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1.
Summary In order to evaluate the accuracy of measurements repeated by a set of gravimeters the semi-systematic errors
2
and
3
were introduced besides the random error
1
in[1]. It is shown that Eqs.(10) and(11), given in[1], should not be used to determine these errors, but Eqs.(8) and(9). 相似文献
2.
Summary On the basis of long period measurements of ionospheric absorption in five A3 circuits in Central Europe, it is shown that the considerable seasonal variation of the diurnal asymmetry of absorption, found in[1], exhibits practically no year-to-year variability and is well-developed at equivalent frequencies f
eq
1 MHz, while it vanishes at F
eq
2 MHz. The limited data on the diurnal asymmetry of the D-region electron concentration are consistent with the seasonal pattern of the diurnal asymmetry in absorption. A tentative hypothesis of nitric oxide variability as the cause of the seasonal variation of the asymmetry is proposed. 相似文献
3.
Summary Using the data in[1], the scale factor for lengths is derived of the geopotential model R
0
=GM/W
0
(W
0
is the potential on a generalized geoid). The resulting value, R
0
==6 363 672.9 m, which is2 m less than the original value[5], is practically the same as that in[6]. 相似文献
4.
Summary In 1967, a series of observations were carried out at Lomnický tít of the intensity of light of the clear sky. Using the de Bary method[1], the observations were used to determine the function of simple dispersion on turbind particles in the atmosphere and compared with theoretical functions, which hold for Jung's power distribution of the particles according to size[7] and for the logarithmic Gauss distribution of the particles[8]. 相似文献
5.
Summary As regards the concept of complete weight p with which an observed quantity (e.g., the direction of theA–G net) should enter the net adjustment, according to Eq.(1), apart from the fundamental weight p
0
), determined by the number of repetitions, it should also contain the time parameter pt according to Eq.(11), where c>1 is a constant, and t is the number of days of observation, and also the refraction factor pr according to Eqs(17, 18), where q is the structural weight of the direction. The condition for being able to determine pr with the directions is observation by means of the three-directional vertex method[2], because it is not possible to localize lateral refraction by angular methods. The theory of complete weight is in favour of observations with a high fundamental weight p
0
which automatically yield higher values of t, and also of pt. The introduction of the complete weight into the experimental directional net in Fig. 2 caused the mean value of the uneliminated refraction error to decrease from 0.24 to 0.12, the mean square error of the adjusted direction being 0.17. The value of the constant c was investigated and the method of determining the parameter pr was derived also for lengths measured electro-optically. Mention is made of the effect of complete weights on the length adjustment of a net in[6]. 相似文献
6.
Summary The stochastic properties of the vector function, formed by the components and of the deflection of the vertical and by the height of the geoid , are studied by utilizing the mathematical model in[4]. The properties of the error components of the said vector are also studied and a method is described for comparing the results when the vector function was obtained directly by means of astro-geodetic methods and when the vector function was generated by the Vening-Meinesz and Stokes transformation. 相似文献
7.
Summary The model of filtration of a linearly polarized HM-wave in a system of three homogeneous layers, limited by two halfspaces and treated in[1], is generalized. The wave attenuation is considered in all inner layers of the system and the model is applied to the filtration of HM-waves in the lower layers of the magnetosphere, i.e. in the ionosphere. The nature of the changes of the functional dependences is studied, i.e. of the amplitude coupling factor on the frequency under variation of the fundamental parameters, defining the filtering medium. Filtration models are demonstrated and discussed for the periods of maximum and minimum solar activity during daytime and at night. The relation between the properties of filtration and the possibilities of observing geomagnetic pulsations on the Earth's surface is pointed out. 相似文献
8.
Summary Among the various dynamic ray tracing systems described by ervený and Hron[1] is one particular linear system of second order that readily provides identical parameters (in the ray centred coordinate system) to those that fall out of the system by Popov and Peník[3, 4]. Hence the initial conditions of the latter system for sources and interfaces can easily be used to provide those for the linear system of second order. 相似文献
9.
Alexander Roglinov Ludmil Christoskov Reviewer J. Vaněk 《Studia Geophysica et Geodaetica》1977,21(1):11-18
Summary Aki's spectral 2 model[1] is used to estimate the amplitude field at epicentral distances up to 1000 km in the case of an absorption coefficient of seismic waves which varies with distance. Velocity spectra, the periods of the maximum of these spectra and the maximum velocity amplitudes are obtained. The results are compared with[2] and it is shown that the divergence of the amplitude field decreases if a variable absorption coefficient is used. The theoretical results, obtained in this case, approach the results seen in practice. The possibility of determining the limits of epicentral distances, at which the amplitude field may be considered as linear, is given. 相似文献
10.
Summary The integral mean values of gravity on the surface W=W
0
, obtained from satellite observations with the use of harmonic coefficients[3, 7] and from terrestrial gravity measurements[12], are compared. The squares and products of the harmonic coefficients were neglected, with the exception of [J
2
(0)
]
2
, which was taken into account. The Potsdam correction and the geocentric constant are being discussed. The paper ties up with[13–15] and the symbols used are the same. The given problem was treated, e.g., in[2, 4, 6, 8–10]; in the present paper the values of gravity are compared directly. 相似文献
11.
Summary Radii of curvature and their anomalies of a smoothed geoidal surface are computed using Stokes's constants J
n
(k)
, S
n
(k)
of the Earth's body, obtained from satellite orbit dynamics[2]. Different degrees n of smoothing are used (n = 8, 12, 21). The notations are the same as in[4, 5]. 相似文献
12.
Evaluation and application of the ion microprobe in the strontium isotope geochemistry of carbonates
Richard A. Exley 《Earth and Planetary Science Letters》1983,65(2):303-310
A modified AEI-IM20 ion microprobe has been used to measure87Sr/86Sr ratios in carbonates. A suite of carbonates with varying major elements (Ca, Mg, Fe, Mn) was studied at low and high (M/ΔM ? 3000) mass resolution to determine the types and intensities of molecular species isobaric with Sr peaks; Sr data collected at low mass resolution must be corrected for Ca2 and CaMgO species. Rb/Sr ratios are extremely low, and correction for87Rb is not required (< 0.1‰ of87Sr).Usable Sr isotopic data may be obtained from calcite givenSr≥ 400ppm, and for Sr > 5000 ppm a precision of ～ ± 1‰ (± 0.0007) in87Sr/86Sr (2σ mean) can be achieved under optimum conditions. The corrections for Ca2 and CaMgO are smaller than the within-run precision in calcite, but in dolomite the correction for CaMgO is + 1.5%. Mass fractionation corrections to87Sr/86Sr (based on86Sr/88Sr= 0.1194) are typically +8 to +10‰. Good agreement between ion probe and solid source mass spectrometer results was found for calcites of known Sr isotopic composition: ST4a (～ 400ppm Sr), average ion probe87Sr/86Sr= 0.7267 ± 0.0015, solid source87Sr/86Sr= 0.72680 ± 0.00008 [14]; JCG36 (～ 6000ppm Sr), average ion probe87Sr/86Sr= 0.7056 ± 0.0009, solid source87Sr/86Sr= 0.70588 ± 0.00009 [16]; JCG44 (～ 6000ppm Sr), average ion probe87Sr/86Sr= 0.7057 ± 0.0006, solid source87Sr/86Sr= 0.70540 ± 0.00008 [16]. The ability of the ion microprobe to measure87Sr/86Sr for 10-μm spots in calcite was used: (1) to measure variation in87Sr/86Sr of ～ 0.01 on a centimetre scale in a hydrothermally altered basalt from the Isle of Skye, northwestern Scotland; and (2) to determine the Sr isotopic composition of tiny (< 35 μm) calcite grains in a veined mantle lherzolite from Bultfontein, South Africa. Because of calcite's ubiquitous occurrence in many parageneses this technique may offer many opportunities for the measurement of fine scale heterogeneities in87Sr/86Sr. 相似文献
13.
Dubovikov and Canuto (Dubovikov, M.S. and Canuto, V.M., Complete Eulerian-mean tracer equation for coarse resolution OGCMs. Geophys. Astrophys. Fluid Dyn., 2006, 100, 197–214), after averaging the tracer conservation equation in density coordinates and transforming to height coordinates, concluded that present ocean models are missing important terms in their mean tracer equations. Here we point out some errors made by Dubovikov and Canuto (2006) in their isopycnal averaging procedure. We draw on the temporal-residual-mean (TRM) theory and show that when the isopycnal averaging and coordinate transformation are performed correctly, the tracer equations of present ocean circulation models are recovered. We therefore conclude that present ocean circulation models are not neglecting the leading order terms identified by Dubovikov and Canuto (2006). 相似文献
14.
Summary The evolution of the opinions as to the problem of the triaxiality of the Earth in the period prior to satellite geodesy can be seen, e.g., in[1–18]. Recently the opinion has been voiced that triaxiality is a result of the mathematical treatment of data rather than reality[19–21], especially since this is a comparatively small parameter. This opinion is not in contradiction with the results of satellite observations[22–28], but the non-zero values of the harmonic coefficients of the second degree and second order are a reality, they yield a value of the equatorial flattening of about1/90 000, and the representation of the equatorial section by an ellipse is justified even if the harmonics n=3, k=1 and n=3, k=3 have amplitudes only about half as small, and some other parameters might occur with just as much justification besides triaxiality. 相似文献
15.
16.
Résumé On donne les résultats de l'analyse de la dérive des pendules horizontaux de la station Píbram-Bezové Hory au cours des années 1927–1938. Différemment aux résultats publiés déjà antérieurement[2], on a tout d'abord séparé par la méthode des moindres carrés la dérive linéaire et le terme à période de durée d'un an exactement et ce n'est que le reste qu'on a analysé par la méthode de l'analyse spectrale spéciale[4, 6]. On a trouvé dans les deux éléments une période de 222, respectivement 223 jours, non considérée jusqu'alors et ne pouvant pas être interprétée jusqu'à présent du point de vue physique. Les autres résultats sont en bon accord avec ceux reçus à l'origine. On peut conclure de la comparaison des phases des composantes annuelles des pendules horizontaux et du mouvement du pôle[5] que les deux événements sont du même origine. 相似文献
17.
18.
In mean-field dynamo theory, the electromotive force term 〈u′ × B′〉 due to small-scale fields connects the small-scale magnetic field with the large-scale field. This term is usually approximated as the α-effect, assumed to be instantaneous in time and local in space. However, the approximation is valid only when the magnetic Reynolds number Rm is much less than unity, and is inappropriate when Rm ? 1, which is the condition satisfied in the Earth's core or solar convection zone. We introduce a function φ qr as a non-local and non-instantaneous generalization of the usual α-effect and examine its behaviour as a function of Rm in the range 1/64 ≤ Rm ≤ 10 for a kinematic dynamo model. We use the flow of G.O. Roberts 1972 (Phil, Trans. Roy. Soc. London Ser. A, 1972, 271, 411–454), which is steady and has non-zero helicities and two-dimensional periodicity. As a result, we identify three regions in Rm space according to the behaviour of the function φ qr : (i) Rm ? 1/4, where the function φ qr is local and instantaneous and can be approximated by the traditional α and β effects, (ii) 1/4 ? Rm ? 4, where the deviation from the traditional α and β effects increases and non-localness and non-instantaneousness increase, and (iii) Rm ? 4, where boundary layers develop fully and non-localness and non-instantaneousness are prominent. We show that the non-local memory effect for Rm ? 4 strongly affects the dynamo action and explains an observed augmentation of the growth rate in the dispersion relation. The results imply that the non-local memory effect of the electromotive force should be important in the geodynamo or the solar dynamo. 相似文献
19.
R. James Brown 《Pure and Applied Geophysics》1973,105(1):759-769
Summary Relative arrival times at the Uppsala tripartite seismograph array station are used to determinedT/d and ray azimuth for some 200 compressional phases. Corrections, although very small, are applied for station elevations, telephonic transmission delays and array geometry. The computeddT/d and ray azimuths are further corrected to remove the effect of lateral heterogeneity immediately beneath the array station. Errors indT/d and azimuth are considered from a partly theoretical, partly empirical approach. They amount to about 0.18 sec/deg indT/d and 1.6° in azimuth. Standard deviations in epicentral locations are empirically determined to be about 2° due to slowness error and less than 1.5° due to azimutherror; or about 250 km overall. These figures compare favourably with other, more costly, arrays. 相似文献
20.
Dr. K. Burkhart 《Pure and Applied Geophysics》1954,27(1):116-120
Zusammenfassung In der modernen Registriertechnik strebt man immer mehr danach mittels elektrischer Übertragungsanlagen (Verstärker) geophysikalische Vorgänge sofort sichtbar aufzuzeichnen. Bei der Erdmagnetik konnte die photographische Aufzeichnung wegen ihrer Genauigkeit durch keine andere Methode ersetzt werden. Eine elektrische Übertragung auf P. Schreiber ist nur mit Hilfe von Differential-Photozellen möglich. Am obigen Observatorium läuft seit Oktober 1953 eine Anlage für die Deklination und Horizontalintensität. DasH-Variometer (einTöpfer-Instrument) ist temperaturkompensiert; dasD-Variometer wurde am Observatorium hergestellt und besitzt ein Plexiglas-Gehäuse. Die mit besonderen Blenden ausgestatteten Projektoren beleuchten die Variometer, die gleichmäßig ausgeleuchtete Lichtrechtecke auf die Zellen werfen. — Die Skalenwerte betragen inD: 0.70±0.03, inH: 4.2±0.05 Gamma pro pars. Die Anlage erweist sich als sehr praktisch für die Prognose ionosphärischer Störungen.
Summary In modern technique for recordings the directly visible drawing of geophysical processes is more and more used by means of electrical arrangements of transmission (amplifier). The photographic recording in the research of earth-magnetism could not be substituted with another method on account of its exactness. An electrical transmission at point-writers is only possible with differential-photocells. At the Observatory in Fürstenfeldbruck an arrangement for declination and horizontalintensity is now working since October 1953. TheH-variometer (byTöpfer) is compensated for temperature; theD-variometer was constructed at the Observatory and has a case of plexigum. The projecters furnished with special diaphragm lights up the variometers which throw equal clear rectangles of light at the cells. — The scalevalues are inD 0.70±0.03, inH: 4.2±0.05 Gamma per pars. The arrangement is very usefull for prognosis of ionospheric disturbances.相似文献