面向单脉冲信号分类的集成特征选择与评价

受大量射频干扰信号影响, 快速从海量观测数据中准确识别出单脉冲信号已成为天文数据处理的一项重要任务, 而设计和提取有效数据特征, 是利用机器学习进行单脉冲信号高效识别的决定因素. 针对如何选择最优特征, 进而提升单脉冲信号的分类精度这一关键问题, 设计了面向单脉冲信号分类的集成特征选择方法. 方法首先混合单脉冲信号的参数特征、统计特征和抽象特征, 然后分别利用5种单一特征选择方法选出各自的最优特征集, 最后利用贪心策略对5种单一方法获取的最优特征集进行集成筛选, 获取最优集成特征集. 实验表明, 最优特征集合既包含统计特征也包含抽象特征. 在相同特征数量下, 利用集成特征选择比单一特征选择能获得更高的模型精度, 可使F1值最高提升1.8%. 在海量数据背景下, 集成特征选择对减少特征数量、提升分类性能和加快数据处理速度具有重要作用.     

Impacts of a bottom trawling exclusion zone on Snow Crab abundance and fish harvester behavior in the Labrador Sea, Canada

The Hawke Box trawling exclusion zone off southern Labrador is a 8610 km² closed area implemented in 2003 to protect soft-shelled pre-recruit Snow Crab and juvenile cod from mortality imposed by shrimp trawling and other bottom-impact fisheries. This study utilizes survey, logbook, and observer data from the Snow Crab and Northern Shrimp fisheries to assess the effectiveness of the Hawke Box in protecting and possibly enhancing the Snow Crab resource off southern Labrador. The results indicate that the exclusion zone has failed to protect pre-recruit crabs largely due to a redistribution and intensification of directed Snow Crab effort inside the Box in the years following closure. This unexpected outcome resulted in a high level of fishery-induced mortality to pre-recruit crabs and masked any potential positive outcomes from the cessation of trawling. The shortcomings that contributed to the failure of this exclusion area are discussed in relation to the current state of knowledge on the effectiveness of marine protected areas in general as management tools for conserving aquatic resources.     

东海蟹类群落结构特征的研究

依据1998年5月(春季)、8月(夏季)、11月(秋季)和1999年2月(冬季)在东海26°00′—33°00′N、127°00′E以西海域的蟹类资源调查资料,对东海蟹类群落结构的特征进行了定量分析。结果表明,东海蟹类优势种有双斑、银光梭子蟹、细点圆趾蟹、长手隆背蟹、日本、武士、锈斑、三疣梭子蟹、泥脚隆背蟹、锐刺长蟹和纤手梭子蟹。其中银光梭子蟹、细点圆趾蟹、双斑和三疣梭子蟹是东海蟹类的主要优势种。常见种是艾氏牛角蟹、红星梭子蟹、绵蟹、变态、光掌、十一刺栗壳蟹、七刺栗壳蟹、象牙长螯蟹、卷折馒头蟹、直额、武装筐形蟹和显著琼娜蟹。种类组成特征方面,冬、春季蟹类少数优势种的优势性明显,秋季优势度种间差异不明显。种类数比较:东海南部最多(57种),中部次之(45种),北部最少(仅37种);不同季节间,春季最多(57种),其次是夏季(53种),秋、冬季较少(仅49种);水深越深的水域,种类数越多。多样性比较:冬、春、秋3季,从北到南,蟹类多样性逐渐增高,且随着水深加深而增大;夏季不同,水深小于40m的浅海多样性指数最高。东海蟹类共可分为3个生态类群,即广温广盐生态类群、高温广盐生态类群和高温高盐生态类群。     

对虾白斑综合症病毒病围栏封闭预防技术研究简报

病毒性流行病使世界的养虾业遭受到了严重挫折 ,其中又以白斑综合症病毒 (ＷＳＳＶ)病流行最广 ,危害最大。针对这种病的病原、病理和流行病学已进行了大量的研究 ,对于如何预防也做了很多探索 ,但迄今没有得到很好的解决。养虾界总结出高位池塘养殖、内地淡化养殖、远海岸卤水、井水或渗水养殖和虾池配养肉食性鱼类等办法 ,都有一定的效果。但这些办法大多要求一定的条件 ,缺乏普适性 ,而且往往有时效限制 (即养殖年久后也会发病 ) ;有的则只是减小了发病机率 ,并不是十分可靠 (如配养肉食性鱼类 )。因此 ,研制出一种具有普适性 (特别是能…     

The major upgrade of the MAGIC telescopes,Part II: A performance study using observations of the Crab Nebula

MAGIC is a system of two Imaging Atmospheric Cherenkov Telescopes located in the Canary island of La Palma, Spain. During summer 2011 and 2012 it underwent a series of upgrades, involving the exchange of the MAGIC-I camera and its trigger system, as well as the upgrade of the readout system of both telescopes. We use observations of the Crab Nebula taken at low and medium zenith angles to assess the key performance parameters of the MAGIC stereo system. For low zenith angle observations, the standard trigger threshold of the MAGIC telescopes is ∼ 50  GeV. The integral sensitivity for point-like sources with Crab Nebula-like spectrum above 220 GeV is (0.66 ± 0.03)% of Crab Nebula flux in 50 h of observations. The angular resolution, defined as the σ of a 2-dimensional Gaussian distribution, at those energies is ≲ 0.07°, while the energy resolution is 16%. We also re-evaluate the effect of the systematic uncertainty on the data taken with the MAGIC telescopes after the upgrade. We estimate that the systematic uncertainties can be divided in the following components: < 15% in energy scale, 11%–18% in flux normalization and ± 0.15 for the energy spectrum power-law slope.     

1PN近似下脉冲星导航的观测方程及精度分析

完整推导1PN度规形式下脉冲到达时间方程与脉冲星导航的观测方程。分析导航观测中的相对论影响;给出观测方程的级数展开形式,在此基础上分析脉冲星历表参数对观测时间的影响;讨论行星星历误差对观测时间的影响;推导星体扁率引起的测量时延表达式,分析不同星体扁率引起的时延量级。     

γ射线脉冲星的代参数和能谱分析

为了对脉冲星的高能辐射进行研究,根据脉冲星观测的实际情况,重新推导了脉冲星代参数的计算公式.发现脉冲星的代参数与其γ射线能谱有很好的线性相关性,并拟合了代参数和能谱之间的线性关系.     

Non-symmetrical sparking may hint “zits” on a pulsar surface

Pulsar electrodynamics could be relevant to the physics of stellar surface, which remains poorly understood for more than half a centenary and is difficult to probe due to the absence of direct and clear observational evidence. Nevertheless, highly sensitive telescopes (e.g., China's Five-hundred-meter Aperture Spherical radio Telescope, FAST) may play an essential role to solve the problem since the predicted surface condition would have quite different characteristics in some models of pulsar structure, especially after the establishment of the standard model of particle physics. For instance, small hills (or “zits”) may exist on solid strangeon star surface with rigidity, preferential discharge, that is, gap sparking, may occur around the hills in the polar cap region. In this work, with the 110-min polarization observation of PSR B0950 $$08 targeted by FAST, we report that the gap sparking is significantly non-symmetrical to the meridian plane on which the rotational and magnetic axes lie. It is then speculated that this asymmetry could be the result of preferential sparking around zits which might rise randomly on pulsar surface. Some polarization features of both single pulses and the mean pulse, as well as the cross-correlation function of different emission regions, have also been presented.     

Morphology and characteristics of radio pulsars

This review describes the observational properties of radio pulsars, fast rotating neutron stars, emitting radio waves. After the introduction we give a list of milestones in pulsar research. The following chapters concentrate on pulsar morphology: the characteristic pulsar parameters such as pulse shape, pulsar spectrum, polarization and time dependence. We give information on the evolution of pulsars with frequency since this has a direct connection with the emission heights, as postulated in the radius to frequency mapping (RFM) concept. We deal successively with the properties of normal (slow) pulsars and of millisecond (fast-recycled) pulsars. The final chapters give the distribution characteristics of the presently catalogued 1300 objects.Received: 5 December 2003, Published online: 15 April 2004 Correspondence to: Richard Wielebinski