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排序方式: 共有659条查询结果,搜索用时 15 毫秒
651.
652.
Sajad Zareie Kazem Rangzan Hassan Khosravi Vladimir Modestovich Sherbakov 《Arabian Journal of Geosciences》2018,11(14):391
Remote sensing data can be used as the basis for meteorological data. Due to the limitations of meteorological stations on the Earth, derivation of land surface temperature is one of the most important aspects of the remote sensing application in climatology studies. In the present study, Landsat-8 thermal infrared sensor data of the scene located over Khuzestan province with row/path of 165/38 were used to derive land surface temperature (LST). Normalized difference vegetation index (NDVI), fraction of vegetation cover, satellite brightness temperature, and land surface emissivity were calculated as the vital criteria to derive LSTs using the split window algorithms. LST determination was performed by nine different split window algorithms. Eventually, LST products were evaluated using ground-based measurements at the meteorological stations of the study area. The results showed that algorithm of Coll and Casselles had a highest accuracy with RMSE 1.97 °C, and Vidal’s method presented the lowest accuracy to derive LST with RMSE 4.11 °C. According to the results, regions with high density of vegetation and water resources have lowest diurnal temperature and regions with bare soils and low density of vegetation have a highest diurnal temperature. Results of the study indicated that LST algorithm accuracy is an important factor in the environmental and climate change studies. 相似文献
653.
Stanislav S. Kutuzov Vladimir N. Mikhalenko Alexi M. Grachev Patrick Ginot Ivan I. Lavrentiev Anna V. Kozachek Victoria V. Krupskaya Alexey A. Ekaykin Levan G. Tielidze Pavel A. Toropov 《Environmental Earth Sciences》2016,75(23):1488
First-ever ice core drilling at Mt. Kazbek (Caucasus Mountains) took place in the summer of 2014. A shallow ice core (18 m) was extracted from a plateau at ~4500 m a.s.l. in the vicinity of the Mt. Kazbek summit (5033 m a.s.l.). A detailed radar survey showed that the maximum ice thickness at this location is ~250 m. Borehole temperature of ?7 °C was measured at 10 m depth. The ice core was analyzed for oxygen and deuterium isotopes and dust concentration. From the observed seasonal cycle, it was determined that the ice core covers the time interval of 2009–2014, with a mean annual snow accumulation rate of 1800 mm w. eq. Multiple melt layers have been detected. δ18O values vary from ?25 to ?5‰. The dust content was determined using a particle sizing and counting analyzer. The dust layers were investigated using scanning electron microscopy and X-ray diffraction analysis. Dust can be separated into two categories by its origin: local and distant. Samples reflecting predominantly local origin consisted mainly of magmatic rocks, while clay minerals were a characteristic of dust carried over large distances, from the deserts of the Middle East and Sahara. The calculated average dust flux over three years at Kazbek was of 1.3 mg/cm2 a?1. Neither δ18O nor dust records appear to have been affected by summer melting. Overall, the conditions on Kazbek plateau and the available data suggest that the area offers good prospects of future deep drilling in order to obtain a unique environmental record. 相似文献
654.
655.
Vladimir A. Krasnopolsky 《Planetary and Space Science》2011,59(10):952-964
This paper deals with two common problems and then considers major aspects of chemistry in the atmospheres of Mars and Venus. (1) The atmospheres of the terrestrial planets have similar origins but different evolutionary pathways because of the different masses and distances to the Sun. Venus lost its water by hydrodynamic escape, Earth lost CO2 that formed carbonates and is strongly affected by life, Mars lost water in the reaction with iron and then most of the atmosphere by the intense meteorite impacts. (2) In spite of the higher solar radiation on Venus, its thermospheric temperatures are similar to those on Mars because of the greater gravity acceleration and the higher production of O by photolysis of CO2. O stimulates cooling by the emission at 15 μm in the collisions with CO2. (3) There is a great progress in the observations of photochemical tracers and minor constituents on Mars in the current decade. This progress is supported by progress in photochemical modeling, especially by photochemical GCMs. Main results in these areas are briefly discussed. The problem of methane presents the controversial aspects of its variations and origin. The reported variations of methane cannot be explained by the existing data on gas-phase and heterogeneous chemistry. The lack of current volcanism, SO2, and warm spots on Mars favor the biological origin of methane. (4) Venus’ chemistry is rich and covers a wide range of temperatures and pressures and many species. Photochemical models for the middle atmosphere (58-112 km), for the nighttime atmosphere and night airglow at 80-130 km, and the kinetic model for the lower atmosphere are briefly discussed. 相似文献
656.
Finding relative satellite orbits that guarantee long-term bounded relative motion is important for cluster flight, wherein
a group of satellites remain within bounded distances while applying very few formationkeeping maneuvers. However, most existing
astrodynamical approaches utilize mean orbital elements for detecting bounded relative orbits, and therefore cannot guarantee
long-term boundedness under realistic gravitational models. The main purpose of the present paper is to develop analytical
methods for designing long-term bounded relative orbits under high-order gravitational perturbations. The key underlying observation
is that in the presence of arbitrarily high-order even zonal harmonics perturbations, the dynamics are superintegrable for
equatorial orbits. When only J
2 is considered, the current paper offers a closed-form solution for the relative motion in the equatorial plane using elliptic
integrals. Moreover, necessary and sufficient periodicity conditions for the relative motion are determined. The proposed
methodology for the J
2-perturbed relative motion is then extended to non-equatorial orbits and to the case of any high-order even zonal harmonics
(J
2n
, n ≥ 1). Numerical simulations show how the suggested methodology can be implemented for designing bounded relative quasiperiodic
orbits in the presence of the complete zonal part of the gravitational potential. 相似文献
657.
On the relation between steep monoclinal flexure zones and steep hydraulic gradients 总被引:1,自引:0,他引:1
Steep hydraulic gradients are found in association with steep monoclinal flexures. However, the physics of the reduction of the hydraulic conductivity, which is responsible for the steep gradients, has seldom been studied. We present results of hydrological and mechanical modeling aiming to study the effect of such steep hydraulic gradients demonstrated in the Judea Group Aquifer system, Israel. The hydrological configuration of steep dips and anisotropy between flows parallel and perpendicular to the bedding planes was simulated using the FEFLOW code. It exhibited a situation whereby part of the flow is oblique to the bedding planes and therefore some steepening of the hydraulic gradients occurred due to actual conductivity reduction. However, this reduction is not enough to account for the steeper gradients observed. The effect of a deep-seated reverse fault under the monocline on the permeability distribution within the structure was examined by numerical mechanical simulations. It exhibited a compressional stress distribution in the steep part of the monocline, which, due to shortening and closure of joints and voids, is presumably responsible for a significant pressure-induced permeability reduction. This process by itself in a layered structure, including interlayering of thin marl layers, could be responsible for the steep hydraulic gradients in the steep part of the monocline. 相似文献
658.
<正>Whalfera wiszniewskii sp.nov.is described from the Late Eocene Baltic amber.The genus Whalfera is considered as the only fossil genus confidently assigned to the Rhachlberothinae.Others previously placed in this subfamily belong to Paraberothinae(except perhaps for Oisea).The Late Eocene/present Rhachiberothinae and the Cretaceous Paraberothinae are considered to be the subfamilies of Berothidae. 相似文献
659.
Vladimir Frid Dmitri Doudkinski Gady Liskevich Efim Shafran Arie Averbakh Nikolay Korostishevsky Larisa Prihodko 《Environmental Earth Sciences》2010,60(4):787-798
This paper deals with the integration of electrical resistivity tomography and geochemical methods for studying four different
fire-prone landfills. Landfill gas composition (CH4, H2S, O2, CO, CO2) and subsurface temperature were measured with the constant net 50 × 50 m from the depth 10–60 cm. 28 electrical resistivity
tomography lines were surveyed, while Wenner and Sclumberger electrode arrays were employed for all measurements. At the studied
sites the landfill gas and temperature measurements mapped gas and temperature anomalies over underground fire sources. 2D
electrical resistivity tomography lines, performed over these anomalies, showed these fire sources as high-resistivity zones.
The joint employment of the electrical imaging and geochemical survey seems to be a useful tool in carrying out diagnostic
investigations at fire-prone landfills. 相似文献