Investigating the age and structure of the infrared old open clusters LK 1, LK 10, FSR 1521 and FSR 1555     

C. Bonatto  E. Bica 《Monthly notices of the Royal Astronomical Society》2009,392(1):483-496

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The topology and polarization of subbeams associated with the 'drifting' subpulse emission of pulsar B0943+10 – V. A new look at the low-frequency burst-mode emission     

Svetlana A. Suleymanova  Joanna M. Rankin 《Monthly notices of the Royal Astronomical Society》2009,396(2):870-877

This paper reports new observations of pulsar B0943+10 carried out at the Pushchino Radio Astronomy Observatory (PRAO) at the low radio frequencies of 42, 62 and 112 MHz. B0943+10 is well known for its exquisitely regular burst-mode (B-mode) drifting subpulses as well as its weaker and chaotic quiescent mode. Earlier Arecibo investigations at 327 MHz have identified remarkable, continuous changes in its B-mode subpulse drift rate and integrated-profile shape with durations of several hours. These PRAO observations reveal that the changes in profile shape during the B-mode lifetime are strongly frequency dependent – namely the measured changes in the component amplitude ratio are more dramatic at 327 and 112 MHz as compared with those at 62 and 42 MHz. The differences, however, are most marked during the first several tens of minutes after B-mode onset; after an hour or so the profile shape changes tend to be more similar at all four frequencies. We also have found that the linear polarization of the integrated profile increases continuously throughout the lifetime of the B mode, going from hardly 10 per cent just after onset to some 40–50 per cent after several hours. Pulsar B0943+10's B mode thus provides a unique new opportunity to investigate continuous systematic changes in the plasma flow within the polar flux tube. While refraction in the pulsar's magnetosphere may well play some role, we find that the various frequency-dependent effects, both between and within the two modes, can largely be understood geometrically. If the modes and B-mode decay reflect systematic variations in the carousel-'spark' radius and emission height then a specific set of profile and linear polarization changes would be expected.  相似文献   

The silicate and carbon-rich models of CoRoT-7b, Kepler-9d and Kepler-10b     

Yan-Xiang Gong  Ji-Lin Zhou 《天体物理学报》2012,(6):678-692

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Late Quaternary glaciations in the Cogarbu valley,Bhutanese Himalaya   总被引：1，自引：0，他引：1  

Xu Peng  Yixin Chen  Gengnian Liu  Beibei Liu  Yingkui Li  Qing Liu  Yesong Han  Weilin Yang  Zhijiu Cui 《第四纪科学杂志》2019,34(1):40-50

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冀中饶阳凹陷西柳10断块古近系沙三段-沙二段层序地层及沉积演化          下载免费PDF全文

王旭旭  张廷山  张喜  孙文钊 《沉积与特提斯地质》2019,39(4):27-37

为了探讨饶阳凹陷蠡县斜坡北东缘西柳10断块古近系沙河街组沙三段-沙二段(Es~3-Es~2)层序地层特征及其沉积特征,依据高分辨率层序地层学理论,结合岩心、测井等资料,对研究区沙三段-沙二段层序地层进行划分,对其沉积特征、相带展布及其演化规律进行研究。研究结果表明,沙河街组沙三段-沙二段可划分为4个III级旋回,11个IV级旋回,32个V级旋回。沉积物岩性以细砂岩、粉砂岩及泥岩为主,沉积环境主要为辫状河三角洲平原和三角洲前缘,划分出7种沉积微相。结合研究区区域构造演化及沉积背景,认为沙三段-沙二段沉积时期,主要经历湖退到湖进的演变过程。  相似文献   

Meltwater discharge during the Holocene from the Wilkes subglacial basin revealed by beryllium isotope analysis of marine sediments     

Bethany Behrens  Yosuke Miyairi  Adam D. Sproson  Masako Yamane  Yusuke Yokoyama 《第四纪科学杂志》2019,34(8):603-608

Understanding Antarctic Ice Sheet dynamics related to global climate change is of scientific and societal interest as the future behaviour of the ice sheet under the currently changing climate is unknown. We present beryllium‐10 (¹⁰Be) analysis of a high‐resolution marine sediment core from the Adélie Basin near the eastern Wilkes Land margin, which is susceptible to marine ice sheet instability due to the low‐lying nature and down‐sloping trough of the Wilkes Subglacial Basin. Combined with a newly constructed age model using compound specific radiocarbon dates, the data reveal three events associated with high meteoric ¹⁰Be at ca. ~10 ka, ca. ~6.5 ka and from ca. ~4 ka. We interpret these high meteoric ¹⁰Be events to be derived from the deposition of ¹⁰Be released from the ice sheet during meltwater discharge. In particular, the shift to higher meteoric ¹⁰Be concentration at~4 ka may correspond to changes in climate patterns at this time. Copyright © 2019 John Wiley & Sons, Ltd.  相似文献   

Late Pleistocene climate of the northern Iberian Peninsula: New insights from palaeoglaciers at Fuentes Carrionas (Cantabrian Mountains)     

Ramn Pellitero  Jos M. Fernndez‐Fernndez  Nstor Campos  Enrique Serrano  Alfonso Pisabarro 《第四纪科学杂志》2019,34(4-5):342-354

New ¹⁰Be dates for glacial landforms in the Fuentes Carrionas area (Cantabrian Mountains, nothern Spain) are presented. Mapped and dated landforms in Fuentes Carrionas made possible a palaeoglacier reconstruction for four glacial stages. Results were compared to other nearby palaeoenvironmental proxies, so a final approximation on the mean annual temperature and annual precipitation that caused the four glacial advance stages is proposed. Glaciers reached their maximum extension at 36 ka, in a cold and dry environment. A second advance stage took place between 18.5 and 19.5 ka, during the Last Glacial Maximum (LGM), when glaciers advanced in a wet environment, with positive rainfall anomalies. A third glacial advance was dated during the Oldest Dryas, in which climate shifted to extremely cold and dry conditions. Finally, a last stage has been identified and proposed to the Younger Dryas, in which precipitation anomalies are negligible. Our results confirm some of the previously made palaeoglacial and palaeoenvironmental inferences for the Iberian Peninsula, as well as provide valuable and accurate anomalies, which are useful for climate modelling.  相似文献   

莫高窟PM10浓度与气象要素的关系     

杨小菊  赵学勇  武发思  张正模  薛平  陈章  汪万福  张国彬 《中国沙漠》2021,41(6):54-64

采用2018年敦煌莫高窟第16窟窟内与窟区PM₁₀浓度及气象数据,分析PM₁₀时空分布特征及其影响因素。结果表明：（1）两处监测点PM₁₀浓度主要分布在50 μg·m^-3以下,受重污染天气影响较小;春、冬、秋、夏季依次降低,窟区PM₁₀浓度在春、冬季高于窟内,夏、秋季反之。（2）PM₁₀浓度3月最高,9月最低,5—9月窟内月均值高于窟区。PM₁₀污染日数窟内5月最多,而窟区3、5月较多。（3）PM₁₀浓度日变化曲线在春季和秋季呈“双峰”型,夏季和冬季呈“单峰”型。（4）在半封闭环境的洞窟内,沙尘暴发生前后,PM₁₀浓度达到极值及恢复至原来水平的时间均滞后于窟区。（5）在不同季节PM₁₀浓度与气温、风速和降水呈负相关。除秋季外,PM₁₀浓度与相对湿度、气压呈正相关。（6）窟区全年主风向为ESE,在冬春两季,此风向PM₁₀浓度最高,PM₁₀主要来自三危山前的戈壁滩、干涸的大泉河河道以及窟前裸露的地表积尘。  相似文献   

内蒙古东部春季三类沙尘天气气溶胶散射系数及其与PM10、能见度相关性分析   总被引：3，自引：0，他引：3  

王天舒  牛生杰 《大气科学》2017,41(1):121-131

利用内蒙古东胜、锡林浩特两站2004~2006年春季（3~5月）积分浊度计的观测资料,结合同期PM10质量浓度、大气能见度等资料,分析了背景、扬沙、沙尘暴、强沙尘暴等不同强度沙尘天气气溶胶散射系数的分布特征,讨论了不同强度沙尘天气过程中散射系数、PM10、能见度的日变化规律,以及不同强度沙尘天气过程中散射系数与PM10质量浓度、散射系数与能见度的相关关系。结果表明:散射系数能够很好地反映沙尘天气强度;随沙尘天气强度增强,散射系数日变化从双峰型向单峰型转变;沙尘天气强度较弱时,PM10与散射系数的日变化不相似,强沙尘暴过程中PM10与散射系数的日变化有一定的相似性;能见度与散射系数日变化趋势相反;散射系数与PM10质量浓度呈正相关性,沙尘天气越强,相关性越好,背景、扬沙、沙尘暴、强沙尘暴相关系数分别为0.201、0.809、0.898和0.953;散射系数与能见度有指数相关关系,随沙尘天气强度增强二者相关性逐渐增强,背景、扬沙、沙尘暴、强沙尘暴相关系数分别为-0.773、-0.870、-0.918和-0.940。  相似文献   

基于MODIS数据中国天山积雪面积时空变化特征分析   总被引：1，自引：0，他引：1       下载免费PDF全文

何海迪  李忠勤  张明军 《干旱区地理》2018,41(2):367-374

基于2011-2015年MOD10A2积雪产品和气象数据,通过几何校正、去云预处理,应用归一化差分积雪指数算法等获取中国境内天山山区积雪覆盖面积数据,分析了积雪面积的时空变化特征及与气温降水的关系。结果表明：（1）年内积雪面积呈单峰变化,9月开始积累,次年1月达峰值,3月气温回暖消融加速,至7月最小。春秋季波动较大但没有明显的增减趋势,夏季积雪面积最小,冬季最大且呈减小趋势。（2）2001-2015年积雪覆盖面积整体上呈减少趋势,积雪覆盖率最大值的波动比最小值的波动更加剧烈。（3）积雪覆盖率随着海拔升高而增大,海拔<1 500 m区域积雪覆盖率低于10%,海拔>4 500 m以上区域平均可达70%,为常年稳定积雪区。积雪覆盖率在西北坡最高,南坡最低。（4）年均气温升高是积雪覆盖面积减小的主因,年积雪覆盖面积变化与年降水量变化保持一致的下降趋势。  相似文献