Reconstruction and prediction of the total solar irradiance: From the Medieval Warm Period to the 21st century     

《New Astronomy》2015

  相似文献   

Maintenance and development of the Ural high and its contribution to severe cold wave activities in winter 2020/21          下载免费PDF全文

Jingbei Peng  Shuqing Sun  Bomin Chen 《大气和海洋科学快报》2022,15(2):54-58

2020年底至2021年初,连续两次强寒潮入侵中国东部地区,导致大范围强降温.本文研究这两次寒潮的特征和形成机理.主要结果如下:从2020年12月中旬到2021年1月中旬,乌拉尔山地区维持一宽阔的高压脊.脊前北风的维持和加强导致局地斜压性增加,导致下游横槽槽底等高线梯度加大,冷平流加强,西伯利亚高压加强和向南扩张.准定...  相似文献   

The Tully-Fisher relations of the Eridanus group of galaxies     

A. Omar  K. S. Dwarakanath 《Journal of Astrophysics and Astronomy》2006,27(1):7-23

The Tully-Fisher (TF) or the luminosity-linewidth relations of the galaxies in the Eridanus group are constructed using the HI rotation curves and the luminosities in the optical and in the near-infrared bands. The slopes of the TF relations (absolute magnitudevs log2V _flat) are −8.6 ± 1.1, −10.0 ±1.5, −10.7 ±2.1, and −9.7 ±1.3 in the R, J, H, and K bands respectively for galaxies having flat HI rotation curves. These values of the slopes are consistent with those obtained from studies of other groups and clusters. The scatter in the TF relations is in the range 0.5-1.1 mag in different bands. This scatter is considerably larger compared to those observed in other groups and clusters. It is suggested that the larger scatter in the TF relations for the Eridanus group is related to the loose structure of the group. If the TF relations are constructed using the baryonic mass (stellar +HI + Helium mass) instead of the stellar luminosity, nearly identical slopes are obtained in the R and in the near-infrared bands. The baryonic TF (baryonic massvs log2V _flat) slope is in the range 3.5–4.1.  相似文献   

Open cluster ASCC21 as a probable birthplace of the neutron star Geminga     

V. V. Bobylev  A. T. Bajkova 《Astronomy Letters》2009,35(6):396-405

We analyze the encounters of the neutron star (pulsar) Geminga with open star clusters in the OB association Ori OB1a through the integration of epicyclic orbits into the past by taking into account the errors in the data. The open cluster ASCC21 is shown to be the most probable birthplace of either a single progenitor star for the Geminga pulsar or a binary progenitor system that subsequently broke up. Monte Carlo simulations of Geminga-ASCC21 encounters with the pulsar radial velocity V _r = ?100±50 km s^?1 have shown that close encounters could occur between them within ≤10 pc at about t = ?0.52 Myr. In addition, the trajectory of the neutron star Geminga passes at a distance of ≈25 pc from the center of the compact OB association λ Ori at about t = ?0.39 Myr, which is close to the age of the pulsar estimated from its timing.  相似文献   

Elemental abundance analyses with DAO spectrograms: XXX. The middle B through early A stars ξ2 Ceti (B9 III), 21 Aquilae (B8 II‐III), ι Aquilae (B5 III), and ι Delphini (A2V)     

S.J. Adelman  P.C. Westbrook  A.F. Gulliver 《Astronomische Nachrichten》2010,331(4):378-383

This series of high quality elemental abundance analyses of mostly main‐sequence band normal and peculiar B, A, and F stars defines their properties and provides data for the comparison with the analyses of somewhat similar stars and with theoretical predictions. Most use high dispersion and high S/N (≥ 200) spectrograms obtained with CCD detectors at the long camera of the Coudé spectrograph of the 1.22‐m Dominion Astrophysical Observatory telescope. Here we reanalyze 21 Aql with better quality spectra and increase the number of stars consistently analyzed in the spectral range B5 to A2 by analyzing three new stars for this series. In the early A stars the normal and non‐mCP stars have abundances with overlapping ranges. But more stars are needed especially in the B5 to B9 range. ξ² Cet on average has a solar composition with a few abundances outside the solar range while both 21 Aql and ι Aql have abundances marginally less than solar. The abundances of ι Del are greater than solar with a few elements such as Ca being less than solar. It is an Am star (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

走向21世纪的矿床学   总被引：10，自引：2，他引：10  

翟裕生 《矿床地质》2001,20(1):10-14

文章简要回顾了百年来矿床学取得的重要进展，包括：（1）矿床成因分类的建立；（2）层控矿床研究与矿床多成因理论的兴起；（3）板块构造与区域成矿规律；（4）矿床模型；(5)型矿床研究；（6）海洋现代热液成矿作用的发现；（7）成矿演化的不可逆性与节律性等。针对21世纪中人类社会可持续发展的需要，矿床学研究出现了两个新趋势；（1）全球化；（2）矿业开发与环境保护一体化。面临着三个主要研究领域；（1）成矿理论的推陈出新；（2）研究开发新型矿产资源，建立广义的矿产资源地质学；（3）建立绿色矿业体制所需的矿床学基础研究。  相似文献   

第四纪科学发展展望   总被引：12，自引：0，他引：12       下载免费PDF全文

刘东生 《第四纪研究》2003,23(2):165-176

第四纪科学是地球科学的一个分支.20世纪中国第四纪研究的发展历史,可以分为两个阶段:1909～1949年,强调理论研究与实际应用的结合,适当地采用"全盘西化"的办法,将中国与世界先进的差距,由100年缩短为50年,跨越了一大步;1950～2000年,在完成国家需求的鼓励下,适当地越过经典研究范畴,参与环境问题和全球变化的研究,使得中国第四纪科学追赶了50年的差距.在21世纪开始之时,中国与国际第四纪研究的步伐有前有后,但基本上是站在同一起跑线上.对21世纪的第四纪研究,作者提出了以"研究过去只是为了未来"和"地学的文艺复兴在呼唤未来"为题的两个思路,从1)以人为本--务实社会需求;2)地球和人类共同的历史--人与自然和谐;3)我们需要自己提出理论--一种科学文化;4)群众需要第四纪--极大地提高人民的素质等4个方面展望了中国第四纪研究的新形势.  相似文献   

ISO observations of molecular hydrogen in the DR 21 bipolar outflow     

Michael D. Smith    Jochen Eislöffel  & Christopher J. Davis 《Monthly notices of the Royal Astronomical Society》1998,297(3):687-691

We demonstrate that a wide range of molecular hydrogen excitation can be observed in protostellar outflows at wavelengths in excess of 5 μm. Cold H₂ in DR 21 is detected through the pure rotational transitions in the ground vibrational level (0–0). Hot H₂ is detected in pure rotational transitions within higher vibrational levels (1–1, 1–2, etc.). Although this emission is relatively weak, we have detected two 1–1 lines in the DR 21 outflow with the ISO SWS instrument. We thus investigate molecular excitation over energy levels corresponding to the temperature range 1015–15 722 K, without the uncertainty introduced by differential extinction when employing near-infrared data.
This gas is thermally excited. We uncover a rather low H₂ excitation in the DR 21 West Peak. The line emission cannot be produced from single C-shocks or J-shocks; a range of shock strengths is required. This suggests that bow shocks and/or bow-generated supersonic turbulence is responsible. We are able to distinguish this shock-excited gas from the fluoresced gas detected in the K band, providing support for the dual-excitation model of Fernandes, Brand & Burton.  相似文献   

可持续发展综论   总被引：5，自引：1，他引：4  

夏汉平 《热带地理》1998,18(2):156-161

对可持续发展的概念、产生背景、内涵及其生态观进行了论述,提出了为实现可持续发展应采取的策略和应遵循的原则,剖析了中国必须实施可持续发展战略的原因,并指出要走具有中国特色的持续发展道路。  相似文献   

Timing of deglaciation on the northern Alpine foreland (Switzerland)     

Susan Ivy-Ochs  Jörg Schäfer  Peter W. Kubik  Hans-Arno Synal  Christian Schlüchter 《Eclogae Geologicae Helvetiae》2004,97(1):47-55

  相似文献