1997年3月9日漠河日全食外日冕结构及相对强度分布     

李秋莎  张柏荣 《天文研究与技术》2000,(2):11

利用简单的视频图像采集系统 ,对 1 997年 3月 9日用PanasonicNV -S880EN型摄像机拍摄的黑龙江漠河日全食黄光 (加GG1 1滤光片 )和白光日冕观测资料进行计算处理 ,得到大于 1 .5R⊙ 的太阳活动低年外日冕结构及其相对强度分布。  相似文献   

Ionospheric measurements of relative coronal brightness during the total solar eclipses of 11 August, 1999 and 9 July, 1945     

C. J. Davis  M. Lockwood  S. A. Bell  J. A. Smith  E. M. Clarke 《Annales Geophysicae》2000,18(2):182-190

Swept-frequency (1/10 MHz) ionosonde measurements were made at Helston, Cornwall (50°06N, 5°18W) during the total solar eclipse on August 11, 1999. Soundings were made every three minutes. We present a method for estimating the percentage of the ionising solar radiation which remains unobscured at any time during the eclipse by comparing the variation of the ionospheric E-layer with the behaviour of the layer during a control day. Application to the ionosonde date for 11 August, 1999, shows that the flux of solar ionising radiation fell to a minimum of 25±2% of the value before and after the eclipse. For comparison, the same technique was also applied to measurements made during the total solar eclipse of 9 July, 1945, at Sörmjöle (63°68N, 20°20E) and yielded a corresponding minimum of 16 ± 2%. Therefore the method can detect variations in the fraction of solar emissions that originate from the unobscured corona and chromosphere. We discuss the differences between these two eclipses in terms of the nature of the eclipse, short-term fluctuations, the sunspot cycle and the recently-discovered long-term change in the coronal magnetic field.  相似文献   

Conceptual problems with remote element synthesis     

O. K. Manuel 《Journal of Earth System Science》2000,109(1):195-203

The notion of remote element synthesis has recently been modified to explain the presence of nucleogenetic isotopic anomalies and decay products of short-lived nuclides by injection of a small amount ofexotic nucleogenetic material. Even with this modification, remote element synthesis seems inconsistent with the following observations:

–	Evidence of coupled variations in the chemical and isotopic compositions of the source material for meteorites.
–	Residual coupling of chemical and isotopic heterogeneities across planetary distances in the solar system today.
–	The mass-fractionation relationship seen across isotopes of elements in the planetary system, in the solar wind, and in solar flares.
–	Linkage of short-lived radioactivities with isotopic anomalies and with physical properties of their host grains, as expected for early condensate of fresh stellar debris.
–	Temporal and spatial distributions of short-live nuclides and their decay products.
–	Mirror-image (+ and −) isotopic anomalies in meteorite grains that sum to “normal” isotopic ratios, as expected of unmixed products of the same nuclear reactions that produced our bulk elements.
–	The lac supporting evidence for “presolar” grains or nearby stars that injectedexotic material into the early solar nebula.

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节气气候变化与上消化道出血的关系研究     

吴荣娟  邱赠东林平 《广西气象》2007,28(3):47-49

通过对2000-2005年龙岩市第一医院上消化道出血（UGB）患者入院时的节气归属及当时气象资料的收集,分析不同节气气候变化与UGB的关系,运用最优子集回归方法建立关系模式进行综合分析,得出影响上消化道出血发病趋势的关键气象要素是节气最高气温、最低气温、平均水汽压;通过节气气候因素对UGB影响的认识,提出相应的预防保健措施。  相似文献   

昌吉市太阳总辐射的气候学计算及其变化特征分析     

阿帕尔  叶尔克江 《沙漠与绿洲气象(新疆气象)》2007,1(2):36-39

利用昌吉市1961—1997年的逐日气候资料,对昌吉市1961—1997年多年平均逐日太阳总辐射进行了气候学计算,并分析了其变化特征和变化趋势,结果表明:昌吉市太阳总辐射多年平均年日总量为22.82MJ.m-2.d-1,太阳总辐射在8～9月份最高,12月份最低,昌吉市的太阳总辐射呈逐年下降趋势。  相似文献   

On the Dynamics of Dust Grains in a Hierarchical Environment     

Marcos  C. De La Fuente  Marcos  R. De La Fuente 《Earth, Moon, and Planets》1998,81(2):145-173

Most main sequence stars are binaries or higher multiplicity Systems and it appears that at birth most stars have circumstellar disks. It is commonly accepted that planetary systems arise from the material of these disks; consequently, binary and multiple systems may have a main role in planet formation. In this paper, we study the stage of planetary formation during which the particulate material is still dispersed as centimetre-to-metre sized primordial aggregates. We investigate the response of the particles, in a protoplanetary disk with radius R_D = 100 AU around a solar-like star, to the gravitational field of bound perturbing companions in a moderately wide (300–1600 AU) orbit. For this purpose, we have carried out a series of simulations of coplanar hierarchical configurations using a direct integration code that models gravitational and viscous forces. The massive protoplanetary disk is around one of the components of the binary. The evolution in time of the dust sub-disk depends mainly on the nature (prograde or retrograde) of the relative revolution of the stellar companion, and on the temperature and mass of the circumstellar disk. Our results show that for binary companions near the limit of tidal truncation of the disk, the perturbation leads to an enhanced accretion rate onto the primary, decreasing the lifetime of the particles in the protoplanetary disk with respect to the case of a single star. As a consequence of an enhanced accretion rate the mass of the disk decreases faster, which leads to a longer resultant lifetime for particles in the disk. On the other hand, binary companions may induce tidal arms in the dust phase of protoplanetary disks. Spiral perturbations with m = 1 may increase in a factor 10 or more the dust surface density in the neighbourhood of the arm, facilitating the growth of the particles. Moreover, in a massive disk (0.01M⊙) the survival time of particles is significantly shorter than in a less massive nebula (0.001M⊙) and the temperature of the disk severely influences the spiral-in time of particles. The rapid evolution of the dust component found in post T Tauri stars can be explained as a result of their binary nature. Binarity may also influence the evolution of circumpulsar disks. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

太阳常数的变化与太阳软x射线辐射流量及低频天波时延的关系   总被引：1，自引：0，他引：1  

王素琴  潘炼德 《时间频率学报》1998,21(1):49-53

本文对1982年在陕西临潼接收的美国罗兰-C西北大平洋链Y台发射的100kHz低频一跳天波时延的实测资料及SMS－GOES测量的太阳1～8A软x射线的每日辐射流量与SMM／ACRIMI测量的太阳常数之间的关系进行了分析。结果表明：太阳1～8A软x射线辐射流量与太阳常数之间存在较强的负相关;低频一跳天波时延与太阳常数之间存在着较强的正相关。并对此进行了讨论。  相似文献   

Fine structure of the red giant clump from Hipparcos data, and distance determinations based on its mean magnitude     

Léo Girardi  Martin A. T. Groenewegen  Achim Weiss  & Maurizio Salaris 《Monthly notices of the Royal Astronomical Society》1998,301(1):149-160

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Investigations of the effects of manganese addition to Dry Creek Saltfield brines     

Peri S.J. Coleman 《International Journal of Salt Lake Research》1998,7(1):25-40

Trials conducted at Dry Creek, a solar saltfield north of Adelaide, Australia, indicate that manganese, as manganous sulphate, can increase both the purity and strength of salt crystals grown at an ambient or neutral-slightly acid pH range resulting in a salt suitable for high purity uses. The improved load bearing strength of the crystals indicates that manganous sulphate could also be useful in salt floor maintenance. However, the impact of an apparently slight rise in pH to 8.5 was significant. Crystals produced at the higher pH from the manganese enriched brine were opaque with many tiny, almost colloidal crystals. The salt did not drain well, had low load bearing strength and was notably impure.  相似文献   

基于地理信息系统的太阳直接辐射与冰川物质平衡的关系   总被引：4，自引：1，他引：3  

丁永建 《冰川冻土》1998,20(2):157-162

基于冰川微地形对冰川物质平衡重要影响的认识,在考虑朝向、坡度、地形遮蔽等因素的条件下,以地理信息系统为手段,对乌鲁木齐河源１号冰川冰面太阳可能直接辐射进行了理论计算．在此基础上,建立了计算冰面任意一点物质平衡的Ｂ＝ｆ（Ｔ,Ｒ）（气温－辐射）模型．比较了该模型与Ｂ＝ｆ（Ｔ）（气温）模型、Ｂ＝ｆ（Ｐ,Ｔ）（降水－气温）模型及Ｂ＝ｆ（Ｑ）（能量平衡）模型之间的优缺点,表明该模型具有物理意义明确、计算精度较高、参数易于获得等优点,从而为计算冰川物质平衡提供了新的途径．  相似文献