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11.
Mustafa Basaran Gunay Erpul A. Ugur Ozcan Pieter Bogman Wim M. Cornelis Donald Gabriels 《Environmental Earth Sciences》2010,61(7):1375-1384
There are various types of the windblown sediment traps developed for wind tunnel and field studies. One of the main supports
expected from these traps is in measuring surface dust concentrations to appropriately derive flux equations. The measurement
performance and accuracy of a trap is very important and depends strictly upon the physical characteristics and the behaviors
of dust grains with air flows. This paper presents the measurement results of static pressure distribution (SPD) of wind flow
around Vaseline-coated slide (VCS) catchers with an aim of finding out whether or not particle trapping efficiency (η) of
the VCS is related to the SPD. The SPD was evaluated by a wind reduction coefficient (R
c) in a series of wind tunnel experiments with different VCS settings which have different attachment configurations on a pole.
Three VCS configurations were considered: a configuration on a circular plastic pole (CPP) and two configurations on wooden
square poles (WSP1 and WSP2, respectively). Thus, the primary contribution of this work was to experimentally analyze the effect of the different attachment
configurations on the SPD, and the secondary objective was to determine the effect of the SPD on the η. It was shown that
spatial correlation and spatial pattern of the R
c were different in the surrounding area of each configuration, and ANOVA and DUNCAN tests indicated that η(s) of WSP1, WSP2, and CPP were different at the significant level of P ≤ 0.05 with the mean of 0.94 ± 0.09, 0.63 ± 0.14, and 1.13 ± 0.07, respectively. Additionally, the amount of PM20, PM40, PM60, PM80, and PM100 trapped by the configurations of WSP1, WSP2, and CPP considerably varied depending upon the particular aerodynamic circumstances associated with every configuration. 相似文献
12.
Lapperre Rimbaud E. Bense Victor F. Kasse Cornelis van Balen Ronald T. 《Hydrogeology Journal》2022,30(4):1233-1257
Hydrogeology Journal - Faults in the Roer Valley Rift System (Netherlands, Belgium, and Germany) act as barriers to lateral groundwater flow in unconsolidated sedimentary aquifers. This causes a... 相似文献
13.
Cornelis De Jager 《Astrophysics and Space Science》1974,31(2):417-425
The increasing number of interesting variable X-ray sources asks for an instrument for continuously monitoring the brightness of the most important X-ray sources over the whole sky. We describe a system consisting of a set of identical large position-sensitive detectors, mounted on the sides of a polyhedral satellite. Each counter is illuminated through a large diaphragm, with binary shadow characteristics. By holographic methods the X-ray image of the observed part of the sky could be derived from the illumination of each detector by multiplex analysing methods. The satellite should have fairly coarse (half a degree accuracy) three-axial stabilization, and an on-board computersteered data accumulation system. A relation is derived between the number of transparent holes in the diaphragm, the total count rate, and the flux of the faintest observable source. It appears that for a diaphragm with a few hundred transparent holes (detector geometrical area ≈103 cm2) an integration time of approximately 6 min is needed in order that sources with a count rate of 0.01 cm?2 s?1 should still be observable with a confidence limit of 99%. 相似文献
14.
Cornelis De Jager 《Solar physics》1987,114(2):387-388
15.
Cornelis Zwaan 《Solar physics》1974,37(1):99-111
The sunspot models published so far do not reproduce the observed run of the umbral continuum intensities over the entire spectral range 0.5 < < 4 m. Moreover, in several previous models is the temperature gradient smaller than both the adiabatic and the radiative equilibrium gradient.Agreement between intensities computed from acceptable models and measured intensities can be obtained by introducing an additional opacity for 0.8 m, which is probably caused by the crowding of atomic and molecular lines. We present a new umbral model atmosphere with a wavelength dependent opacity enhancement factor which explains the continuum intensities and also reproduces plausible center-to-limb variations and line profiles. This model is in radiative equilibrium down to 0.5 = 1.5, with an effective temperature of 4000 ± 100K. For the deeper superadiabatic layers a small but probably significant departure from radiative equilibrium is indicated by the intensities in the range 1.5 < < 2.4 m.The uncertainties in the present model and the effect of the additional opacity on line profiles are briefly discussed. 相似文献
16.
The contributions of any arbitrary photospheric velocity field to (macroturbulent) line displacement, and to (microturbulent) line broadening can be expressed by the macro- and micro-turbulent filters f
M
(k) and f
t(k), where k is the wavenumber of the energy spectrum in which the line-of-sight component of the velocity field can be decomposed. As a correction to a previous computation of f
M
and f
t
we give in this Note improved values for the filter functions for weak lines in LTE. An example of the way to use the filter functions is given. 相似文献
17.
Cornelis De Jager 《Solar physics》1981,74(1):11-17
The Sun is a variable star in many respects: there are secular varitions related to the general solar evolution, and - as discovered in recent years - there are many short period variations of which the 5 min and 160 min pulsations are the most important ones. Magnetic fields in the outer convective mantle play a dominant role in the 22-years cycle. The origin of solar magnetic variability is a key problem in astrophysics. The relation between solar variability and changes in the Earth's climate is a crucial element in climatology.Introductory talk to the 14th ESLAB Symposium: Physics of Solar Variations, 16–19 September, 1980, Scheveningen, The Netherlands. 相似文献
18.
19.
20.
Günay Erpul Donald Gabriels Melis Özge Pınar Çağlar Sagun Wim Cornelis 《地球表面变化过程与地形》2021,46(14):2870-2883
The effects of wind-driven rain (WDR) on sand detachment were studied under various raindrop obliquities. Results suggested a significant reduction in compressive stress on sand surfaces for a two-dimensional experimental set-up in a wind tunnel. During experiments, sand particles in splash cups were exposed to both wind-free rain (WFR) and WDR driven by horizontal winds of 6.4, 8.9 and 12.8 m s−1 and rainfall intensities of 50, 60, 75 and 90-mm h−1 to assess the sand detachment rate (D, in g m−2 s−1). The effects of sand moisture state (dry and wet) on the detachment of different-sized particles (0.20–0.50 and 0.50–2.00 mm, respectively) were also tested. Factorial analysis of variance showed that shear and compressive stress components evaluated by horizontal and vertical kinetic energy flux terms (KEx and KEy, respectively, in J m−2 s−1) along with their vector sum (KEr, in J m−2 s−1) explained the variation in D. Neither sand size nor sand moisture was statistically significant alone although binary interactions of KEr, KEx and KEy with the sand size and three-way interaction of KEx, sand size and moisture were statistically significant. These results can be explained by size-dependent variation in sand compressibility and surface friction related to the total stress field developed by a given partition of shear and compressive stresses of wind-driven oblique raindrops (KEx/KEy). Further analysis of the variation of the unit sand detachment rate (Du = D/KEr = g J−1) with rain inclination (α, in degrees) better revealed the effect of WDR obliquity on Du that further changed with sand size class and moisture state. Finally, the difference in the resulting stress field differentiable by the oblique raindrop trajectories of the experiment over sand surface significantly affected the non-cohesive particle detachment rates, to some extent interacted with size-dependent compressibility and interface shear strength of sand grains. 相似文献