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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
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Transplant trials of the seagrass Posidonia australis were carried out after loss of seagrasses following eutrophication and increased turbidity in two marine inlets on the south coast of Western Australia. A pilot study in Oyster Harbour measured survival and growth in situ for 4 years. Long-term survival rates were high (96–98%), providing plants were anchored into the sediment. All unanchored plants were lost in the first winter. Following the success of the pilot study, a more comprehensive program began 3 years later with over 500 transplant units collected from either actively growing edges of nearby patches (plagiotropic growth form) or within established meadows (orthotropic growth form). Transplant units from edges expanded at a faster rate compared to units from mid-meadow but increases in shoot numbers were similar. Growth rates in the first 2.5 years averaged 10–20 cm yr−1 horizontal rhizome extension, depending on the source of the transplant units, and 4–12 shoots per initial shoot yr−1, depending on the initial shoot number of the transplant unit. After 5 years, shoot numbers of individual transplants were similar to shoot densities recorded for natural meadows, >500 shoots m−2. Approximately, 10% of transplants from mid-meadow flowered in the first year, whereas transplants from edges flowered only after 5 years. 相似文献
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Tao An Xiao-Yu Hong Wen-Xia Feng Jun-Hui Zhao Shanghai Astronomical Observatory Chinese Academy of Sciences Shanghai National Astronomical Observatories Chinese Academy of Sciences Beijing Harvard-Smithsonian Center for Astrophysics Garden Street MS Cambridge MA 《中国天文和天体物理学报》2004,4(6):527-532
We observed 1938-155, a broad line radio galaxy (BLRG), with the Very Large Array (VLA) at 90cm with an angular resolution of 6.8" × 4.0". The source consists of two components separated by 4 arcsec (- 20kpc, for H0 = 65km s-1 Mpc-1, q0 = 0.5) along the SE-NW direction. Both components show steep-spectra with a similar spectral index α - 0.83 ± 0.07 (Sv ∝ v-α). The bright double components are surrounded by a low-brightness cocoon. The radio properties of the two bright components are consistent with the hot spots produced by twin jets. An upper limit of - 0.0008 for the core dominance parameter (R) is inferred, suggesting there is no prominent radio core in the source. Assuming a modest viewing angle 30f77, a jet velocity is estimated - 0.07 c, based on the jet to counter-jet brightness ratio (J). The lower limit in jet speed inferred is consistent with no Doppler beaming effect on the jet. The radio galaxy 1938-155 could be an exceptional BLRG with no prominent radio core or jet. 相似文献
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Christopher A.Tout 《中国天文和天体物理学报》2007,(2)
Based on previous works of OPAL, we construct a series of opacity tables for various metallicities Z=0, 0.000 01, 0.000 03, 0.000 1, 0.000 3, 0.001, 0.004, 0.01, 0.02, 0.03, 0.04, 0.05, 0.06, 0.08 and 0.1. These tables can be easily used in Eggleton's stellar evolution code in place of the old tables without changing the code. The OPAL tables are used for log10(T/K) > 3.95 and Alexander's for log10(T/K) < 3.95. At log10(T/K) = 3.95, the two groups' data fit well for all hydrogen mass fractions. Conductive opacities are included by reciprocal addition according to the formulae of Yakovlev and Urpin. A comparison of 1 and 5 M models constructed with the older OPAL tables of Iglesias and Rogers shows that the new opacities have most effect in the late stages of evolution, the extension of the blue loop during helium burning for intermediate-mass and massive stars. 相似文献
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龙门山断裂构造带GPS研究 总被引：21，自引：10，他引：11
龙门山断裂构造带作为川青地块与扬子地块的碰撞边界，具有特殊的构造性质及明显的分段性。根据1991年以来GPS观测结果，对其分段活动性的研究表明：断裂带运动速率北段为1．54ram／a，中段为2．77mm／a，南段为5．23mm／a。现代构造活动性质总体表现为挤压走滑；同时，由北向南逐渐由挤压走滑转变为伸展走滑，其原因为在青藏高原总体运动条件下的相邻活动断裂的相互作用、相互影响。 相似文献
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青藏高原东缘鲜水河断裂与龙门山断裂交会区现今的构造活动 总被引：18，自引：1，他引：18
鲜水河断裂与龙门山断裂交会区具有特殊的构造性质。通过对交会区GPS观测,得到欧亚框架下运动速度场。利用所得的运动速度结果,采用刚性地块假设下的最小二乘法拟合方法,得到川滇、川青、扬子地块运动速度分别为(19.2±2.8)mm/a、(10.7±3.2)mm/a、(9.7±1.6)mm/a,地块运动方向由SE逐渐变成SEE,呈现出顺时针旋卷特征;鲜水河断裂运动速度为(9.3±2.8)mm/a,断裂性质为左旋走滑;龙门山断裂运动速度为(1.2±2.2)mm/a,断裂性质为右旋挤压。 相似文献
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