全文获取类型
收费全文 | 38031篇 |
免费 | 1341篇 |
国内免费 | 747篇 |
专业分类
测绘学 | 1082篇 |
大气科学 | 3273篇 |
地球物理 | 8914篇 |
地质学 | 13660篇 |
海洋学 | 2933篇 |
天文学 | 7717篇 |
综合类 | 220篇 |
自然地理 | 2320篇 |
出版年
2022年 | 257篇 |
2021年 | 504篇 |
2020年 | 511篇 |
2019年 | 490篇 |
2018年 | 1070篇 |
2017年 | 1059篇 |
2016年 | 1310篇 |
2015年 | 1010篇 |
2014年 | 1256篇 |
2013年 | 2106篇 |
2012年 | 1472篇 |
2011年 | 1733篇 |
2010年 | 1531篇 |
2009年 | 1895篇 |
2008年 | 1576篇 |
2007年 | 1448篇 |
2006年 | 1399篇 |
2005年 | 1172篇 |
2004年 | 1145篇 |
2003年 | 1067篇 |
2002年 | 966篇 |
2001年 | 880篇 |
2000年 | 821篇 |
1999年 | 703篇 |
1998年 | 714篇 |
1997年 | 721篇 |
1996年 | 535篇 |
1995年 | 543篇 |
1994年 | 506篇 |
1993年 | 415篇 |
1992年 | 382篇 |
1991年 | 348篇 |
1990年 | 402篇 |
1989年 | 343篇 |
1988年 | 289篇 |
1987年 | 387篇 |
1986年 | 325篇 |
1985年 | 418篇 |
1984年 | 454篇 |
1983年 | 439篇 |
1982年 | 414篇 |
1981年 | 387篇 |
1980年 | 367篇 |
1979年 | 344篇 |
1978年 | 375篇 |
1977年 | 322篇 |
1976年 | 306篇 |
1975年 | 328篇 |
1974年 | 282篇 |
1973年 | 301篇 |
排序方式: 共有10000条查询结果,搜索用时 31 毫秒
11.
12.
Roberto F. Viotti Lucio Angelo Antonelli Sonja Rebecchi Corinne Rossi 《Journal of Astrophysics and Astronomy》2002,23(1-2):19-22
We have investigated with BeppoSAX the long term behaviour of the harder X-ray component of the supposed supermassive binary
system η Car along its 5.52 year cycle. We have found that in March 1998 during egress from the last December 1997 eclipse,
this component was the same as outside eclipse, but for a large (×3.5) increase of NH
h
, that can be attributed to the presence or formation of opaque matter in front of the source near periastron. Unexpectedly,
at that time the iron 6.7 keV emission line was 40% stronger. BeppoSAX has for the first time found ahard X-ray tail extending to at least 50 keV, that cannot be adequately fitted with an additional hotter thermal component. The 2–100 keV
spectrum of η Car is instead well fitted with an absorbed powerlaw spectrum with photon index 2.53, suggesting non-thermal
emission as an alternative model for the core source. 相似文献
13.
Zsolt Sándor Bálint Érdi Carl D. Murray 《Celestial Mechanics and Dynamical Astronomy》2002,84(4):355-368
The dynamics of co-orbital motion in the restricted three-body problem are investigated by symplectic mappings. Analytical and semi-numerical mappings have been developed and studied in detail. The mappings have been tested by numerical integration of the equations of motion. These mappings have been proved to be useful for a quick determination of the phase space structure reflecting the main characteristics of the dynamics of the co-orbital problem. 相似文献
14.
15.
16.
The surface digital photometry for NGC 5253 and NGC 2915 is given. The luminosity profiles and colour gradients are discussed and compared. It is concluded that NGC 2915 differs from NGC 5253, both in the extension and intensity of the star burst event because of the kinematical behaviour of the captured gas.CONICET, Buenos Aires, Visiting Astronomer, Cerro Tololo Inter-American Observatory, La Serena, Chile, operated by NSF 相似文献
17.
M. J. Freyberg H. Bräuninger W. Burkert G. D. Hartner O. Citterio F. Mazzoleni G. Pareschi D. Spiga S. Romaine P. Gorenstein B. D. Ramsey 《Experimental Astronomy》2005,20(1-3):405-412
The Max-Planck-Institut für extraterrestrische Physik (MPE) in Garching, Germany, uses its large X-ray beam line facility PANTER for testing X-ray astronomical instrumentation. A number of telescopes, gratings, filters, and detectors, e.g. for astronomical satellite missions like Exosat, ROSAT, Chandra (LETG), BeppoSAX, SOHO (CDS), XMM-Newton, ABRIXAS, Swift (XRT), have been successfully calibrated in the soft X-ray energy range (< 15keV). Moreover, measurements with mirror test samples for new missions like ROSITA and XEUS have been carried out at PANTER. Here we report on an extension of the energy range, enabling calibrations of hard X-ray optics over the energy range 15–50 keV. Several future X-ray astronomy missions (e.g., Simbol-X, Constellation-X, XEUS) have been proposed, which make use of hard X-ray optics based on multilayer coatings. Such optics are currently being developed by the Osservatorio Astronomico di Brera (OAB), Milano, Italy, and the Harvard-Smithsonian Center for Astrophysics (CfA), Cambridge, MA, USA. These optics have been tested at the PANTER facility with a broad energy band beam (up to 50 keV) using the XMM-Newton EPIC-pn flight spare CCD camera with its good intrinsic energy resolution, and also with monochromatic X-rays between C-K (0.277 keV) and Cu-Kα (8.04 keV).
PACS: 95.55.Ka, 95.55.Aq, 41 50.+h, 07.85.Fv 相似文献
18.
19.
20.
Parametric transduction offers valuable advantages for underwater acoustic communications. Perhaps the most significant benefit is the fact that high directivity is achieved by means of a physically small transmit transducer. This feature may, ultimately, be employed to permit long-range, low-frequency communication using a compact source. The high directivity is desirable to combat multipath propagation and to achieve data communications in water which is shallow by comparison with range. A real-time, high data-rate “model” differential phase shift keying (DPSK) communication system has been constructed and demonstrated. This system uses parametric transduction, with a 300-kHz primary frequency and a 50-kHz secondary frequency. Experimental results show that the system can be employed to combat multipath propagation in shallow water and can achieve high data-rate text and color image transmission at 10 and 20 kb s-1 for 2-DPSK and 4-DPSK, respectively, through a transmission bandwidth of 10 kHz. The “model” system was developed to confirm performance predictions for a future, operational long-range link employing a 50-kHz primary frequency and a 5-kHz secondary frequency 相似文献