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31.
Summary Two groups of basaltic rocks with normal and reversed NRM were examined. It was found that in both groups the primary NRM, synchronous with the period of rock formation, is preserved. Relations of the primary NRM to the origin and the degree of oxidation of magnetic minerals were considered in detail. 相似文献
32.
Sławomir Breiter 《Celestial Mechanics and Dynamical Astronomy》1999,74(4):253-274
Eccentricity resonances between the secular motion of an Earth satellite's orbit and the longitudes of the Sun and the Moon
are studied within a Hamiltonian framework. The problem is approximated in a traditional manner, with the Earth's potential
including only the second zonal harmonic, and a Hill‐type approximation for perturbing bodies. For a family of 10 resonances,
stable and unstable points are identified and libration widths are estimated. Numerical values are given for the maximum variation
of eccentricity available at each resonance. The respective amplitudes of the perigee heights' librations range from 2 to
750 km. The resonances of the solar origin are generally stronger than their lunar counterparts.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
33.
Sylwia Grabowska Jerzy W. Mietelski Krzysztof Kozak Paweł Gaca 《Journal of Atmospheric Chemistry》2003,46(2):103-116
The Petryanov air filters combined into half-year sets were analyzed for the presence of 40K, 137Cs and 22Na by means of low-background gamma rays spectrometry. Each sample contains aerosols from more than 1 Mm3 of air. Samples were collected in ground level air at Kraków (Southern Poland) from 1996 to 2002. Activity concentrations of 40K are almost constant with the mean of 14.7± 4.5 Bq m–3. Activity concentrations of 137Cs, which are on the level of single Bq m– 3 show exponential decrease with effective half-life time of 7.07± 0.77 years. The cosmogenic 22Na shows a strong seasonal variation with significant different mean values activity concentration between 0.333± 0.095 Bq m–3 and 0.137± 0.045 Bq m–3, for summer and winter, respectively. Moreover, the activity ratio for two cosmogenic radionuclides: 22Na and measured previously 7Be show also changes with statistically significant seasonal differences. The lower values were found during winters. The mechanisms which might govern this ratio are discussed. The conclusion is that transport of 22Na during summer seems to be so much effective, that results in kind of relative depletion of stratosphere of this nuclide. 相似文献
34.
Sławomir Breiter 《Celestial Mechanics and Dynamical Astronomy》2003,85(3):209-218
Fundamental models are the simplest, one degree of freedom Hamiltonians that serve as a tool to understand the qualitative effects of various resonances. A new, extended fundamental model (EFM) is proposed in order to improve the classical, Andoyer type, second fundamental model (SFM). The EFM Hamiltonian differs from the SFM by the addition of a term with the third power of momentum; it depends on two free parameters. The new model is studied for the case of a first-order resonance, where up to five critical points can be present. Similarly, to the respective SFM, it admits only the saddle-node bifurcations of critical points, but its advantage lies in the capability of generating the separatrix bifurcations, known also as saddle connections. The reduction of parameters for the EFM has been performed in a way that allows the use of the model in the case of the so-called abnormal resonance. 相似文献
35.
The analysis of application of two dynamical models (``Earth–Moon' and``barycentre' model) in the motion of Near Earth Asteroids was performed. Mainaim was the quantitative estimation of the influence of lunar perturbations on the motionof NEA. Additionally, basic tests of application of numerical methods weremade (RMVS3 and B–S methods). The orbits of 1083 Apollo–Aten–Amor and 7selected AAA objects were adopted as test particles in numerical integrationof the motion. The comparison between results obtained by both dynamicalmodels is discussed in detail. In specific cases, the application of the``Earth–Moon' dynamical model is very important and cannot be neglected incomputations of orbits. 相似文献
36.
Stanisław P. Kasperczuk 《Celestial Mechanics and Dynamical Astronomy》2000,76(4):215-227
In a recent paper Ballersteros and Ragnisco (1998) have proposed a new method of constructing integrable Hamiltonian systems.
A new class of integrable systems may be devised using the following sequence:
, where A is a Lie algebra
is a Lie–Poisson structure on R
3, C is a Casimir for
is a reduced Poisson bracket and (A, ▵) is a bialgebra. We study the relation between a Lie-Poisson stucture Λ and a reduced Poisson bracket
, which is a key element in using the Lie algebra A to constructing this sequence. New examples of Lie algebras and their
related integrable Hamiltonian systems are given.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
37.
The Harvard CMT catalogue contains 481 shallow earthquakes that occurred between 1 January 1977 and 30 November 2005 within
a broad region defined by the geographical latitude from 3°S to 14°N and by the longitude from 91°E to 102°E. There are 230
events that occurred before the great earthquake of 26 December 2004. Their surface distribution is not uniform and the source
area of the 2004 great event appears as an area of seismic quiescence with a radius of about 100 km. There are 186 events
that occurred between the two great earthquakes of 26 December 2004 and 28 March 2005. Practically all of them are located
to the northwest from the great earthquake of 2005, that in turn was followed by 63 events, mostly located to the southeast.
The cumulative seismic moment from earthquakes before the occurrence of the great event of 2004 increased rather regularly
with time, with sudden increase about twenty years and two years before the occurrence of the great event. The seismic moment
of earthquakes between the two great events increased rapidly during the first ten-fifteen days, then flattened out and increased
slowly with time. After the great event of 2005 the seismic moment shows quiet increase during some 115 days, then sudden
jump, followed by very small activity till the end of our observations. From the spatial distribution of seismic moment of
earthquakes that occurred before the great event of 2004 it follows that its largest release appeared to the southeast from
the great event, around the rupture area of the great earthquake of 2005. The largest release of seismic moment from earthquakes
between the two great events is observed in the vicinity of the 2004 event and further up to the north. The seismic moment
from earthquakes that occurred after the great event of 2005 was mostly released in its vicinity and further down to the south. 相似文献
38.
Lightning discharges monitored by the SAFIR network system in Poland have been additionally identified over the 100×100 km
area near Warsaw by single-point independent recordings of electric field and Maxwell current rapid changes. The data collected
in summer thunderstorm days of 2002 showed some untypical properties of the lightning discharges which are rarely observed.
Especially remarkable was a number of ground multi-stroke flashes with the return strokes (RS) which transported to the earth
charges of opposite signs. Bipolar flashes (BF) of this kind were mostly involved in the events in which the nearby intracloud
(ic) and cloud-to-ground (c-g) discharges were very closely associated in time. Events of such a close collocation of two
different types of lightning discharges, previously called the complex lightning discharge events (CLDE), were quite often
observed during summer thunderstorms in Poland.
The events of this kind, i.e. 8 flashes, identified by the SAFIR detection system as BF’s present the multiple stroke flashes
of the mean horizontal separation distance between striking points of particular RS equal to (2.8 ± 2.1) km and of the mean
time interval between strokes of (46.8 ± 74.4) ms. The time separation between the observed BF and the adjacent ic flashes
was from 0.1 to 335 ms, and horizontal separation distance between them ranged from 1.8 to 14.5 km. The multiplicity of the
recorded BF’s ranged from 2 to 4 strokes. Four of these BF’s followed the ic discharge, but the other three preceded the ic
and one was alone with no close ic. 相似文献
39.
B. Offerle C. S. B. Grimmond K. Fortuniak K. Kłysik T. R. Oke 《Theoretical and Applied Climatology》2006,84(1-3):103-115
Summary Energy fluxes have been measured over an area near the centre of the city of Łódź, Poland, since November 2000. The site was
selected because the building style (surface cover and morphology) is typical of European cities, yet distinct from the majority
of cities where energy balance observations have been studied thus far. The multi-year dataset permits consideration of temporal
changes in energy balance partitioning over a wide range of seasonal and synoptic conditions and of the role of heat storage
and anthropogenic fluxes in the energy balance. Partitioning of net radiation into the turbulent fluxes is consistent in the
two years, with the largest differences occurring due to differing precipitation. The monthly ensemble diurnal cycles of the
turbulent fluxes over the two years are similar. The largest differences occur during the July–September period, and are attributable
to greater net radiation and lower rainfall in 2002. The latent heat flux accounts for approximately 40% of the turbulent
heat transfer on an annual basis. The average daily daytime Bowen ratio and its variability are slightly reduced during the
summer (growing) season. Anthropogenic heat is a significant input to the urban energy balance in the winter. The fluxes observed
in this study are consistent with results from other urban sites. 相似文献
40.
Summary Data from two automatic stations in Łódź (one urban and one rural) for the period 1997–2002 are analyzed to reveal urban–rural
contrasts of such parameters as air temperature, relative humidity, water vapour pressure and wind speed. Under favourable
weather conditions the highest temperature differences between the urban and rural station exceeds 8 °C. Relative humidity
is lower in the town, sometimes by more than 40%. Water vapour pressure differences can be either positive (up to 5 hPa) or
negative (up to −4 hPa). Wind speed at the urban station is on average lower by about 34% in night and 39% during daytime.
Regression analysis shows that for rural winds lower than 1.13 m s−1 urban winds can be stronger than rural speeds. Attention has also been paid to singularities in the course of the analyzed
parameters over 24 hour periods. It is shown that the typical course of the urban heat island intensity under favourable conditions
is similar in all season. Four stages of this course have been distinguished. Wind speed differences also seem to change in
a typical way. Case studies show that humidity contrasts, unlike temperature, can evolve in different ways under fine weather
conditions. Types of relative humidity evolution are proposed. 相似文献