全文获取类型
收费全文 | 230篇 |
免费 | 8篇 |
国内免费 | 1篇 |
专业分类
航空 | 84篇 |
航天技术 | 125篇 |
综合类 | 1篇 |
航天 | 29篇 |
出版年
2024年 | 1篇 |
2023年 | 6篇 |
2021年 | 2篇 |
2020年 | 5篇 |
2019年 | 6篇 |
2018年 | 12篇 |
2016年 | 1篇 |
2015年 | 1篇 |
2014年 | 8篇 |
2013年 | 9篇 |
2012年 | 8篇 |
2011年 | 6篇 |
2010年 | 8篇 |
2009年 | 16篇 |
2008年 | 20篇 |
2007年 | 34篇 |
2006年 | 4篇 |
2005年 | 6篇 |
2004年 | 2篇 |
2003年 | 5篇 |
2002年 | 2篇 |
2001年 | 4篇 |
2000年 | 5篇 |
1999年 | 7篇 |
1998年 | 14篇 |
1996年 | 3篇 |
1995年 | 1篇 |
1994年 | 34篇 |
1993年 | 2篇 |
1992年 | 2篇 |
1991年 | 3篇 |
1990年 | 2篇 |
排序方式: 共有239条查询结果,搜索用时 218 毫秒
81.
TRACE is a single-instrument solar mission that will be put into a Sunsynchronous polar orbit and will obtain continuous solar observations for about 8 months per year. It will collect images of solar plasmas at temperatures from 104 to 107 K, with 1-arcsec spatial resolution and excellent temporal resolution and continuity. With such data, we expect to gain a new understanding of many solar and stellar problems ranging from coronal heating to impulsive magnetohydrodynamic phenomena. 相似文献
82.
从工程应用角度,基于太阳、月球位置和卫星轨道根数推导了太阳和月球对地球同步轨道卫星红外地球敏感器干扰的计算公式及预报方法,同时给出了安全模式下卫星Z轴跟踪太阳时星上天线指向变化的计算模型。计算结果和卫星下传遥测数据验证了方法的正确性,可用于实际卫星管理。 相似文献
83.
Statistical study of radio drifting pulsation structures with associated CMEs and other observations
Chengming Tan Y.H. Yan Y.Y. Liu Q.J. Fu S.J. Wang H.R. Ji Z.J. Chen H.R. Jing 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(6):969-975
Solar radio burst, especially the fine structures (FSs) and the drifting pulsation structures (DPSs), may be used as an important diagnostics tool to draw the evolution map of the flare loop in the initial phase of solar flares. In this work, 52 radio events were found accompanying with DPSs. They were all observed with the Solar Radio Spectrometers (0.625–7.6 GHz) of China during 1998–2004. Combining the radio observations with LASCO-C2, Goes-8 SXR, Hα, EUV and Trace observations, we analyzed all these events and obtained some statistic conclusions: First, 88% DPSs take place at the initial phase of the radio burst, and their rich spectrum characteristics are helpful to understand the events further. Second, 83% DPSs are associated with CMEs or ejection events, and all the events are accompanied by Goes SXR flare. Third, for CMEs and DPSs, which take the first step, there is no significant predominance of either of them. The relationship between the DPSs and CMEs is still not clear in this study because of the lack of spatial resolution in the centimeter–decimeter band. However, the EIT or Trace ejection happened during the onset/end time of DPSs. They are signatures of the initial phase of CMEs. Two events will be illustrated to explain this. 相似文献
84.
M.C. Rabello-Soares B.J. Thompson D. Scherrer C. Morrow 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(8):1206-1211
Education and public outreach (EPO) is one of the four components of the International Heliophysical Year (IHY). It is fundamental in achieving one of IHY’s primary objectives which is to “demonstrate the beauty, relevance and significance of Space and Earth science to the world.” 相似文献
85.
Linhui Sui Gordon D. Holman Brian R. Dennis 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(6):976-983
We present observations of a C9.4 flare on 2002 June 2 in EUV (TRACE) and X-rays (RHESSI). The multiwavelength data reveal: (1) the involvement of a quadrupole magnetic configuration; (2) loop expansion and ribbon motion in the pre-impulsive phase; (3) gradual formation of a new compact loop with a long cusp at the top during the impulsive phase of the flare; (4) appearance of a large, twisted loop above the cusp expanding outward immediately after the hard X-ray peak; and (5) X-ray emission observed only from the new compact loop and the cusp. In particular, the gradual formation of an EUV cusp feature is very clear. The observations also reveal the timing of the cusp formation and particle acceleration: most of the impulsive hard X-rays (>25 keV) were emitted before the cusp was seen. This suggests that fast reconnection occurred during the restructuring of the magnetic configuration, resulting in more efficient particle acceleration, while the reconnection slowed after the cusp was completely formed and the magnetic geometry was stabilized. This observation is consistent with the observations obtained with Yohkoh/Soft X-ray Telescope (SXT) that soft X-ray cusp structures only appear after the major impulsive energy release in solar flares. These observations have important implications for the modeling of magnetic reconnection and particle acceleration. 相似文献
86.
Electron and proton acceleration by a super-Dreicer electric field is further investigated in a non-neutral reconnecting current
sheet (RCS) with a variable plasma density. The tangential B
z
and transverse magnetic field components B
x
are assumed to vary with the distances x and z from the X nullpoint linearly and exponentially, respectively; the longitudinal component (a ‘guiding field’) is accepted
constant. Particles are found to gain a bulk of their energy in a thin region close to the X nullpoint where the RCS density
increases with z exponentially with the index λ and the tangential magnetic field B
x
also increases with z exponentially with the index α. For the RCS with a constant density (λ = 0), the variations of the tangential magnetic field
lead to particle power-law energy spectra with the spectral indices γ1 being dependent on the exponent α as:
for protons and
for electrons in a strong guiding field (β > 10−2) and
for electrons in a moderate or weak guiding field (β > 10−4). For the RCS with an exponential density increase in the vicinity of the X nullpoint (λ≥ 0) there is a further increase
of the resulting spectral indices γ that depends on the density exponent index λ as
for protons and for electrons in weaker guiding fields and as
for electrons in stronger guiding fields. These dependencies can explain a wide variety (1.5–10) of particle spectral indices
observed in solar flares by the variations of a magnetic field topology and physical conditions in a reconnecting region.
This can be used as a diagnostic tool for the investigation of the RCS dynamics from the accelerated particle spectra found
from hard X-ray and microwave emission. 相似文献
87.
R.D. Bentley A. Csillaghy J. Aboudarham C. Jacquey M.A. Hapgood K. Bocchialini M. Messerotti J. Brooke P. Gallagher P. Fox N. Hurlburt D.A. Roberts L. Sanchez Duarte 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
Heliophysics is a new research field that explores the Sun–Solar System Connection; it requires the joint exploitation of solar, heliospheric, magnetospheric and ionospheric observations. 相似文献
88.
The coronal magnetic field in the northern polar coronal hole in 1986 is predicted on the basis of the photospheric magnetic field observations and the horizontal current-current sheet coronal model (Zhao and Hoeksema, 1993). The predicted magnetic field intensity is stronger near the center of the hole than near the edge. The calculated expansion factor for the entire hole does not match the expansion factor of any flux tube in the hole, suggesting that it would not be appropriate to use the expansion factor for entire hole to represent the divergence of the flux tube in analyzing the acceleration and heating of the plasma in coronal holes. 相似文献
89.
屈建军 《西安航空技术高等专科学校学报》2002,20(4):33-35,39
孙中山晚年复归儒学,根源于其坚定的民族立场,对西方“文明”的反省,以及建设革命党和从事政党政治的需要。 相似文献
90.