太阳光球磁通量南北不对称性研究     

宋文彬  汪景琇  马霞 《天文学报》2005,46(1):19-26

运用统计方法系统研究了1978-2002年太阳光球磁通量南北不对称性变化特征，发现其与太阳活动周有关．不对称值在太阳活动极小年要明显高于太阳活动极大年，并且磁通量变化总是由上升段的北半球占优逐渐过渡到下降段的南半球占优．另外运用小波变换方法详细讨论了这种不对称性变化可能存在的周期信息．  相似文献   

CO2 output and δ13C(CO2) from Mount Etna as indicators of degassing of shallow asthenosphere     

W. D'Alessandro  S. Giammanco  F. Parello  M. Valenza 《Bulletin of Volcanology》1997,58(6):455-458

 An estimated average CO₂ output from Etna's summit craters in the range of 13±3 Mt/a has recently been determined from the measured SO₂ output and measured CO₂/SO₂ molar ratios. To this amount the CO₂ output emitted diffusely from the soil (≈ 1 Mt/a) and the amount of CO₂ dissolved in Etna's aquifers (≈ 0.25 Mt/a) must be added. Data on the solubility of CO₂ in Etnean magmas at high temperature and pressure allow the volume of magma involved in the release of such an amount of this gas to be estimated. This volume of magma (≈ 0.7 km³/a) is approximately 20 times greater than the volume of magma erupted annually during the period 1971–1995. On the basis of C-isotopic data of CO₂ collected in the Etna area and of new hypotheses on the source of Mediterranean magmas, significant contributions of CO₂ from non-magmatic sources to the total output from Etna are unlikely. Such large outputs of CO₂ and also of SO₂ from Etna could be due to an anomalously shallow asthenosphere beneath the volcano that allows a continuous escape of gases toward the surface, even without migration of magma. Received: 7 August 1996 / Accepted: 9 November 1996  相似文献   

利用重复重力观测资料研究地震活动与地壳的损伤演化过程     

张永志  朱桂芝  祝意青 《大地测量与地球动力学》2001,21(3):14-20

利用细观损伤力学模型建立了地壳损伤演化过程与地球重力场变化的关系 ,讨论了利用重力观测资料计算地壳微裂纹密度参数变化分布的理论与计算方法。利用河西地区 1992～ 1999年多期重复重力观测资料对该地区的裂纹密度参数变化进行了计算 ,并将计算结果与该地区的各观测时间段内相应发生的一级以上地震活动进行了对比分析 ,取得了一些有意义的结论和认识。  相似文献   

Formation of current helicity and emerging magnetic flux in solar active regions   总被引：1，自引：0，他引：1  

Hongqi Zhang 《Monthly notices of the Royal Astronomical Society》2001,326(1):57-66

We present the results of a photometric study of X-ray-active weak-lined T Tauri (WTT) stars in the η Chamaeleontis star cluster. Multi-epoch V -band photometric monitoring during 1999 and 2000 of the 10 X-ray-active WTT stars found that all were variable in one or both years, with periods ascribed to rotational modulation of starspots. Comparison between the rotational and X-ray properties of these objects indicates the saturation level,     observed in other studies of X-ray-active pre-main-sequence stars, persists in the η Cha stars from the slow- to the fast-rotator regimes. Cousins VRI photometry of the WTT stars has enabled us to investigate further the photometric properties of these stars. The stars appear sufficiently coeval to distinguish near-equal-mass binaries within the sample. A new Hertzsprung–Russell diagram for these objects suggests ages of 4–9 Myr for M-type RECX primaries using the tracks of D'Antona & Mazzitelli.  相似文献   

特定折扣率的二度价格歧视研究     

方国敏 《成都信息工程学院学报》2008,23(4):460-463

研究基于垄断厂商收益最大化的特定折扣率的定价问题,给出解的具体表达式,同时解决原有文献中需求函数为非线性函数时,最优固定折扣率的解的问题。  相似文献   

Rotation periods for stars of the TW Hydrae association: the evidence for two spatially and rotationally distinct pre-main-sequence populations     

Warrick A. Lawson  Lisa A. Crause 《Monthly notices of the Royal Astronomical Society》2005,357(4):1399-1406

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Testing solar forcing of pervasive Holocene climate cycles     

Chris Turney  Mike Baillie  Steve Clemens  David Brown  Jonathan Palmer  Jonathan Pilcher  Paula Reimer  Hanns Hubert Leuschner 《第四纪科学杂志》2005,20(6):511-518

The temporal and spatial extent of Holocene climate change is an area of considerable uncertainty, with solar forcing recently proposed to be the origin of cycles identified in the North Atlantic region. To address these issues we have developed an annually resolved record of changes in Irish bog tree populations over the last 7468 years which, together with radiocarbon‐dated bog and lake‐edge populations, extend the dataset back to ～9000 yr ago. The Irish trees underpin the internationally accepted radiocarbon calibration curve, used to derive a proxy of solar activity, and allow us to test solar forcing of Holocene climate change. Tree populations and age structures provide unambiguous evidence of major shifts in Holocene surface moisture, with a dominant cyclicity of 800 yr, similar to marine cycles in the North Atlantic, indicating significant changes in the latitude and intensity of zonal atmospheric circulation across the region. The cycles, however, are not coherent with changes in solar activity (both being on the same absolute timescale), indicating that Holocene North Atlantic climate variability at the millennial and centennial scale is not driven by a linear response to changes in solar activity. Copyright © 2005 John Wiley & Sons, Ltd.  相似文献   

The effects of temperature and substrate on ontogenetic behavior of bastard halibut, Paralichthys olivaceus (T. et S.)     

刘栋  线薇薇  朱鑫华 《中国海洋湖沼学报》2005,23(1)

1 INTRODUCTION Scientific management of aquacultural andnatural populations studies on the early life historyof flatfishes in the aspects of their metamorphosisand benthic settlement accompanying pronouncedtransitions in morphology, behavior and habitatecology have received much attention (Youson,1988). Accumulated data showed that temperatureand substrate played a main role in the recruitmentsuccess of flatfish during their early development(Rijnsdorp et al., 1995, Gibson and Robb, 2000…  相似文献   

How Fast the Nucleus of Comet Hale–Bopp was Rotating?     

Shulman  L. M.  Kidger  M.  Serrat-Ricart  M.  Torres-Chico  R. 《Earth, Moon, and Planets》2002,90(1-4):109-117

At the First International Conference on Comet Hale–Bopp(Canaries, 1998) many astronomers agreed with the value of theperiod of axial rotation of its nucleus, which was obtained byobservers by a comparison of the two sequential patterns of thedust arcs. It was noted that the pattern had been repeated each∼12 hours. The value 11.35^h was taken as the periodof axial rotation. However, alternative periods of 4 and 8 days havealso been suggested. The possible reasons for thisdiscrepancy are discussed. It is shown that a short period could be obtained by a misidentification of the same arc on twosequential images and, as a result, an overestimate of theradial velocity of dust in the arcs. To obtain the half day period one must take the projected velocity of the arc ∼ 1.6 km/s,which exceeds the H₂O gas expansion velocity. If one takes a lower expansion velocity a longer period would be obtained.  相似文献   

海南岛近海海域7个沉积岩芯的现代沉积速率及其分布特征   总被引：4，自引：0，他引：4  

许冬  龙江平  钱江初  席鹏 《海洋学研究》2008,26(3):9-17

利用多道α能谱仪,对2005年8～9月在海南岛近海采集的7个沉积岩芯进行了210Pb的沉积速率测定,探讨了海南岛近海陆架上现代沉积速率的区域性分布特征,结果表明:位于港湾内的B1168站位由于沉积物供应充足,有最高的沉积速率,达2.9 cm/a;位于河口海湾附近且受沿岸流影响的B289站位,有很高的沉积速率,可达1.6 cm/a,沉积环境较稳定;位于西南海底沙脊区北缘且靠近昌化江河口的B97、B135、B10站位也有较高沉积速率,分别达到1.0、0.89和0.47 cm/a,在表层都出现了210Pb放射性活度倒置的现象,表明所处区域有较强混合作用;处于西南外陆架的C4站位受北部湾环流影响,沉积速率为0.6 cm/a;位于东部外陆架的B377站位处于上升流区,沉积速率较低,为0.21 cm/a.可见,海南岛近海陆架上的现代沉积速率存在着明显的区域分布:在物质来源丰富的沿岸流作用区和河口区附近,现代沉积速率很高;在陆架环流沉积作用区,现代沉积速率也较高;在水深较大的外陆架上,由于沉积物供应相对匮乏,沉积速率一般较低;在近岸潮流沙脊区,由于水动力很强,无法形成现代细粒沉积.同时,在陆架上,沉积速率有随着水深的增加而降低的趋势.由此可见,海南岛近海海域的沉积速率与该区的物质供应、水动力条件和海底地形等因素有密切关系.  相似文献