Theorie der im Elastischen Halbraum Durch eine Flächenförmige Quelle Erregten Weller (3. Teil)     

Karel Pěč 《Studia Geophysica et Geodaetica》1962,6(2):152-167

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Cartographic Design and Usability of Visual Variables for Linear Features   总被引：1，自引：0，他引：1  

Petr Kubíček  Zdeněk Stachoň  Zbyněk Štěrba  Jiří Apeltauer  Tomáš Urbánek 《The Cartographic journal》2017,54(1):91-102

This article addresses the measurement and assessment of response times and error rates in map-reading tasks relative to various modes of linear feature visualization. In a between-subject design study, participants completed a set of map-reading tasks generated by approaches to a traffic problem. These entailed quick and correct decoding of graphically represented quantitative and qualitative spatial information. The tasks first involved the decoding of one graphic variable, then of two variables simultaneously. While alternative representations of qualitative information included colour hue and symbol shape, the quantitative information was communicated either through symbol size or colour value. In bivariate tasks, quantitative and qualitative graphical elements were combined in a single display. Individual differences were also examined. The concept of cognitive style partially explains the variability in people’s perception and thinking, describing individual preferences in object representation and problem-solving strategies. The data obtained in the experiment suggest that alternative forms of visualization may have different impacts on performance in map-reading tasks: colour hue and size proved more efficient in communicating information than shape and colour value. Apart from this, it was shown that individual facets of cognitive style may affect task performance, depending on the type of visualization employed.  相似文献   

Freezing characteristics of a highway subgrade     

Teltayev Bagdat  Suppes Elena 《寒旱区科学》2017,9(3):325-330

Temperature and moisture variations were experimentally investigated for the subgrade of the Astana-Burabai Highway, located in the northern region of Kazakhstan.Temperature and moisture were measured by means of specially manufactured sensors,including an element for temperature measurement based on the effect of thermal resistance and an element for moisture measurement through diamagnetic permeability.It was determined that the long-term average depth of frost penetration was 237 cm.In the upper part of the subgrade with 1 m of thickness,the average duration of a frozen condition decreases toward the bottom from 131 days to 117 days,with an average rate of 0.133 day/cm.The unfrozen water content decreases with the negative temperature reduction.In the case of high values of initial moisture (12%~22%),the unfrozen water content does not depend on the initial moisture;and it decreases under the power law,with reduction of negative temperature.In the case of the lowest values of moisture (9%~12%),the unfrozen water content depends also on negative temperature;but its values are considerably lower.  相似文献   

Detection Capability of Selected Seismic Stations in Central Europe     

Kristeková  Miriam  Skáčiková  Iveta 《Studia Geophysica et Geodaetica》1997,41(2):149-163

The 50% and 90% P-wave detection thresholds of 3 Austrian, 2 Czech, 5 German, 1 Hungarian and 3 Slovak seismic stations have been determined for four intervals of epicentral distances by a direct method using the maximum-likelihood technique. The USGS-NEIC Earthquake Data Reports covering the period from January 1990 to November 1994 were used as the reference system. The seismic stations Kaperské Hory (KHC, Czech Republic) and Collmberg (CLL, Germany) are the stations with the best detection capabilities for all investigated intervals of epicentral distances.  相似文献   

Nonlinear Evolution of Thermal Structures. Numerical Approach     

María Trevisan  Felipe Cordero  Miguel H. Ibáñez S 《Astrophysics and Space Science》1997,256(1-2):381-386

A numerical algorithm using a two stage, two level difference scheme has been developed to solve the heat transfer equation with nonlinear heat diffusion and bulk energy losses. The algorithm is an extension of the scheme developed by Meek and Norbury (1982). The first stage calculates an intermediate value which is used in a second stage to estimate a new value. The scheme is consistent, second-order convergent in space and almost second order in time. It has been applied to the nonlinear stability and time evolution of thermal structures constituted by optically thin plasmas with solar abundances. The configuration has been assumed to be heated at a rate T^m, cooled at a rate Tⁿ and a thermal conduction coefficient T^k. In particular, the second order analytical approximation considered in previous papers (Ibáñez and Rosenzweig, 1995; Steele and Ibáñez, 1997) has been worked out for arbitrary amplitude of the initial temperature disturbance. Particular cases of interest in Astrophysics are considered.  相似文献   

Radiant ephemeris and radiant area of the Perseid meteoroid stream     

B. A. Lindblad  V. Porubčan 《Earth, Moon, and Planets》1995,68(1-3):409-418

More than 600 double-station photographic recordings of Perseid meteor trails have been obtained at various stations in the period 1937–1985. This large data sample has recently been used to determine the activity profile and mean orbit of the Perseid meteoroid stream (Lindblad and Poruban, 1994). In the present paper the radiant of the Perseid meteoroid stream is studied based on a sample of 592 double-station photographic recordings. The daily motion of the radiant and the change of the size of the radiant area with date is investigated. A daily motion of 1.40° in right ascension and 0.20° in declination is derived. These values are slightly larger than those previously found by other researchers. The contraction of the radiant area at shower maximum previously reported from visual observations is confirmed. In a further study radiant areas derived for the dates of the new and the old Perseid maxima are compared. It is found that the radiant area of the new maximum is smaller than that of the old maximum.  相似文献   

Similarities of and differences between three mountain belts at the border of the pannonian basin due to the behaviour of the mohorovičić discontinuity     

Krešimir Čolić  Svetozar Petrović  Hans Sünkel  Miloslav Burda  Miroslav Bielik  Vincenc Vyskočil 《Studia Geophysica et Geodaetica》1994,38(2):131-139

Summary The Dinarides, the Eastern Alps and the Western Carpathians being situated at the borders of the Pannonian basin, are of very similar origin. Therefore, the results obtained in the investigation of correlations between Earth gravity field parameters (absolute geoid undulations, gravity anomalies), the surface topography and the shape of the Mohorovičić discontinuity, were compared. It was found that these three regions have the same basic characteristics, but also their own specific features. While the similarities follow clearly from these investigations, the found differences might partly be a consequence of non-uniformity and unmatched quality of data sets used for the three regions. A short version of this paper, entitled "Kindredness of three mountain belts at the border of the Pannonian basin — deduced from the behavior of the Mohorovičić discontinuity" was presented at the 7th International Symposium "Geodesy and Physics of the Earth", Potsdam, October 5–10, 1992 and published in the Proceedings. Presently a visiting professor at the Graz University of Technology, Institute for Theoretical Geodesy, Department for Physical Geodesy, Austria. Presently at the Berlin University of Technology, Germany, as an Alexander von Humboldt Foundation Research Fellow.  相似文献   

On the transformation of planetary waves of tropospheric origin into waves in radio wave absorption in the lower ionosphere     

Jan Laštovička  Adolf Ebel  Adriena Ondrášková 《Studia Geophysica et Geodaetica》1994,38(1):71-81

Summary Calculations are carried out of upward propagation of a tropospherically forced 10-day planetary wave into the upper middle atmosphere with the use of the COMMA-R model of the University of Cologne, of its transformation into a wave in electron density by means of the model of the Comenius University, and of its final transformation into a wave in radio wave absorption in the lower ionosphere applying the computer code of the Geophysical Institute. The calculations show that the absorption may be used for investigating the planetary wave activity, particularly of its long-term trends. The possibility of propagation of planetary waves from the winter hemisphere to the summer hemisphere is illustrated, which could contribute to explanation of the occurrence of travelling planetary waves in the mesosphere in summer.Dedicated to the Memory of Professor Karel P  相似文献   

Incompatible magnetic behaviour of fine-grained natural haematite samples prepared in similar ways     

Eduard Petrovský  Mark J. Dekkers  Vladimír Kropáček  Pavel Hejda  Tomáš Zelinka 《Studia Geophysica et Geodaetica》1994,38(1):46-56

Summary The results of a magnetic study of two batches of sized natural haematite fractions (from Kada, Czech Republic) are reported. One of the sample batches was prepared by ultrasonic micro precision sieving in propanon (acetone), the other in ethanol (alcohol). Surprisingly, the magnetic behaviour of the ethanol-sieved fractions was much softer (e.g. H_cr 20 kA/m) as compared with the propanon-sieved fractions (H_cr > 200 kA/m). Thermomagnetic measurements suggest a maghemite portion is present in the material used for the preparation of the ethanol-sieved samples. Possible causes of this puzzling behaviour are discussed. However, no definite conclusion can be drawn on the basis of the data presently available.Presented at 3rd Biennial Meeting on New Trends in Geomagnetism, Smolenice Castle, West Slovakia, June 22–29, 1992.  相似文献   

Solar wind and spin of small interplanetary particles     

Jozef Klačka 《Earth, Moon, and Planets》1994,66(2):213-216

The action of the solar corpuscular radiation on the rotational properties of small interplanetary dust particles is investigated. It is shown that the solar wind increases the angular momentum (spin) of the particle. Analytic solutions are presented for dominant terms in which quantities of the orders (v/u) ⁿ ,n 1, are neglected (v is the orbital velocity of dust particle around the Sun andu is the speed of the solar wind particles).  相似文献