肇源新型自动土壤水分观测仪与人工平行观测资料对比分析     

罗贯宇  王继梅 《黑龙江气象》2014,31(3):42-43

采用对比差值、差值概率等方法对肇源2012年5月3日-11月13日期间GStar DZN2型自动土壤水分观测仪与人工平行对比观测的土壤湿度资料进行统计。结果表明,人工与自动观测资料的一致性在20和40 cm土层表现最好,60 cm土层表现最差,总体上人工观测值高于自动观测值。  相似文献   

色球耀斑Hα谱线轮廓不对称性研究     

于晓霞  甘为群 《天文学报》2006,47(1):54-62

Hα谱线轮廓的不对称性是色球耀斑光谱观测中的重要特征,也是耀斑动力学过程的重要观测事实之一．以紫金山天文台太阳光谱仪的观测资料为依据,给出Hα谱线不对称性的典型轮廓．在考虑氢原子非热激发、电离的作用下,经验性地计算了不同大气模型下谱线的不对称性特征,并在此基础上,对观测谱线进行半经验的研究．结果表明, 色球区的向下运动能够产生Hα谱线的红、蓝不对称性,并可以再生具体耀斑的谱线不对称性特征．此外,不仅非热粒子的能流、谱指数大小以及速度场所处的高度对谱线轮廓有影响,耀斑大气的背景模型对谱线的轮廓也有一定的影响．  相似文献   

Relation between the “Double-Hump” Behavior in the Radio Band and the Broad-Line Luminosity for Blazars     

Zhao-Hua Xie  Hong Dai    Jian-Ming Hao  Lei-Ming Du  Xiong Zhang Physics Department  Yunnan Normal University  Kunming  Yunnan Astrophysics Center  Yunnan University  Kunming Graduate School of Chinese Academy of Sciences  Beijing 《中国天文和天体物理学报》2007,(2)

The physics behind the spectral energy distribution (SED) of blazars remains open. We assembled 36 blazars to tackle the factors that control their SED. Now, many blazar spec- tra have the "double hump" feature in the radio and far-IR frequencies. For these a parameter, , is created to characterize the behavior of the SED. We found a significant correlation be- tween the broad-line luminosity (LBLR) and . Because LBLR is an indicator of the accreting power of the source in blazars, we derived a linear correlation, ∝ M˙1/3.18, which suggests that the SED of blazars may depend on the accretion rate, like that of BL Lac objects. We also found a significant correlation between ■ and for a sample of 11 blazars (out of one of 36) with available black hole masses. This implies the Eddington accretion ratio may influence the shape of the SED of blazars.  相似文献   

考虑LS+AR模型基础数据量的极移预报研究          下载免费PDF全文

徐海龙  乔书波  王穆阳 《天文学报》2022,63(2):14

针对目前极移最小二乘(Least Square, LS)+自回归(AutoRegressive, AR)预报模型的单一数据选取方案, 提出分别考虑LS模型数据量和AR残差数据量的组合数据模式, 并对极移预报时单一数据和组合数据预报结果精度进行分析, 探讨模型输入数据量对极移预报精度的影响. 结果表明, 模型输入数据量的变化对极移预报结果影响较大. 采用组合数据预报的方式相比较于单一数据量预报方式精度更高, 特别是针对30--360 d跨度内的中长期预报, 组合数据量的极移预报精度可比单一数据量预报精度有较大改善. 结论证明组合数据在极移预报时具有一定的优势, 可为以后极移预报数据量选取提供一定的借鉴参考意义.  相似文献   

太阳运动Ⅳ型射电爆发的相干辐射模型     

王德焴 《天文学报》2004,45(2)

为解释太阳运动Ⅳ型射电爆发的相干辐射机制提出一个理论模型.从耀斑中产生的高能电子,可以被扩展上升的太阳磁流管俘获.在磁流管顶部,这些高能电子的速度分布形成为类束流速度分布,激发柬流等离子体的不稳定性,并且主要直接放大O模电磁波.不稳定性增长率敏锐地依赖了日冕等离子体参数fpe/fce和射束温度Tb,这能定性解释在太阳运动Ⅳ型射电爆发中观测到的高亮温度和高偏振度,以及宽频谱的特性.  相似文献   

A Possible 456-Day Optical Period of OQ 530     

Yi Liu Juan Li Jun-Hui Fan 《中国天文和天体物理学报》2007,7(3):380-388

The post-1994observationsof the blazar OQ 530 in optical BV RI bands, and radio observations at 22GHz and 37GHz were collected. The date compensated discrete Fourier transform (DCDFT) and CLEANest methods were used to search for possible periodicities. Two possible periods of 456±100 days and 258±29 days were found in the optical bands. The existence of possible correlations between the optical and radio emissions was investigated by means of discrete correlation function (DCF) analysis, and no significant correlation was found. Some possible mechanisms for the periodic variability are discussed.  相似文献   

峨边彝族自治县沙坪镇羊竹坝崩塌地质环境条件及危石稳定性评价     

《四川地质学报》2022,(Z2):51-54

勘查区位于大渡河右岸近河床斜坡地带,属构造剥蚀及河流侵蚀低山地貌。通过对沙坪镇羊竹坝崩塌地质环境条件的研究,同时对该区危石稳定性进行了评价,认为区内地质灾害的类型主要为危石崩塌。危石区(单体)在持续降雨或地震的情况下多处于欠稳定状态,产生失稳破坏的可能性大。因此对工作区进行治理十分必要。  相似文献   

鄂尔多斯盆地西南部上古生界储层裂缝研究     

王倩  候玢池  张琦 《地下水》2015,(2)

裂缝的发育不仅可以提高基质渗透率,增大油气产量,而且可能成为油气二次运移的主要通道,因此定量评价储层(尤其是致密砂岩储层)的裂缝频率、发育规模和空间分布是十分必要的,通过岩心观察、薄片分析及测井资料解释等表明,研究区盒8、山1、山2段裂缝较为发育,以水平裂缝和高角度近垂直裂缝为主;约90%的裂缝为有效裂缝,显示气层或干层;约30%的裂缝产出层段为气层和含气层,可见宏观裂缝的发育为油气富集提供了良好的运移通道。成像测井显示,研究区微裂缝发育也较为广泛,以垂直裂缝为主,为天然气向上运移提供了通道。  相似文献   

EGUP与黑洞熵的修正值     

白吉龙  温廷敦 《天文学报》2015,56(1):1-6

目前,人们对黑洞Bekenstein-Hawking熵的量子修正值产生了极大的兴趣,尤其是黑洞熵对数修正项的系数.在广义不确定关系(GUP)的基础上,通过引入了推广的广义不确定关系(EGUP),运用面积定理计算了3类时空的黑洞熵的修正值,得到的黑洞熵的修正项的系数是正的.这种计算方法不仅对单视界时空适用,而且对有内视界的黑洞时空依然成立,并且在EGUP基础上计算出黑洞熵的修正值.相比GUP基础上得到的黑洞熵,EGUP可以应用于大尺度时空下,所以应用范围更广.此计算方法简洁明了,物理意义明确,可为黑洞熵对数修正值系数的确定提供参考.  相似文献   

Structure and evolution of magnetic fields associated with solar eruptions     

Haimin Wang  Chang Liu 《天文和天体物理学研究(英文版)》2015,(2):145-174

This paper reviews the studies of solar photospheric magnetic field evolution in active regions and its relationship to solar flares. It is divided into two topics, the magnetic structure and evolution leading to solar eruptions and rapid changes in the photospheric magnetic field associated with eruptions. For the first topic, we describe the magnetic complexity, new flux emergence, flux cancelation, shear motions, sunspot rotation and magnetic helicity injection, which may all contribute to the storage and buildup of energy that trigger solar eruptions. For the second topic, we concentrate on the observations of rapid and irreversible changes of the photospheric magnetic field associated with flares, and the implication on the restructuring of the three-dimensional magnetic field. In particular, we emphasize the recent advances in observations of the photospheric magnetic field, as state-of-the-art observing facilities(such as Hinode and Solar Dynamics Observatory) have become available. The linkages between observations, theories and future prospectives in this research area are also discussed.  相似文献