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脉冲星强、弱辐射模式变换的分析研究
Alternative TitleStudy of the Phenomena of Pulsar's Strong and Weak Mode;Switching
迪里努尔·阿不都热希提1; 艾力·伊沙木丁2
2012
Source Publication新疆大学学报(自然科学版)
Volume29Issue:4Pages:452-459
Contribution Rank2
Abstract本文主要讨论了脉冲星强、弱辐射模式变换现象.通过分析研究脉冲星消零现象、旋转暂现射电源现象,以及有些脉冲星中发现的稀疏的超强单个脉冲现象,指出这三种现象可能都是脉冲星磁层处于某种临界态时的强、弱辐射模式变换现象,只是模式的持续时标很不一样.提出脉冲星强、弱模式的持续时标和脉冲星射电辐射的演化有关系.随着脉冲星自转能不断损耗,脉冲星的总的射电辐射可能是随着强辐射模式的持续时标的不断变短而不断下降.
Other AbstractIn this paper, we mainly study the strong, weak mode switching phenomenon of pulsar. Through analyzing of the nulling, rotating radio transient (RRAT), as well as the sparse super strong pulse phenomenon which founded in some pulsars, we pointed out that, all these three phenomenon are the strong, weak mode switching phenomenon of the pulsar when its magnetosphere is in a certain critical state. Only the durations of the strong mode in these three phenomenon are very different. We proposed that the strong, weak emission mode duration of pulsar have a relation with the the evolution of pulsar radiation. With the continuous loss of rotating energy of pulsar, pulsar total radio emission may be gradually decreased as the duration of strong emission mode took less and less time.
Keyword脉冲星 单个脉冲 旋转暂先射电源
SubtypeJournal Article
Indexed By中文核心期刊要目总览
Language中文
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/659
Collection射电天文研究室_脉冲星研究团组
光学天文与技术应用研究室
Corresponding Author艾力·伊沙木丁
Affiliation1.新疆大学物理科学与技术学院,新疆乌鲁木齐830046
2.中国科学院新疆天文台,新疆乌鲁木齐830011
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
迪里努尔·阿不都热希提,艾力·伊沙木丁. 脉冲星强、弱辐射模式变换的分析研究[J]. 新疆大学学报(自然科学版),2012,29(4):452-459.
APA 迪里努尔·阿不都热希提,&艾力·伊沙木丁.(2012).脉冲星强、弱辐射模式变换的分析研究.新疆大学学报(自然科学版),29(4),452-459.
MLA 迪里努尔·阿不都热希提,et al."脉冲星强、弱辐射模式变换的分析研究".新疆大学学报(自然科学版) 29.4(2012):452-459.
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