Interferometric space missions for the search for terrestrial exoplanets: Requirements on the rejection ratio     

Lisa Kaltenegger  Malcolm Fridlund  Anders Karlsson 《Astrophysics and Space Science》2006,306(3):147-158

The requirements on space missions designed to study Terrestrial exoplanets are discussed. We then investigate whether the design of such a mission, specifically the Darwin nulling interferometer, can be carried out in a simplified scenario. The key element here is accepting somewhat higher levels of stellar leakage. We establish detailed requirements resulting from the scientific rationale for the mission, and calculate detailed parameters for the stellar suppression required to achieve those requirements. We do this utilizing the Darwin input catalogue. The dominating noise source for most targets in this sample is essentially constant for all targets, while the leakage diminishes with the square of the distance. This means that the stellar leakage has an effect on the integration time only for the nearby stars, while for the more distant targets its influence decreases significantly. We assess the impact of different array configurations and nulling profiles and identify the stars for which the detection efficiency can be maximized.  相似文献   

Carbon isotope composition of long chain leaf wax n-alkanes in lake sediments: A dual indicator of paleoenvironment in the Qinghai-Tibet Plateau     

《Organic Geochemistry》2015

The carbon isotope composition (δ¹³C values) of long chain n-alkanes in lake sediments has been considered a reliable means of tracking changes in the terrigenous contribution of plants with C₃ and C₄ photosynthetic pathways. A key premise is that long chain leaf wax components used for isotope analysis are derived primarily from terrigenous higher plants. The role of aquatic plants in affecting δ¹³C values of long chain n-alkanes in lacustrine sediments may, however, have long been underestimated. In this study, we found that a large portion of long chain n-alkanes (C₂₇ and C₂₉) in nearshore sediments of the Lake Qinghai catchment was contributed by submerged aquatic plants, which displayed a relatively positive carbon isotope composition (e.g. −26.7‰ to −15.7‰ for C₂₉) similar to that of terrestrial C₄ plants. Thus, the use of δ¹³C values of sedimentary C₂₇ and C₂₉ n-alkanes for tracing terrigenous vegetation composition may create a bias toward significant overestimation/underestimation of the proportion of terrestrial C₄ plants. For sedimentary C₃₁, however, the contribution from submerged plants was minor, so that the δ¹³C values for C₃₁ n-alkane in surface sediments were in accord with those of the modern terrestrial vegetation in the Lake Qinghai region. Moreover, we found that changes in the δ¹³C values of sedimentary C₂₇ and C₂₉ n-alkanes were closely related to water depth variation. Downcore analysis further demonstrated the significant influence of endogenous lipids in lake sediments for the interpretation of terrestrial C₄ vegetation and associated environment/climate reconstruction. In conclusion, our results suggest that the δ¹³C values of sedimentary long chain n-alkanes (C₂₇, C₂₉ and C₃₁) may carry different environmental signals. While the δ¹³C values of C₃₁ were a reliable proxy for C₄/C₃ terrestrial vegetation composition, the δ¹³C values of C₂₇ and C₂₉ n-alkanes may have recorded lake ecological conditions and sources of organic carbon, which might be affected by lake water depth.  相似文献   

应用GPS数据和Slepian基函数反演川云渝地区陆地水储量变化     

成帅  袁林果  姜中山  刘中冠  张迪  徐小凤 《地球物理学报》2021,64(4):1167-1180

局部Slepian函数是将局部区域内的地球物理信号转化为空间谱的一种方法,其可以保证在球面上局部范围内获得最优谱平滑解,非常适用于局部范围地球物理信号的研究.本文利用中国陆态网西南地区72个测站的连续GPS观测资料分析川云渝地区陆地水负荷形变特征,并基于Slepian函数方法解算60阶的空间谱基函数,结合弹性质量负荷理论研究了川云渝地区2011年至2015年陆地水储量变化的时空分布模式.针对Slepian函数的边界效应问题,本文使用GLDAS格网数据计算得到站点处垂直负荷位移时间序列,然后利用该位移数据来进行水储量变化恢复实验,结果表明当边界扩充为3°时能较好地恢复GLDAS模型输出的陆地水储量变化.通过对比区域内GPS、GRACE、GLDAS得到的等效水高以及降雨数据,发现季节性降水是陆地水变化的一个重要驱动因子,GPS反演结果与GRACE和GLDAS数据具有较强的空间一致性.云南地区周年变化要强于川渝地区,其中云南西部的山区陆地水变化最大,约为30 cm,最小为川北以及重庆地区仅为7 cm.相较于GPS反演结果,GRACE与GLDAS明显低估了陆地水储量的季节性变化,分别达到24%和47%.比较分析地区内平均等效水高时间序列的相位发现,GPS得到的陆地水变化与降雨数据一致性较好,而GRACE与GLDAS存在一到两个月左右的时延.同时GPS能较好的探测出2015年1月左右南方地区大范围的强降水,而GRACE与GLDAS并没有体现出该现象,说明GPS能更为灵敏地探测到局部地区陆地水的变化.在站点等效水高时间序列上,GPS与GRACE的相关性总体上要优于GPS与GLDAS,陆地水周年变化较大的云南和四川西部地区站点三种数据间相关性较好,而其他季节性信号不明显的地区则相关性较差.本文的研究表明运用GPS-Slepian方法能够独立地监测高时空分辨率的陆地水储量变化,是作为当前补充GRACE观测资料空缺期的有益尝试.  相似文献   

A history of the global understanding of the Earth     

《Comptes Rendus Geoscience》2014,346(11-12):275-278

The author contributes to the development of a history of the global understanding of the Earth. He summarizes the main steps in the knowledge of the Earth's interior from antiquity to the present time and draws some lessons from this history.  相似文献   

A Review on Submarine Groundwater Discharge     

Liu Huatai  Guo Zhanrong 《地球科学进展》2014,29(7):774-785

Submarine Groundwater Discharge(SGD), an important part of global water cycle, is recently recognized as a research highlight on the land ocean interaction in the coastal zone. Firstly, This paper analyzes the components and driving force of SGD, and summarizes the main estimating methods of SGD and its individual strengths and weaknesses. Secondly, the paper describes the important role of SGD in transporting dissolved mass into the costal ocean and significant impacts on the ecological environment of costal ocean, and through analyzing the biogeochemical process in the mixing zone of fresh salt water, indicates the important position of subterranean estuary in studying submarine groundwater discharge. Finally, the paper points out the major problems currently existing in SGD research, then presents the future research direction.  相似文献   

气候变化对中国北方荒漠草原植被的影响   总被引：70，自引：2，他引：70  

李晓兵  陈云浩  张云霞  范一大  周涛  谢锋 《地球科学进展》2002,17(2):254-261

气候变化对陆地生态系统的影响及其反馈是全球变化研究的焦点之一。利用气候变量实现对遥感植被指数所表示的植被绿度信息的模拟，可以尝试作为表达生物圈过去和未来状态的一种途径。利用1961-2000年的气温、降水和1983-1999年的NOAA/AVHRR资料，分析了中国北方地带性植被类型荒漠草原植被分布区的短尺度气候的年际和季节变化，及其对植被的影响。结果表明，过去40年中该区域年际气候变化表现为增温和降水波动。年NDVI的最大值（NDVI_max）可以较好地反映气候的变化，过去17年中NDVI_max出现的时间略有提前。综合分析NDVI、植被盖度、NPP、区域蒸散量、土壤含水量及其气候的年际变化，表明增温加剧了土壤干旱化，降水和土壤含水量仍是制约本区植被生长的根本原因。  相似文献   

空间大地测量测定板块运动新进展   总被引：1，自引：0，他引：1  

赖锡安  徐菊生  王庆廷  张国安 《地球科学进展》2002,17(4):576-581

主要阐述利用空间大地测量测定和研究板块运动的研究成果及最新进展，并与地质学方法进行了比较，结果表明空间大地测量方法测定板块运动由单一手段发展为多种手段的综合，最新的研究是利用ITRF₉₆、ITRF₉₇地球参考架的站坐标及速率建立新的板块运动模型，这些模型和相同时期的地质模型，整体上一致但仍存在着差异。对于太平洋板块所有大地测量测定的运动速率均大于地质学模型，极位置的经度也有系统偏差。  相似文献   

岩石热导率的温压实验及分析   总被引：9，自引：0，他引：9  

赵永信  杨淑贞 《地球物理学进展》1995,10(1):104-113

岩石热导率是岩石热物性中最主要者，是研究地壳和上地幔热结构、地球深部热状态以及各种工程岩体内空气与围岩之间热交换的重要参数，该参数的测定不但是大地热流测量的重要内容之一，也是矿山采掘、石油开发和地热能利用不可缺少的工作。本文简要介绍了利用环形热源法在不同温压条件下对岩石热导率的测试和研究。文中不但介绍了测量原理和测量装置结构，并给出了不同岩性岩石在室温至１８０℃、常压至２２ＭＰａ状态下的测量结果，  相似文献   

Comment on “Constraints on the source of lunar cataclysm impactors” (Cuk et al., 2010, Icarus 207, 590-594)     

Renu Malhotra  Robert G. Strom 《Icarus》2011,216(1):359-362

Cuk et al. (Cuk, M., Gladman, B.J., Stewart, S.T. [2010]. Icarus 207, 590-594) argue that the projectiles bombarding the Moon at the time of the so-called lunar cataclysm could not have been mainbelt asteroids ejected by purely gravitational means, in contradiction with a conclusion that was reached by Strom et al. (Strom, R.G., Malhotra, R., Ito, T., Yoshida, F., Kring, D.A. [2005]. Science 309, 1847-1850). We demonstrate that Cuk et al.’s argument is erroneous because, contrary to their arguments, the lunar highlands do register the cataclysm impacts, lunar class 1 craters do not represent the size distribution of the cataclysm craters, and the crater size distributions on the late-forming basins are quite similar to those of the highlands craters, albeit at a lower number density due to the rapid decline of the impact flux during the cataclysm.  相似文献   

How common are Earth-Moon planetary systems?     

S. Elser  J. Stadel 《Icarus》2011,214(2):357-365

The Earth’s comparatively massive moon, formed via a giant impact on the proto-Earth, has played an important role in the development of life on our planet, both in the history and strength of the ocean tides and in stabilizing the chaotic spin of our planet. Here we show that massive moons orbiting terrestrial planets are not rare. A large set of simulations by Morishima et al. (Morishima, R., Stadel, J., Moore, B. [2010]. Icarus. 207, 517-535), where Earth-like planets in the habitable zone form, provides the raw simulation data for our study. We use limits on the collision parameters that may guarantee the formation of a circumplanetary disk after a protoplanet collision that could form a satellite and study the collision history and the long term evolution of the satellites qualitatively. In addition, we estimate and quantify the uncertainties in each step of our study. We find that giant impacts with the required energy and orbital parameters for producing a binary planetary system do occur with more than 1 in 12 terrestrial planets hosting a massive moon, with a low-end estimate of 1 in 45 and a high-end estimate of 1 in 4.  相似文献