Associations of decimetric type Ⅲ bursts with coronal mass ejections and Hα flares     

Yuan Ma  De-Yu Wang  Jun Lin    Shuo Dai  Xue-Fei Zhang National Astronomical Observatories of China / Yunnan Astronomical Observatory  Chinese Academy of Sciences  Kunming  China Purple Mountain Observatory  Nanjing  China Harvard-Smithsonian Center for Astrophysics  Cambridge  MA  USA 《中国天文和天体物理学报》2010,10(5)

We present a statistical study of decimetric type Ⅲ radio bursts,coronal mass ejections(CMEs),and Hα flares observed in the period from July 2000 to March2005.In total,we investigated 395 decimetric type Ⅲ radio burst events,21% of which showed apparent correlation to CMEs that were associated with Hα flares.We noticed that the Hα flares which were strongly associated with CMEs were gradual events,and82% of them took place before CMEs appeared in the field of view of LASCO C2;that most of the CME-associated radio bursts started in the frequency range around750 MHz with a frequency drifting rate of several hundred MHz s-1,of which both positive and negative ones were recognized; and that the correlation of type Ⅲ radio bursts to CMEs without associated flares is fairly vague,less than 9%.  相似文献   

Why are halo coronal mass ejections faster?     

Qing-Min Zhang  Yang Guo  Peng-Fei Chen    Ming-De Ding  Cheng Fang 《中国天文和天体物理学报》2010,10(5)

Halo coronal mass ejections (CMEs) have been to be significantly faster than normal CMEs, which is a long-standing puzzle. In order to solve the puzzle, we first investigate the observed properties of 31 limb CMEs that clearly display loopshaped frontal loops. The observational results show a strong tendency that slower CMEs are weaker in white-light intensity. Then, we perform a Monte Carlo simulation of 20000 artificial limb CMEs that have an average velocity of ～523km s -1. The Thomson scattering of thes...  相似文献   

Infrared spectral evolution of carbon stars     

Pei-Sheng Chen  Xiao-Hong Yang  Hong-Guang Shan National Astronomical Observatories /Yunnan Observatory  Key Laboratory for the Structure  Evolution of Celestial Objects  Chinese Academy of Sciences  Kunming  China 《中国天文和天体物理学报》2010,10(4)

We collected almost all Highly Processed Data Products(HPDP)of ISO SWS01 spectra for the Galactic visual carbon stars,infrared carbon stars,extreme carbon stars and carbon-rich proto-planetary nebulae(PPNs).Those infrared spectra are primarily analyzed and discussed.It is shown that either spectral shapes/peaks,or main molecular/dust features are evidenced to change in the sequence of visual carbon stars,infrared carbon stars,extreme carbon stars and carbon-rich PPNs.Statistically,in this sequence,continua are gradually changed from blue to red and locations of spectral peaks of continua are also gradually changed from short wavelengths to long wavelengths.In addition,in this sequence,intensifies of main molecular/dust features are also gradually changed from prominent in the short wavelengths to prominent in the long wavelengths.Furthermore,from 2MASS and IRAS photometric data,the sequence is also proved.Results in this paper strongly support the previous suggestion for the evolution sequence of carbon-rich objects in our Galaxy,that is the sequence of visual carbon stars→infrared carbon stars→extreme carbon stars→carbon-rich PPNs.  相似文献   

Search for periodicities of the solar irradiance data from the Earth Radiation Budget Satellite (ERBS) using the periodogram method     

Sankar Narayan Patra  Gautam Bhattacharya  Koushik Ghosh 《中国天文和天体物理学报》2010,10(4)

We have analyzed the solar irradiance data from the Earth Radiation Budget Satellite(ERBS)during the time period from 1984 October 15 to 2003 October 15.By first filtering the data by Simple Exponential Smoothing,we have applied the periodogram method to the processed data in order to search for its time variation.The study exhibits multi-periodicities on these data around 110,118,574 and 740d with very high confidence levels(more than 99%).These periods are significantly similar to the periods of other solar activities which may suggest that solar irradiance may be associated with other solar activities.  相似文献   

High-contrast coronagraph for ground-based imaging of Jupiter-like planets     

Jiang-Pei Dou    De-Qing Ren    Yong-Tian Zhu  National Astronomical Observatories / Nanjing Institute of Astronomical Optics & Technology  Chinese Academy of Sciences  Nanjing  China  Key Laboratory of Astronomical Optics & Technology  Nanjing Institute of Astronomical Optics & Technology  China Physics & Astronomy Department  California State University Northridge  Nordhoff Street  Northridge  California – 《中国天文和天体物理学报》2010,10(2)

We propose a high-contrast coronagraph for direct imaging of young Jupiter-like planets orbiting nearby bright stars. The coronagraph employs a steptransmission filter in which the intensity is apodized with a finite number of steps with identical transmission in each step. It should be installed on a large ground-based telescope equipped with a state-of-the-art adaptive optics system. In this case, contrast ratios around 10-6 should be accessible within 0.1 arcsec of the central star. In recent progress, a...  相似文献   

Bianchi type-I cosmological models with perfect fluid in general relativity     

Rishi Kumar Tiwari 《中国天文和天体物理学报》2010,10(4)

Einstein's field equations with variable gravitational and cosmological constants are considered in the presence of perfect fluid for the Bianchi type-Ⅰ universe by assuming that the cosmological term is proportional to R-m(R is a scale factor and m is a constant).A variety of solutions are presented.The physical significance of the respective cosmological models are also discussed.  相似文献   

杭州地区大气水分特征及相关问题的初步探讨     

张玉娟 《气象科技》2007,35(1):61-65

用1951年1月至2003年12月NCEP/NCAR再分析格点比湿、垂直速度资料,以及杭州站降水量资料,分析了杭州地区对流层整层可降水量、低层空气垂直上升运动强度以及地面降水量的演变特点。结果发现,可降水量与低层空气垂直上升运动具有显著的年代际变化,且这两者均利于降水的时段,降水量不一定偏多,这说明空中水资源具有很大的开发空间。对杭州6月大气可降水量的长期变化特征与全球同纬度地区作了对比,发现近53年来,杭州地区6月份降水量处于下降趋势。  相似文献   

沈阳长白乡-观音阁断裂、抚顺浑河断裂的定位和活动性研究   总被引：3，自引：0，他引：3  

雷清清  王超  赵晓辉  曲乐 《震灾防御技术》2007,2(2):128-136

本文基于对沈阳长白乡-观音阁断裂,以及抚顺浑河断裂开展的1:10000地质地貌填图工作,获得了这两条断裂在最老第四纪地层热释光的测年结果,它们分别为(112±6.7)ka和(150±9.0)ka。长白乡-观音阁断裂为一沿丘陵山地前缘分布的断裂,由2—3条分支断裂组成,最新的断面活动显示为压扭性正断层性质。断裂在晚更新世坡洪积扇堆积形成以来没有活动显示。3条浅层人工地震测线探测结果表明,其上断点均未错断第四系上更新统底界。断裂为中更新世活动断裂,晚更新世以来没有活动。浑河断裂为一沿丘陵山地前缘分布的断裂,由3—4条分支断裂组成,最新的断面活动显示为压扭性正断层性质。断裂在晚更新世坡洪积扇堆积形成以来没有活动显示。5条浅层人工地震测线探测结果表明,其上断点均在第四系上更新统底界以下。断裂为中更新世活动断裂,晚更新世以来没有活动。  相似文献   

加强土地整理工作 促进农村经济发展     

李岩晖 《山西地质》2010,(3):14-16

通过对曲沃县汾河滩土地开发整理项目的调查与研究,并对项目完成情况进行评价,得出土地整理项目利国利民,受到农民热烈欢迎的结论。  相似文献   

洮河泥沙分布及变化分析     

凡炳文  陈文  李计生 《地下水》2010,32(3):118-120,123

以洮河红旗站1956~2005年水文监测资料为依据,通过对泥沙分布特征、年内年际变化规律和水沙匹配情况进行分析,得出洮河泥沙具有含量高、输沙总量大、产沙的区域性、年际的波动性、年内的不均匀性和时间的集中性六大特点。  相似文献