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1.
Summary On the basis of investigating 10 storms (1965–1967) good correlation was found between the density of the solar wind energy (2=1/2mNv2) and the intensity of the main phase of the geomagnetic storms, expressed in terms of the maximum decrease of the horizontal intensity (B=H/cos). The relation between 2, or Nv2, and B could then be used to determine the quantities and 0 ( is the factor expressing the increase in energy density in the magnetosphere, 0 is the energy density of the particles in a quiet magnetosphere). A comparison with the directly observed distribution of the energy density of the particles in the magnetosphere indicates that the computed value of 0 seems to be realistic. The magnitude of the factor will have to be checked again.  相似文献   

2.
Summary Dispersion in Rayleigh waves is discussed for semi-infinite media with = 1(1 ± cos s z) and = 1(1 ± cosh s z), being the rigidity of the medium. A few workers tried with the above Fourier type of model but failed to find the dispersive nature. Because they neglected s due to the complexity of the calculation they arrived at a non dispersive frequency equation. This difficulty is removed in this paper and a dispersive frequency equation is obtained which shows both direct and inverse dispersion. The second model leads to non-convergent solution forz but shows many interesting results which are also discussed.  相似文献   

3.
Piest  Jürgen 《Ocean Dynamics》1963,16(1):9-14
Zusammenfassung Als Zusammenhang zwischen der kennzeichnenden Wellenperiode und der durchschnittlichen Periode im Seegang wird die Formel angesetzt. Mit Hilfe empirischer Unterlagen wird nachgewiesen, daßc eine Funktion des von D. E. Cartwright und M. S. Longuet-Higgins [1956] eingeführten Spektralparameters ist. Es wird eine vorläufige quantitative Beziehung zwischenc und abgeleitet.
Empirical investigations of the relation between the mean and the significant wave period in the sea
Summary It is supposed that the formula represents the relation between the significant wave period and the mean period in the sea. With the aid of empirical data it is demonstrated thatc is a function of the spectral parameter introduced by D. E. Cartwright and M. S. Longuet-Higgins [1956]. A preliminary quantitative relation betweenc and is derived.
Etudes empiriques de la relation entre la période moyenne et la période significative des vagues dans la houle
Résumé On suppose que la formule représente la relation entre la période significative des vagues et la période moyenne dans la houle. A l'aide des données empiriques on montre quec est une fonction du paramètre spectral , introduit par D. E. Cartwright et M. S. Longuet-Higgins [1956]. Une relation quantitative préliminaire entrec et est dérivée.
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4.
Summary The components of the tidal torques along the axes of the inertia ellipsoid of a perfectly elastic Earth have been derived quite independently of the density distribution of masses within the Earth. It has been demonstrated that not only the sectorial, but also the tesseral terms in the tidal forming potential are responsible for the tidal deceleration of the Earth's rotation.
am ¶rt; mau ma nuu u m u a um unu¶rt;a uuu u¶rt;a n u, auu m ¶rt;a an¶rt;uu nmm a. aa, m nuu a¶rt;u au u a m muau, u mau nuuu au nuua nmua.
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5.
Summary Based on the relation between the relative sunspot number R, the number of sunspot groups f 0 generated per unit time on the Sun as a whole and their average lifetime T 0 , and on the extrapolation of time behaviour of f 0 and T 0 , it is proved that abnormally high solar activity may be expected in the first half of the 21st century. At this time, the maximum annual relative sunspot numbers RM of the 11-year cycles should reach values of about 300 units. This abnormally high solar activity in the next century can be understood as the antipole of the Maunderean minimum. This forecast is used to discuss some of the possible consequences of this abnormally high solar activity for the processes on the Earth: changes of climate (heat waves and draughts in Central Europe), in the higher layers of the Earth's atmosphere (anomalous propagation of radio waves, increased effect of the density of the upper atmosphere on the orbits of man-made satellites), in seismicity (increased seismic activity in Europe and Southeast Asia), for technical devices (induced electric currents), in the biosphere. etc.
a mu ¶rt; uau a R nm, unn nm f 0 uu ¶rt;uu u a ë u u ¶rt; n¶rt;ummu uu 0 , u a manuu ¶rt;a f 0 u 0 , naa, m n nu ¶rt; 21 a u¶rt;am uum amum. aua¶rt;u ua a R m¶rt; 11-mu ua m u ¶rt;muam au 300 ¶rt;uu. m uum amum ¶rt; nuam a amun¶rt; a¶rt; uua. a m na ¶rt;am m n¶rt;mu m uum amumu a n nmau a : a uu uama (aa u a n¶rt;a ¶rt; n), a u u am u (aa anmau a¶rt;u, uu n nmmu u am a ¶rt;uu um m), a um (na ua amum n u -m uu), a muu mma (u¶rt;ua muu mu), a u u ma ¶rt;a.
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6.
Summary The position of the Sun with respect to the gravity centre of the Solar System for the beginning of every year of a 3100 — year time series was determined and the harmonic analysis of the parameters of the Sun's motion about the gravity centre was carried out.
unu u u ¶rt; ¶rt;¶rt; u ¶rt; ¶rt;u 3100 u c¶rt;uu u n ¶rt;uu u.
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7.
Summary The method of numerical modelling of ionospheric filtration of the Fourier components of a signal from the frequency range of Pc1 micropulsations is employed in the spectral analysis (frequency f, angle of incidence ) of the relative characteristic of the amplitude and energy reflectivity of the ionospheric layer with respect to ordinary Alfvén modes incident in the meridional plane. The results are presented for four different models characterizing the midlatitude day- and night-time ionosphere under low and high solar activity. The results indicate the specificity of filtration of ordinary Alfvén waves. It is proved that the lower region of the modelled ionosphere, as part of the midlatitude ionospheric wave guide (in particular the F2 layer), behaves like an Alfvén resonator in the given spectral range.
m¶rt; u ¶rt;uau u umauu -mau uaa u amm ¶rt;uanaa unau 1 n¶rtum nma aau (amma f, a¶rt;u ) mum anum¶rt; u mu maamu u ¶rt; ¶rt; a, a¶rt;au a u u¶rt;ua nmu. mam n¶rt;aam ¶rt; m a ¶rt; ¶rt;um m ¶rt; u u nu u u nu amumu. aam nuum umauu a. naa, m ua am ¶rt;ua u (a am F2-u ¶rt;um ¶rt;a) ¶rt;m nma ¶rt;uana a am a.
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8.
Summary The geopotential scale factor R 0 =GM/W 0 has been determined on the basis of satellite altimetry as R 0=(6 363 672·5±0·3) m and/or the geopotential value on the geoid W 0 =(62 636 256·5±3) m 2 s –2 . It has been stated that R 0 and/or W 0 is independent of the tidal distortion of surface W=W 0 due to the zero frequency tide.
¶rt;a nmu amumuu u ama amnmuaa R 0 =GM/W 0 =(6 363 672,5±0,3) m u/uu aunmuaa a nmuu¶rt;a W 0 =(62 636 256,5±3) m2 s–2. m, m R 0 u/uu W 0 auum m nm amu a a nuu ¶rt;au nmu W=W 0 .
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9.
Summary Radiation absorption by water vapour plays an important role in the physics of the atmosphere. The calculation of the absorbed radiation energy by water vapour requires the amount of precipitable water in the atmosphere to be known. Actinometric and aerological measurements were used to establish the relation between vapour pressure and absorbed solar radiation.
u a¶rt;uauu ¶rt; nam uam a amu uuu am. uu n a¶rt;uauu ¶rt; na a¶rt; am m a¶rt; ¶rt; am. u¶rt; mu ¶rt; ¶rt;au ¶rt; naa u n a¶rt;uau a amu muu u auu uu.
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10.
Gomes  E.  Zheng  X.  Pšenčík  I.  Horne  S.  Leaney  S. 《Studia Geophysica et Geodaetica》2004,48(1):215-231
We apply the inversion scheme of Zheng and Peník (2002) to the walkaway VSP data of Horne and Leaney (2000) collected in the Java Sea region. The goal is a local determination of parameters of the medium surrounding the borehole receiver array. The inversion scheme is based on linearized equations expressing qP-wave slowness and polarization vectors in terms of weak anisotropy (WA) parameters. It thus represents an alternative approach to Horne and Leaney (2000), who based their procedure on inversion of the Christoffel equation using a global optimization method. The presented inversion scheme is independent of structural complexities in the overburden and of the orientation of the borehole. The inverson formula is local, and has therefore potential to separate effects of anisotropy from effects of inhomogeneity. The data used are components of the slowness vector along the receiver array and polarization vectors. The inversion is performed without any assumptions concerning the remaining components of the slowness vector. The inversion is made (a) assuming arbitrary anisotropy, i.e., without any assumptions about symmetry of the medium, (b) assuming transverse isotropy with a vertical axis of symmetry and (c) assuming isotropy of the medium. Inverted are the raw data as well as data, in which weighting is used to reduce the effect of outliers. It is found that the WA parameters z, 15 and 35 are considerably more stable than the parameters x and x. The latter two parameters are also found to be strongly correlated. Weaker correlation is also found between the mentioned two parameters and z. The results of inversion show clearly that the studied medium is not isotropic. They also seem to indicate that the studied medium does not possess the VTI symmetry.  相似文献   

11.
Summary Thirty wave records taken by the O. W. S. Weather Explorer in the Atlantic Ocean, studied in a previous paper (J. Darbyshire [1959a]), are taken and the statistical distribution of wave heights and wave periods found. The mean height for each observed period is also found.The three methods described by D. E. Cartwright and M. S. Longuet-Higgins [1956], are used to evaluate which indicates the departure of the height distribution from a Rayleigh distribution. Agreement between the three results is good enough to verify the accuracy of the theoretical distribution. The relation giving the variation of withT f , the period of maximum energy on the frequency spectrum, derived in the previous paper (J. Darbyshire [1959b]) is verified.The distribution of wave heights on thirty wave records taken by the Morecambe Bay Lightship is also worked out. In this case there is a marked lack of symmetry between the distribution of the heights of crests and troughs, measured from mean sea level. Estimates of by the three methods do not agree so well in this case although the values derived from the frequency spectra vary withT f as would be expected from the relationship derived by J. Darbyshire [1959b].
Die relative Frequenz von Wellenhöhen und -perioden im Atlantischen Ozean und in der Irischen See
Zusammenfassung Dreißig vom O. W. S. 'Weather Explorer im Atlantischen Ozean aufgenommene und in einer früheren Abhandlung (J. Darbyshire [1959a]) untersuchte Seegangs-registrierungen werden zur Ermittlung der statistischen Verteilung von Wellenhöhen und Wellenperioden benutzt. Die mittlere Höhe jeder beobachteten Periode wird ebenfalls bestimmt.Die drei von D. E. Cartwright und M. S. Longuet-Higgins [1956] entwickelten Methoden werden dazu verwendet, den Wert von, das die Abweichung der Höhenverteilung von der Rayleighschen Verteilung ausdrückt, zu berechnen. Die Übereinstimmung zwischen den drei Ergebnissen ist groß genug, um die Genauigkeit der auf theoretischem Wege gewonnenen Verteilung zu bestätigen. Es wird die Richtigkeit der Beziehung bestätigt, die aus der Veränderlichkeit von in Abhängigkeit vonT f resultiert, der Periode der größten Energie im Frequenzspektrum, die bereits in einer früheren Arbeit von J. Darbyshire [1959b] abgeleitet wurde.Die Verteilung der Wellenhöhen für die dreißig Seegangsregistrierungen wird ebenfalls ausgewertet. Hierbei machte sich ein beträchtlicher Mangel an Symmetrie zwischen der Verteilung der Höhen und Tiefen von Wellenkämmen und Wellentälern bemerkbar, die unter Zugrundelegung des mittleren Wasserstandes gemessen wurden. Berechnungen von mit Hilfe dieser drei Methoden zeigen in diesem Falle keine allzu gute Übereinstimmung, obgleich die vom Frequenzspektrum abgeleiteten Werte in Abhängigkeit vonT f variieren, wie dies nach der von J. Darbyshire [1959b] abgeleiteten Beziehung zu erwarten war.
Les fréquences relatives des hauteurs et des périodes des vagues en océan Atlantique et en mer d'Irlande
Résumé Trente enregistrements des vagues obtenus par le navire météorologique «Weather Explorer» en océan Atlantique et analysés antérieurement par J. Darbyshire [1959a] sont utilisés pour. déterminer la distribution des hauteurs et des périodes des vagues. La hauteur moyenne de chaque période observée est également déterminée.Les trois méthodes décrites par D. E. Cartwright et M. S. Longuet-Higgins [1956] servent à estimer la grandeur qui indique la différence entre la distribution des hauteurs et la distribution d'après Rayleigh. L'accord entre les trois résultats est assez satisfaisant pour vérifier l'exactitude de la distribution estimée d'une manière théorique. La relation donnant la variation en fonction deT f , qui sur le spectre de fréquences représente la période de l'énergie maximum, dérivée antérieurement par J. Darbyshire [1959b], se vérifie.Les trente enregistrements, provenant du bateau feu stationné dans la baie de Morecambe, sont analysés pour en obtenir la distribution des hauteurs de vagues. Ces analyses montrent que dans ce cas il existe un défaut remarquable de la Symmetrie entre la distribution des hauteurs des crêtes et celle des profondeurs des creux, mesurées à partir du niveau moyen de la mer. Les estimations de effectuées au moyen de trois méthodes citées ci-dessus, ne s'accordent pas trop bien dans ce cas, bien que les valeurs, dérivées des spectres de fréquences, varient avecT f à mesure que l'on pourrait s'y attendre d'après la relation dérivée par J. Darbyshire [1959b].
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12.
Summary In this paper an attempt is made to define the time variations of theD-region main aeronomical parameters under non-equilibrium conditions by using experimental data by the A3 method, phase-height method and satellite data for the short-wave X-radiation. The SID effect of day-time and time variations of 21 August 1969 electron concentrationN(t) and recombination coefficient (t) are investigated. It is shown that during SID effect (t) increases.
Résumé Dans le présent travail on a procédé à une expérience pour déterminer les variations temporelles des principaux paramètres aéronomiques en utilisant des données expérimentales par la méthode A3 de mesure de l'absorption ionosphérique, la méthode phase-altitude et des données satellites aux rayons X durs. On a examiné les variations diurnes et les variations temporelles lors de SID effet durant le 21 Août 1969, de la densité électroniqueN(t) et du coefficient de récombinaison (t). On a montré que lors de SID effet (t) s'accroît.
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13.
Summary The propagator matrix is expressed in terms of cross-products of spherical Bessel functions and their derivatives. A fast computational algorithm is suggested. The matrix form of the variational principle with the boundary term is derived.
u nu u u u, n¶rt; u¶rt; nu¶rt;u uu u u u nuo¶rt;. ¶rt; au u . ¶rt; u uau nuuna u .
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14.
Summary The seismic energy released by global earthquake activity with time was correlated with F=||, where || is the absolute value of the change of the Sun's acceleration with time. For deep earthquakes and probability P=0.95, the coefficient of correlation was found to be around 0.4. For shallow earthquakes, the dependence was not proved.
¶rt;a u uu (1900–1982.) ua ¶rt; F=||,¶rt; || am au uu u a. mu (h>60 ) u ¶rt; mmu =0.95 uum uu ¶rt;muam0.45. nm mu auum a n¶rt;m¶rt;a.
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15.
au u uu mu a amu am a¶rt; mum ma¶rt;amuauau nmm m a, ¶rt;a m u ¶rt;u naam — aum¶rt; a, nu¶rt; a¶rt;u uu na¶rt;u am — nu muaua muam ¶rt; m ¶rt;a. ¶rt;aa n ma¶rt;amuauu nm naam ¶rt;u munaua nmmu ¶rt;.  相似文献   

16.
Summary The magnetic moments of Uranus and Neptune have been predicted using different scaling laws of planetary magnetism. The predictions for Uranus cover a broad band of values from very weak magnetic fields (tidal relations) to moderate fields (thermal convection hypothesis). Therefore, the direct measurements of this field by Voyager 2 (January 1986) will be very important for testing the individual hapotheses.
a m ama a ¶rt; amua nam ¶rt;a n aum m nam a a nm. aa n¶rt;nmu nuu mu, ¶rt;m u¶rt;am a aum n a nmu aa u u a nmu nma.

Presented at the Fifth Scientific Assembly of IAGA in Prague 1985.  相似文献   

17.
Summary The convection in a rapidly rotating, electrically conducting, horizontal fluid layer, non-constantly stratified and penetrated by an inhomogeneous magnetic field, is studied. The convection is investigated for various ratios of the thickness of the stable and unstable stratified part of the layer. The thermal model of the layer, as well as the analysis of the results have been treated with regard to the physical conditions in the liquid core of the Earth.
am u¶rt;m u m aa mn¶rt; u¶rt;uma nm mamuuau, nua ¶rt;¶rt; aum n. u u¶rt;m ¶rt; a mu m u mu u mu mamuuuao amu . ua ¶rt; , a u aau mam, n¶rt;a anm uuu u u¶rt; ¶rt; u.
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18.
Summary 30 years from the foundation of the Czechoslovak and Slovak Academy of Sciences in 1953 are commemorated in connection with 40 years elapsed from the decase of Prof. V. Láska, founder of gephysics in Cezchoslovakia. The progress achieved in its main lines and the outlooks of further development are described.
mam na 30-m u a u a aa¶rt;u a, ¶rt;a 1953-¶rt;, u u 40-mu m mu a . aa, amuuu auu. nua m mam u¶rt;au n anau u ¶rt;am nnmu ¶rt;a aumu.
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19.
Summary It has been demonstrated that the observed decrease in the second zonal geopotential harmonic linear in time and the secular decrease in the angular velocity of the Earth's rotation do not satisfy the relation defining the secular Love number k as constant during the whole history of the Earth's evolution. The discrepancy disappears if it is assumed thatdk/dt=–2.4×10–6 cy–1 .
aa, m a ¶rt;a au m aauunmuaa u u a ¶rt;a u mu au u ¶rt;mm mu, n¶rt; u a a nm mu umuu u. a uam, u ¶rt;nmumdk/dt=–2,4·10 –6 (mmu)–1 .
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20.
aamuam mam uu mn nma ma-au a. a¶rt; uua¶rt;uma mnam, uuma mnn¶rt;mu u mn nma m ¶rt;uamau au uu uma, n¶rt; m n¶rt; mn nm nu¶rt; a. 2. a u au Q=1,99 u 2,06×10–6 /2 am ¶rt;au mu n ua amu, ma mu (2,5×10–6 a/2 ) aum nam mm ¶rt;uana. um mm am na m¶rt;, ¶rt;¶rt; nu¶rt;m am mam.  相似文献   

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