeding project measurements may be used for finding the deposit spatial pattern and locations of its maximum. In this study, we established the method for finding the spatial distribution of deposited silver iodide over a selected area after hail suppression using the observed characteristics of seeded hailstorms. The estimation of the silver iodide deposit maximum is 155?μg?m?2 during a 6-year period. Our findings agree well with those obtained from sampling silver content in precipitation during the other convective cloud seeding experiments. On the other hand, our method gives an answer of where to place the samplers, and hence more detailed chemical analysis and monitoring can be done in the future. The proposed methodology may be applied for any other target area and cloud seeding scenario. 相似文献
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Mladjen Ćurić Dejan Janc Katarina Veljović 《Theoretical and Applied Climatology》2010,102(3-4):471-481
Convective precipitation is the main cause of extreme rainfall events in small areas. Its primary characteristics are both large spatial and temporal variability. For this reason, the monitoring of accumulated precipitation fields (liquid and solid components) at the surface is difficult to carry out through the use of rain gauge networks or remote-sensing observations. Alternatively, numerical models seem to be the most powerful tool in simulating convective precipitation for various analyses and predictions. Due to a lack of comparisons between modelled and observed precipitation characteristics over a long period of time, we focus our research on comparisons between observations and three model samples of accumulated convective precipitation over a particular study area. We use a numerical cloud model with two model schemes involving the unified Khrgian–Mazin size distribution of cloud drops and a model scheme involving a monodisperse cloud droplet spectrum and the Marshall–Palmer size distribution for raindrops, respectively. For comparison, we have selected a study area with a sounding site. Our analysis shows that the model version with the Khrgian–Mazin size distribution exhibits a better agreement with the observed mean, median and range of extreme values of accumulated convective precipitation. Model simulations with the Khrgian–Mazin size distribution most closely match observations, with a correlation coefficient of 0.91. Use of the Marshall–Palmer size distribution, on the other hand, systemically underestimates the observed precipitation and has the lowest correlation coefficient among the methods, 0.83. Such an investigation is crucial to improve predictions of accumulated convective precipitation for various climatological and hydrological analyses and predictions. 相似文献
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Summary A one-dimensional kinematic model is used to investigate the effects of silver iodide seeding in the region of a Cb cloud between isotherms of –8°C and –12°C. The agent interaction with cloud atmosphere is simulated by an improved microphysical model version which includes phoretic processes. The behaviour of the different agent types is investigated using the maximum values of agent mixing ratios and corresponding agent particle masses and radii.It is shown that the agent residence time in the seeding zone significantly depends on vertical velocity. The residence time is comparable to that previously reported. On the other side, the final graupel production decreases slightly when vertical velocity increases, while the corresponding graupel production is quite different for agents used. The main agent nucleation mechanisms are the Brownian coagulation of cloud droplets, inertial impact of cloud droplets and deposition nucleation.With 9 Figures 相似文献
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