共查询到20条相似文献，搜索用时 187 毫秒
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美国国家大气研究中心优先研究领域新特点 总被引：1，自引：0，他引：1
美国国家大气研究中心于2005年11月提出了新的战略计划。该计划突出的新特点在于无论科学研究活动还是教育、观测设施等方面的战略目标和优先领域,都是以地球系统研究为中心。如在科学研究方面的战略目标确定为：认识地球系统的作用、准确预报地球系统的演变。相应的优先研究领域则为：研究和了解地球和太阳的自然变率;地球系统各分量的相互作用;地球系统预报;人类活动与地球系统的演变等。鉴于NCAR在国际大气科学界的地位,这种以地球系统为中心的优先研究领域对我国大气科学及地球科学研究有一定的借鉴意义,同时也将促使大气科学工作者摆脱传统天气、气候概念的束缚,站在更高的高度来科学审视学科的发展。 相似文献
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SHARE Asia自动气象站网络：喜马拉雅山—喀喇昆仑山地区气候研究的一个必要组成部分 总被引：1，自引：0，他引：1
E. Vuillermoz L. Bertolani C. Smiraglia GP. Verza G. Tartari A. Marinoni P. Bonasoni 《地球科学进展》2006,21(12):1244-1253
Ev K2 CNR SHARE Asia计划的目标就是建立一个沿喜马拉雅山—喀喇昆仑山脉的监测网络，为气象学和气候研究提供参数，特别是为季风变化、大气化学、冰川学、高海拔湖沼学和古湖沼学等研究，同时也为准确地确定地球表面坐标。SHARE Asia 计划的一个特殊的目的是发展一套完整的测量系统，以满足不断进步的环境与地球科学；促进当地的技术升级和建设的能力。
就像WMO CEOP 和UNEP ABC一样，SHARE Asia 气象—气候及大气化学观测站已经成为重要的国际科学计划的一部分。 相似文献
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海洋和大气是地球系统的重要组成部分，其在全球气候变化中具有重要作用。上层海洋与低层大气研究（SOLAS）作为IGBPII第一个新的核心计划，以海洋中深度在100 m以上的水层和 1 000 m以下的大气边界层为主要研究对象，通过多学科的交叉研究，以揭示海洋与大气相互作用的物理和生物地球化学过程耦合及其在气候变化中的作用。SOLAS科学计划得到了世界各国的积极响应，已有16个国家向国际SOLAS科学委员会提交了SOLAS进展状况的国家报告。我国也制定了自己的科学研究计划重点研究中国近海的大气物质入海、海洋温室气体排放、海-气界面上的物质和能量交换过程及其对气候和环境的影响和反馈。 相似文献
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对近年升空的CHAMP和GRACE和将于2007年升空的GOCE卫星在测定地球重力场方面的技术特点和初步成果进行了回顾、比较和评估。并对它们今后在静态和动态的地球重力场构模方面可能的进展作一展望。现在只用一颗重力卫星的轨道摄动数据，就可以以前所未有的可靠性和精确性来求定地球重力场的长波和部分中波。如CHAMP重力卫星的33个月数据所求定的地球重力场模型,相对于曾利用多颗卫星资料所推算的GR1M5 S1重力场模型,在长波方面的精度和可靠性都有很大改善。而GRACE重力卫星的 110天数据所导出成果的空间分辨率，又优于CHAMP的33个月的数据成果。GRACE卫星还有一个重要任务，就是测定重力场非潮汐的短期性或准实时的变化。还介绍了新发表的一个联合地球重力场模型EIGEN CG03C, 360完全阶次，分辨率约30′。CG03C同CHAMP/GRACE以前的重力场模型比较，在400 km波长的精度方面改善了一个量级，大地水准面的精度改善了3 cm，重力异常的精度改善了0.4 mgal。 相似文献
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重力卫星五年运行对求定地球重力场模型的进展和展望 总被引：3，自引：0，他引：3
对近年升空的CHAMP和GRACE和将于2007年升空的GOCE卫星在测定地球重力场方面的技术特点和初步成果进行了回顾、比较和评估。并对它们今后在静态和动态的地球重力场构模方面可能的进展作一展望。现在只用一颗重力卫星的轨道摄动数据,就可以以前所未有的可靠性和精确性来求定地球重力场的长波和部分中波。如CHAMP重力卫星的33个月数据所求定的地球重力场模型,相对于曾利用多颗卫星资料所推算的GRlM5-S1重力场模型,在长波方面的精度和可靠性都有很大改善。而GRACE重力卫星的110天数据所导出成果的空间分辨率,又优于CHAMP的33个月的数据成果。GRACE卫星还有一个重要任务,就是测定重力场非潮汐的短期性或准实时的变化。还介绍了新发表的一个联合地球重力场模型EIGEN-CG03C,360完全阶次,分辨率约30′。CG03C同CHAMP／GRACE以前的重力场模型比较,在400km波长的精度方面改善了一个量级,大地水准面的精度改善了3cm,重力异常的精度改善了0．4mgal。 相似文献
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《Russian Geology and Geophysics》2014,55(7):854-863
The position of lithospheric magnetic anomalies, detected in total magnetic intensity and the vertical component of the magnetic field, has been determined for Siberia using data from the CHAMP satellite. The paper describes the technique for the satellite data processing and the ways of recognition of regional lithospheric magnetic anomalies from satellite-measured values of the total geomagnetic field, which are obtained from several sources (external and internal with respect to the Earth’s surface). Maps of magnetic-field anomalies of different scales have been constructed for several regions of Siberia depending on the method of areal averaging. The possible geologic and physical nature of the magnetic anomalies and their relationship with deep-seated crustal structures are considered. Preliminary interpretation of the magnetic-field maps shows that the anomalies are connected with the present-day large geologic and geophysical elements of the basement. The features of the lithospheric magnetic field, as a parameter reflecting the present position of tectonic structures and their physical properties, can be used for their contouring in combination with other geological and geophysical methods. 相似文献
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《Comptes Rendus Geoscience》2007,339(14-15):917-927
Plate tectonics shaped the Earth, whereas the Moon is a dry and inactive desert, Mars probably came to rest within the first billion years of its history, and Venus, although internally very active, has a dry inferno for its surface. Here we review the parameters that determined the fates of each of these planets and their geochemical expressions. The strong gravity field of a large planet allows for an enormous amount of gravitational energy to be released, causing the outer part of the planetary body to melt (magma ocean), helps retain water on the planet, and increases the pressure gradient. The weak gravity field and anhydrous conditions prevailing on the Moon stabilized, on top of its magma ocean, a thick buoyant plagioclase lithosphere, which insulated the molten interior. On Earth, the buoyant hydrous phases (serpentines) produced by reactions between the terrestrial magma ocean and the wet impactors received from the outer solar system isolated the magma and kept it molten for some few tens of million years. The planets from the inner solar system accreted dry: foundering of wet surface material softened the terrestrial mantle and set the scene for the onset of plate tectonics. This very same process also may have removed all the water from the surface of Venus and added enough water to its mantle to make its internal dynamics very strong and keep the surface very young. Because of a radius smaller than that of the Earth, not enough water could be drawn into the Martian mantle before it was lost to space and Martian plate tectonics never began. The radius of a planet is therefore the key parameter controlling most of its evolutional features. 相似文献
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As a first approximation, the Earth is a sphere; as a second approximation, it may be considered an ellipsoid of revolution.
The deviations of the actual Earth’s gravity field from the ellipsoidal “normal” field are so small that they can be understood
to be linear. The splitting of the Earth’s gravity field into a “normal” and a remaining small “disturbing” field considerably
simplifies the problem of its determination. Under the assumption of an ellipsoidal Earth model, high observational accuracy
is achievable only if the deviation (deflection of the vertical) of the physical plumb line, to which measurements refer,
from the ellipsoidal normal is not ignored. Hence, the determination of the disturbing potential from known deflections of
the vertical is a central problem of physical geodesy. In this paper, we propose a new, well-promising method for modelling
the disturbing potential locally from the deflections of the vertical. Essential tools are integral formulae on the sphere
based on Green’s function with respect to the Beltrami operator. The determination of the disturbing potential from deflections
of the vertical is formulated as a multiscale procedure involving scale-dependent regularized versions of the surface gradient
of the Green function. The modelling process is based on a multiscale framework by use of locally supported surface curl-free
vector wavelets.
相似文献
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Physical state of the very early Earth 总被引：1，自引：0，他引：1
Yutaka Abe 《Lithos》1993,30(3-4):223-235
The earliest surface environment of the Earth is reconstructed in accordance with the planetary formation theory. Formation of an atmosphere is an inevitable consequence of Earth's formation. The atmosphere near the close of accretion is composed of 200 300 bars of H2 and H2O, and several tens of bars of CO and CO2. Either by the blanketing effect of the proto-atmosphere or heating by large planetesimal impacts a magma ocean is formed during accretion. We can distinguish three stages for the thermal evolution of the magma ocean and proto-crust. Stage 0 is characterized by a super-liquidus (or completely molten) regime near the surface. At this stage the surface of the Earth is covered by a super-liquidus magma ocean. No chemical differentiation is expected during this stage. Once the energy flux released by planet formation decreases to the 200 W/m2 level the super-liquidus magma ocean then disappears within a time interval of 1 m.y. This is the transition from stage 0 to 1. Stage 1 is characterized by a partially molten magma ocean. In the magma ocean consisting of 20 30% partial melt, heat transport is controlled by melt-solid separation (a type of compositional convection) rather than thermal convection. Chemical differentiation of the mantle mainly occurs in this stage. Once the energy flux drops to the 160 W/m2 level, more than 90% of water vapor in the proto-atmosphere condense to form the proto-oceans. Several tens of bars of CO and CO2 remain in the atmosphere just after formation of the oceans. Water oceans are occasionally evaporated by large impacts. After each such event, recondensation of the ocean takes several hundred years. Although the surface is covered by a chilled proto-crust, it is short-lived because of extensive volcanic resurfacing activity as well as meteorite impacts resurfacing. This stage ends when the energy flux drops to 0.1 1 W/m2 level. The duration time of stage 1 is estimated to be several hundred million years (the best estimate is about 400 m.y.). Stage 2 is characterized by solid state convection. This stage continues to the present day. One of the most important change on the proto-Earth is the transition from stage 1 to 2, which occurs several hundred million years after the Earth formation. Long-lived crust is formed only after this transition. 相似文献
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In this paper we provide a literature review of the geological and geographic problems that were successfully solved via the application of the Gravity Recovery And Climate Experiment (GRACE) satellite mission data. GRACE is a gravitational satellite mission whose purpose is the precise mapping of variations of the Earth’s gravity field. The data have high resolution, which provides the opportunity to solve many geological and geographical problems. 相似文献
