On the significance of periodic signals in noise analysis of GPS station coordinates time series   总被引：2，自引：0，他引：2  

Janusz Bogusz  Anna Klos 《GPS Solutions》2016,20(4):655-664

Each of the GPS-derived time series consists of the deterministic (functional) and stochastic part. We propose that the deterministic part includes all periodicities from 1st to 9th harmonics of residual Chandler, tropical and draconitic periods and compare it with commonly used calculations of the annual and semi-annual tropical curve. Then, we address the issues of whether all residual periodicities, as proposed here, need to be taken into consideration when performing noise analysis. We use the position time series from 180 International GNSS Service stations obtained at the Jet Propulsion Laboratory using the GIPSY-OASIS software in a Precise Point Positioning mode. The longest series has 22.1 years of GPS daily solutions. The spectral indices range from –0.12 to –0.92, while the median values of “global” spectral indices are equal to: –0.41 ± 0.15, –0.38 ± 0.12 and –0.33 ± 0.18 for North, East and Up components, respectively. All non-modelled geophysical processes or non-included artificial effects in time series lead to an underestimation of errors of velocities, but also to changes in the velocity values themselves. The proposed assumption of seasonals subtraction caused the Akaike information criterion values to show a decrease in the median value of 30 %, which in fact means that all the seasonals mentioned here must be taken into account when analyzing noises. Finally, we noticed that there are some of the GPS stations that improved their velocity uncertainty even of 56 %.  相似文献   

A microphysically-based approach to modeling emissivity and albedo of the martian seasonal caps     

Janusz Eluszkiewicz  Jean-Luc Moncet  Gary B. Hansen 《Icarus》2005,174(2):524-534

A new model of albedo and emissivity of the martian seasonal caps represented as porous CO₂ slabs containing spherical voids and dust particles is described. In the model, a radiative transfer model is coupled with a microphysical model in order to link changes in albedo and emissivity to changes in porosity caused by ice metamorphism. The coupled model is capable of reproducing temporal changes in the spectra of the caps taken by the Thermal Emission Spectrometer onboard the Mars Global Surveyor and it can be used as the forward model in the retrievals of the caps' physical properties (porosity, dust abundance, void and dust grain size) from the spectra. Preliminary results from such inversion studies are presented.  相似文献   

Morphology and evolution of simulated and optical clusters: a comparative analysis     

Nurur Rahman †‡  Janusz Krywult  Patrick M. Motl  Piotr Flin  Sergei F. Shandarin 《Monthly notices of the Royal Astronomical Society》2006,367(2):838-850

We have made a comparative study of morphological evolution in simulated dark matter (DM) haloes and X-ray brightness distribution, and in optical clusters. Samples of simulated clusters include star formation with supernovae feedback, radiative cooling and simulation in the adiabatic limit at three different redshifts,   z = 0.0, 0.10  and 0.25. The optical sample contains 208 Abell, Corwin & Olowin (ACO) clusters within redshift,   z ≤ 0.25  . Cluster morphology, within 0.5 and 1.0 h ⁻¹ Mpc from cluster centre, is quantified by multiplicity and ellipticity.
We find that the distribution of the DM haloes in the adiabatic simulation appears to be more elongated than the galaxy clusters. Radiative cooling brings halo shapes in excellent agreement with observed clusters; however, cooling along with feedback mechanism makes the haloes more flattened.
Our results indicate relatively stronger structural evolution and more clumpy distributions in observed clusters than in the structure of simulated clusters, and slower increase in simulated cluster shapes compared to those in the observed one.
Within   z ≤ 0.1  , we note an interesting agreement in the shapes of clusters obtained from the cooling simulations and observation. We also note that the different samples of observed clusters differ significantly in morphological evolution with redshift. We highlight a few possibilities responsible for the discrepancy in morphological evolution of simulated and observed clusters.  相似文献   

X-ray Flare Spectra from the DIOGENESS Spectrometer and Its Concept Applied to ChemiX on the Interhelioprobe Spacecraft     

Janusz Sylwester  Zbigniew Kordylewski  Stefan Płocieniak  Marek Siarkowski  Mirosław Kowaliński  Stanisław Nowak  Witold Trzebiński  Marek Śtęślicki  Barbara Sylwester  Eugeniusz Stańczyk  Ryszard Zawerbny  Żaneta Szaforz  Kenneth J. H. Phillips  František Fárník  Anatolyi Stepanov 《Solar physics》2015,290(12):3683-3697

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The Main Ostrava Whetstone: composition, sedimentary processes, palaeogeography and geochronology of a major Mississippian volcaniclastic unit of the Upper Silesian Basin (Poland and Czech Republic)     

Jakub Jirásek  Lada Hýlová  Martin Sivek  Janusz Jureczka  Karel Martínek  Ivana Sýkorová  Mark Schmitz 《International Journal of Earth Sciences》2013,102(4):989-1006

The Main Ostrava Whetstone (MOW) is an important lithostratigraphic horizon of the Late Carboniferous sedimentary fill of the late Palaeozoic foreland Upper Silesian Basin. It is the largest and best-identified volcanogenic horizon in the basin, reaching thicknesses of 15.3 m and occupying an area of ca 2,973 km² and a volume after lithification of 9.24 km³. It consists of volcanic materials transported to the basin probably by an aeolian process. Just after sedimentation, these materials were redeposited a short distance away in a shallow water environment. Granularity corresponds to a range from argillaceous siltstones to fine-grained sandstones. The components are dominated by glass shards replaced by clay minerals (mixed illite–smectite structures) in addition to quartz of volcanogenic and terrigenous origins. Sanidine and a plagioclase close to albite are also present. The sedimentary structures, micro-structures and composition of the MOW indicate variable and dynamic hydrodynamic conditions. The MOW represents a series of flooding events, which could be connected with unusual rainfall. Such major flooding events were most likely induced by volcanic eruptions. The available drill-core log data were used to construct a digital model of the whetstone, which showed an east–west zonality in the thicknesses, with the majority being synsedimentary. CA-TIMS U–Pb dating the volcanogenic zircons yields an age of 327.35 ± 0.15 Ma. The source location of the volcanogenic material is not clear; however, it is presumed to have been located in the west of the Upper Silesian Basin.  相似文献   

GPS-derived height changes in diurnal and sub-diurnal timescales   总被引：1，自引：0，他引：1  

Janusz Bogusz  Mariusz Figurski 《Acta Geophysica》2012,60(2):295-317

This paper describes the research concerning precise short-time GPS solutions conducted in the Centre of Applied Geomatics, Military University of Technology, Warsaw, Poland. The data from ASG-EUPOS (Polish Active Geodetic Network) was processed using Bernese 5.0 software and EPN (EUREF Permanent Network) standards and models. In this study, the adapted 3-hour observation window is shifted every hour for obtaining hourly geocentric coordinates in ITRF2005 reference frame. The adjusted network consisted of over 130 stations from Poland and the neighbouring countries, the period covered observations collected from June 2008 through June 2010. These two years of observations allowed for examining short-period oscillations which were found to be closely related to the tidal (dynamic) frequencies. The analysis of the residua from the IERS2003 tidal model was performed using the least squares method with the Eterna software. It confirmed the existence of significant (several millimetres) oscillations in the frequencies corresponding to S1, K1 and K2. The paper describes the idea of data processing and analysis, presents the results of vertical (the Up component) oscillations in main tidal frequency bands, and also includes discussion of possible explanation of the existence of short-period oscillations in the GPS precise solutions and the possibility of propagation of short-period oscillations into long-period spurious changes in the daily (standard) GPS solutions.  相似文献   

Scenarios of the spread of a waste heat discharge in a river — Vistula River case study     

Monika B. Kalinowska  Paweł M. Rowiński  Janusz Kubrak  Dorota Mirosław-Świątek 《Acta Geophysica》2012,60(1):214-231

The problem of two-dimensional mathematical modelling of heated cooling water discharges into running waters is considered in the paper. Two models — one for the evaluation of 2D turbulent velocity field and the other, developed by authors of the study, for 2D heat transport in open-channels — were used in the calculations. Relevant scenarios of the spread of heated water discharged from a designed gas-stem power plant to be constructed at the Vistula River were presented. Environmentally most friendly variant of the discharge of the thermal pollution was selected from among four various variants.  相似文献   

Fast direct GPS P-Code acquisition   总被引：5，自引：0，他引：5  

Jing?PangEmail author  Frank?Van?Graas  Janusz?Starzyk  Zhen?Zhu 《GPS Solutions》2003,7(3):168-175

GPS P-Code has a higher chipping rate, better accuracy, and anti-jamming property than C/A code. Traditionally, GPS P-Code acquisition depends on handover from C/A code. This potentially needs long acquisition time. Moreover, when C/A code is not available, it is no longer possible to acquire GPS P-Code through handover from C/A code. The purpose of this paper is to describe a new overlap average method to facilitate hardware design of fast direct P-Code acquisition. It allows the rapid code phase search to acquire GPS P-Code signals, and also decreases the hardware resource requirement. The small size FFT in the proposed methods is very promising for fast FPGA hardware system design using FFT cores. The simulation results and theoretical analysis are included demonstrating the overall performance of the proposed method.

Jing PangEmail: Phone: +1-916-2784549Fax: +1-916-2787215

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Foreword to the Special Issue of the Symposia on Assessment and Mitigation of Collateral Seismic Hazards     

Janusz Wasowski  Vincenzo Del Gaudio  David K. Keefer 《Surveys in Geophysics》2002,23(6):471-472

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The influence of late Quaternary stagnations on clay sedimentation in the eastern Mediterranean sea     

Dr. Janusz Dominik  Dr. Peter Stoffers 《International Journal of Earth Sciences》1979,68(1):302-317

Late Quaternary sapropels of the eastern Mediterranean differ from normal sediments in their clay mineral composition. Clay minerals in the sapropels studied here are only slightly affected, or are not affected at all by diagenetic alteration. This permits the observation of primary differences. During stagnation periods, the contribution of remote or accessory sources was reduced or even absent. Different circulation patterns and, particularly, a general decline in deeper water currents activity might be held responsible for the observed differences in the clay mineral composition of sapropels and normal sediments.

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Zusammenfassung Die quartären Sapropele des östlichen Mittelmeeres unterscheiden sich von den normal marinen Sedimenten in ihrer Tonmineralzusammensetzung. Die hier untersuchten Tone der Sapropele zeigen nur geringe oder gar keine diagenetischen Veränderungen. Diese Tatsache erlaubt, Rückschlüsse auf primäre Unterschiede zu ziehen. Während der Stagnationsperioden war die Zufuhr von Tonen aus entfernten oder weniger wichtigen Liefergebieten stark vermindert. Unterschiedliche Zirkulation, besonders eine geringere Aktivität der Tiefenströmungen, scheinen die Ursache für die beobachteten Unterschiede in der Tonmineralzusammensetzung zwischen Sapropel- und normal-marinen Sedimenten

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Résumé Les sapropels quaternaires de la Méditerranée orientale se distinguent des vases communes par la composition des minéraux argileux. Les argiles des sapropels examinés sont peu affectés par l'altération diagénétique, ce qui permet l'observation de différences primaires.On a conclu, que pendant les périodes de stagnation, la contribution des argiles provenant des sources éloignées ou secondaires, a été réduite ou même interrompue. Différentes conditions de circulation et, avant tout, la réduction d'activité des courants profonds, sont probablement responsables des différences observées dans la composition des minéraux argilezx des sapropels et des vases communes.

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