Integral transformations of gradiometric data onto a GRACE type of observable     

Michal Šprlák  Pavel Novák 《Journal of Geodesy》2014,88(4):377-390

Integral transformations of gravitational gradients onto a Gravity Recovery And Climate Experiment (GRACE) type of observable are derived in this article. The gravitational gradients represent components of the gravitational tensor in the local north-oriented frame. The GRACE type of observable corresponds to a difference between two gravitational vectors as projected onto the line of sight between the two GRACE satellites. In total, three integral transformations relating vertical–vertical, vertical–horizontal and horizontal–horizontal gravitational gradients with the GRACE type of observable are provided. Spectral and closed forms of corresponding isotropic kernels are derived for each transformation. Special cases show that the integral transformations are general and relate gravitational gradients to many other quantities of the gravitational field, such as the gravitational vector, and its radial and tangential components. Correctness of the mathematical derivations is validated in a closed-loop simulation using synthetic data.  相似文献   

Assess hydrological responses to a warming climate at the Lysina Critical Zone Observatory in Central Europe     

Wenjuan Zheng  Anna Lamačová  Xuan Yu  Pavel Krám  Jakub Hruška  Pavel Zahradníček  Petr Štěpánek  Aleš Farda 《水文研究》2021,35(9):e14281

Climate warming is having profound effects on the hydrological cycle by increasing atmospheric demand, changing water availability, and snow seasonality. Europe suffered three distinct heat waves in 2019, and 11 of the 12 hottest years ever recorded took place in the past two decades, which will potentially change seasonal streamflow patterns and long-term trends. Central Europe exhibited six dry years in a row since 2014. This study uses data from a well-documented headwater catchment in Central Europe (Lysina) to explore hydrological responses to a warming climate. We applied a lumped parameter hydrologic model Brook90 and a distributed model Penn State Integrated Hydrologic Model (PIHM) to simulate long-term hydrological change under future climate scenarios. Both models performed well on historic streamflow and in agreement with each other according to the catchment water budget. In addition, PIHM was able to simulate lateral groundwater redistribution within the catchment validated by the groundwater table dynamics. The long-term trends in runoff and low flow were captured by PIHM only. We applied different EURO-CORDEX models with two emission scenarios (Representative Concentration Pathways RCP 4.5, 8.5) and found significant impacts on runoff and evapotranspiration (ET) for the period of 2071–2100. Results from both models suggested reduced runoff and increased ET, while the monthly distribution of runoff was different. We used this catchment study to understand the importance of subsurface processes in projection of hydrologic response to a warming climate.  相似文献   

Ccd Photometry of the Neglected Contact Binaries V344 Lac and V1191 Cyg     

Theodor Pribulla  Martin Vaňko  DrahomÍr Chochol  Štefan Parimucha  Daniel Baluďanský 《Astrophysics and Space Science》2005,296(1-4):281-284

New photoelectric and CCD observations of the eclipsing contact binary systems V344 Lac and V1191 Cyg are presented and analyzed. All available times of minimum light were used to study period changes of the systems and determine up-to-date ephemerides. The orbital period of V1191 Cyg is found to be increasing at a very fast rate. The photometric elements were determined using the new light curve, radial-velocity curve and broadening function fitting code ROCHE.  相似文献   

Capture of dust grains in exterior resonances with planets     

Miloš šidlichovský  David Nesvorný 《Earth, Moon, and Planets》1996,72(1-3):175-178

The temporary capture of the dust grains in the exterior resonances with planets is studied in the frames of the planar circular three-body problem with Poynting-Robertson (PR) drag. For the Earth and particles ~ 10 Μm the resonances 4/5, 5/6, 6/7, 7/8 are shown to be most effective. The capture is only temporary (of order 10⁵ years) and the position of resonance may be calculated from semi-analytical model using averaged disturbing function. These semi-analytical results are confirmed by numerical integration. For various planet this picture changes as with increasing planetary mass the more exterior resonances become more important. We showed that for Jupiter (at least in the space between Jupiter and Saturn) the resonance 1/2 plays the dominant role. The capture time is here several myr but again eccentricity is evolving to eccentricity e ₀ ~ 0.48 of libration point for this resonance.  相似文献   

钻井液类型对南极冰层取心钻进工作的影响          下载免费PDF全文

宋佳宇  徐会文  韩丽丽  刘宁  张楠  Pavel Talalay 《探矿工程》2015,42(9):13-17

钻井液的类型与性能对于提高极地冰层取心钻进的效率与保证钻孔稳定性具有重要的影响。在分析铠装电动机械钻具工作原理与钻井液循环方式的基础上,较为详细地分析了升降钻具的速度与钻井液粘度与密度之间的关系;分析了现有钻井液类型和所存在的问题;以二元脂肪酸二醇酯、低分子量饱和脂肪酸酯与甲基硅油的试验测试数据为基础,确定了可用于极地冰层取心钻进的钻井液类型及其性能要求。  相似文献   

Integral formulas for computing a third-order gravitational tensor from volumetric mass density,disturbing gravitational potential,gravity anomaly and gravity disturbance   总被引：1，自引：1，他引：0  

Michal Šprlák  Pavel Novák 《Journal of Geodesy》2015,89(2):141-157

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The Fall of the Košice Meteorite          下载免费PDF全文

Pavel P. Povinec  Juraj Tóth 《Meteoritics & planetary science》2015,50(5):851-852

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The Villalbeto de la Peña meteorite fall: II. Determination of atmospheric trajectory and orbit     

Josep M. TRIGO‐RODRÍGUEZ  Ji&#x;í BOROVIKA  Pavel SPURNÝ  Jos L. ORTIZ  Jos A. DOCOBO  Alberto J. CASTRO‐TIRADO  Jordi LLORCA 《Meteoritics & planetary science》2006,41(4):505-517

Abstract— The L6 ordinary chondrite Villalbeto de la Peña fall occurred on January 4, 2004, at 16: 46: 45 ± 2 s UTC. The related daylight fireball was witnessed by thousands of people from Spain, Portugal, and southern France, and was also photographed and videotaped from different locations of León and Palencia provinces in Spain. From accurate astrometric calibrations of these records, we have determined the atmospheric trajectory of the meteoroid. The initial fireball velocity, calculated from measurements of 86 video frames, was 16.9 ± 0.4 km/s. The slope of the trajectory was 29.0 ± 0.6° to the horizontal, the recorded velocity during the main fragmentation at a height of 27.9 ± 0.4 km was 14.2 ± 0.2 km/s, and the fireball terminal height was 22.2 ± 0.2 km. The heliocentric orbit of the meteoroid resided in the ecliptic plane (i = 0.0 ± 0.2°), having a perihelion distance of 0.860 ± 0.007 AU and a semimajor axis of 2.3 ± 0.2 AU. Therefore, the meteorite progenitor body came from the Main Belt, like all previous determined meteorite orbits. The Villalbeto de la Peña fireball analysis has provided the ninth known orbit of a meteorite in the solar system.  相似文献   

Be Stars in Binaries     

Pavel Koubský 《Astrophysics and Space Science》2005,296(1-4):165-168

A brief review of Be stars in binaries is presented. Attention is paid to systems, where the Be phenomenon is clearly connected to the duplicity, but is not a simple consequence of mass transfer.  相似文献   

Preface     

V. Porubčan  I. P. Williams  V. Vanýsek 《Earth, Moon, and Planets》1995,68(1-3):ix-xi

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