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271.
We study the nature of quiet-Sun oscillations using multi-wavelength observations from TRACE, Hinode, and SOHO. The aim is to investigate the existence of propagating waves in the solar chromosphere and the transition region by analyzing the statistical distribution of power in different locations, e.g. in bright magnetic (network), bright non-magnetic and dark non-magnetic (inter-network) regions, separately. We use Fourier power and phase-difference techniques combined with a wavelet analysis. Two-dimensional Fourier power maps were constructed in the period bands 2??C?4?minutes, 4??C?6?minutes, 6??C?15?minutes, and beyond 15?minutes. We detect the presence of long-period oscillations with periods between?15 and 30?minutes in bright magnetic regions. These oscillations were detected from the chromosphere to the transition region. The Fourier power maps show that short-period powers are mainly concentrated in dark regions whereas long-period powers are concentrated in bright magnetic regions. This is the first report of long-period waves in quiet-Sun network regions. We suggest that the observed propagating oscillations are due to magnetoacoustic waves, which can be important for the heating of the solar atmosphere. 相似文献
272.
We performed high resolution spectroscopy of the solar corona during the total solar eclipse of 22 July 2009 in two emission
lines: the green line at 5303 ? due to Fe xiv and the red line at 6374 ? due to Fe x, simultaneously from Anji (latitude 30°28.1′ N; longitude 119°35.4′ E; elevation 890 m), China. A two-mirror coelostat with
100 cm focal length lens produced a 9.2 mm image of the Sun. The spectrograph using 140 cm focal length lens in Littrow mode
and a grating with 600 lines per millimeter blazed at 2 μm provided a dispersion of 30 m? and 43 m? per pixel in the fourth
order around the green line and third order around the red line, respectively. Two Peltier cooled 1k × 1k CCD cameras, with
a pixel size of 13 μm square and 14-bit readout at 10 MHz operated in frame transfer mode, were used to obtain the time sequence
spectra in two emission lines simultaneously. The duration of totality was 341 s, but we could get spectra for 270 s after
a trial exposure at an interval of 5 s. We report here on the detection of intensity, velocity, and line width oscillations
with periodicity in the range of 25 – 50 s. These oscillations can be interpreted in terms of the presence of fast magnetoacoustic
waves or torsional Alfvén waves. The intensity ratios of green to red emission lines indicate the temperature of the corona
to be 1.65 MK in the equatorial region and 1.40 MK in the polar region, relatively higher than the expected temperature during
the low activity period. The width variation of the emission lines in different coronal structures suggests different physical
conditions in different structures. 相似文献
273.
A. Banerjee 《Geological Journal》1969,6(2):181-184
The Viséan sediments between Rhydymwyn and Erryrys have been mapped and divided into a number of lithologic units. A combined study of field relationships and petrography has been made and conclusions have been drawn about depositional environments. 相似文献
274.
Kinwat crystalline inlier exposes Palaeoproterozoic granitoids belonging to the northern extensions of younger phase of Peninsular
gneissic complex (PGC) within Deccan Trap country in Eastern Dharwar Craton (EDC) and bounded in south by a major NW-SE trending
lineament (Kaddam fault). Geochemically, the Kinwat granitoids are similar to high-K, calc-alkaline to shoshonite magnesian
granitoids and subdivided into two major groups, i.e. felsic group (pink and grey granites) and intermediate to felsic group
(hybrid granitoids). The felsic group (∼67–74% SiO2) shares many features with Neoarchaean to Palaeoproterozoic high potassic granites of PGC such as higher LILE and LREE content
and marked depletion in Eu, P and HFSE, especially Nb, Ti, relative to LILE and LREE. The hybrid granitoids (∼58–67% SiO2) have comparatively higher Ca, Mg and Na contents and slightly lower REE content than the granitoids of felsic group. Both,
felsic and hybrid granitoids are metaluminous to weakly peraluminous and belong to highly fractionated I-type suite as evidenced
by negative correlation of SiO2 with MgO, FeOt, CaO, Na2O, Al2O3, whereas K2O, Rb and Ba show sympathetic relationship with SiO2. Moderate to strong fractionated REE patterns (Ce/YbN: ∼54–387) and strong negative Eu anomalies (Eu/Eu*: 0.13–0.41) are quite apparent in these granitoids. The geochemical characteristics
together with mineralogical features such as presence of biotite±hornblende as the dominant ferromagnesian mineral phases
point towards intracrustal magma source, i.e. derivation of magma by partial melting of probably tonalitic igneous protolith
at moderate crustal levels for felsic granites, whereas hybrid granitoids appear to be products of juvenile mantle-crust interaction,
in an active continental margin setting. 相似文献