NAOC Open IR
Are pulsar giant pulses induced by re-emission of cyclotron resonance absorption?
Lu, Ji-Guang1,2; Wang, Wei-Yang3,4; Peng, Bo1,2; Xu, Ren-Xin5,6
2021-03-01
Source PublicationRESEARCH IN ASTRONOMY AND ASTROPHYSICS
ISSN1674-4527
Volume21Issue:2Pages:4
AbstractIt is conjectured that coherent re-emission of cyclotron resonance absorption could result in pulsar giant pulses. This conjecture seems reasonable as it can naturally explain the distribution of pulsars with giant pulses on the P-(P) over dot diagram.
Keywordpulsars: general radiation mechanisms: non-thermal plasmas magnetic fields
Funding OrganizationNational Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Open Project Program of the Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; Open Project Program of the Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; FAST FELLOWSHIP ; FAST FELLOWSHIP ; CAS-MPG LEGACY funding "Low-Frequency Gravitational Wave Astronomy and Gravitational Physics in Space" ; CAS-MPG LEGACY funding "Low-Frequency Gravitational Wave Astronomy and Gravitational Physics in Space" ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Open Project Program of the Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; Open Project Program of the Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; FAST FELLOWSHIP ; FAST FELLOWSHIP ; CAS-MPG LEGACY funding "Low-Frequency Gravitational Wave Astronomy and Gravitational Physics in Space" ; CAS-MPG LEGACY funding "Low-Frequency Gravitational Wave Astronomy and Gravitational Physics in Space" ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Open Project Program of the Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; Open Project Program of the Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; FAST FELLOWSHIP ; FAST FELLOWSHIP ; CAS-MPG LEGACY funding "Low-Frequency Gravitational Wave Astronomy and Gravitational Physics in Space" ; CAS-MPG LEGACY funding "Low-Frequency Gravitational Wave Astronomy and Gravitational Physics in Space" ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Open Project Program of the Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; Open Project Program of the Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; FAST FELLOWSHIP ; FAST FELLOWSHIP ; CAS-MPG LEGACY funding "Low-Frequency Gravitational Wave Astronomy and Gravitational Physics in Space" ; CAS-MPG LEGACY funding "Low-Frequency Gravitational Wave Astronomy and Gravitational Physics in Space"
DOI10.1088/1674-4527/21/2/29
Language英语
Funding ProjectNational Key R&D Program of China[2018YFA0404703] ; National Natural Science Foundation of China[11673002] ; National Natural Science Foundation of China[12003047] ; National Natural Science Foundation of China[U1531243] ; Open Project Program of the Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; FAST FELLOWSHIP ; CAS-MPG LEGACY funding "Low-Frequency Gravitational Wave Astronomy and Gravitational Physics in Space"
Funding OrganizationNational Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Open Project Program of the Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; Open Project Program of the Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; FAST FELLOWSHIP ; FAST FELLOWSHIP ; CAS-MPG LEGACY funding "Low-Frequency Gravitational Wave Astronomy and Gravitational Physics in Space" ; CAS-MPG LEGACY funding "Low-Frequency Gravitational Wave Astronomy and Gravitational Physics in Space" ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Open Project Program of the Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; Open Project Program of the Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; FAST FELLOWSHIP ; FAST FELLOWSHIP ; CAS-MPG LEGACY funding "Low-Frequency Gravitational Wave Astronomy and Gravitational Physics in Space" ; CAS-MPG LEGACY funding "Low-Frequency Gravitational Wave Astronomy and Gravitational Physics in Space" ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Open Project Program of the Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; Open Project Program of the Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; FAST FELLOWSHIP ; FAST FELLOWSHIP ; CAS-MPG LEGACY funding "Low-Frequency Gravitational Wave Astronomy and Gravitational Physics in Space" ; CAS-MPG LEGACY funding "Low-Frequency Gravitational Wave Astronomy and Gravitational Physics in Space" ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Open Project Program of the Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; Open Project Program of the Key Laboratory of FAST, NAOC, Chinese Academy of Sciences ; FAST FELLOWSHIP ; FAST FELLOWSHIP ; CAS-MPG LEGACY funding "Low-Frequency Gravitational Wave Astronomy and Gravitational Physics in Space" ; CAS-MPG LEGACY funding "Low-Frequency Gravitational Wave Astronomy and Gravitational Physics in Space"
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000631527800001
PublisherNATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/78875
Collection中国科学院国家天文台
Corresponding AuthorLu, Ji-Guang
Affiliation1.Chinese Acad Sci, CAS Key Lab FAST, Natl Astron Observ, Beijing 100101, Peoples R China
2.Chinese Acad Sci, Guizhou Radio Astron Observ, Guiyang 550025, Peoples R China
3.Chinese Acad Sci, Natl Astron Observ, Key Lab Computat Astrophys, Beijing 100101, Peoples R China
4.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
5.Peking Univ, Dept Astron, Beijing 100871, Peoples R China
6.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China
Recommended Citation
GB/T 7714
Lu, Ji-Guang,Wang, Wei-Yang,Peng, Bo,et al. Are pulsar giant pulses induced by re-emission of cyclotron resonance absorption?[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2021,21(2):4.
APA Lu, Ji-Guang,Wang, Wei-Yang,Peng, Bo,&Xu, Ren-Xin.(2021).Are pulsar giant pulses induced by re-emission of cyclotron resonance absorption?.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,21(2),4.
MLA Lu, Ji-Guang,et al."Are pulsar giant pulses induced by re-emission of cyclotron resonance absorption?".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 21.2(2021):4.
Files in This Item:
There are no files associated with this item.
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[Lu, Ji-Guang]'s Articles
[Wang, Wei-Yang]'s Articles
[Peng, Bo]'s Articles
Baidu academic
Similar articles in Baidu academic
[Lu, Ji-Guang]'s Articles
[Wang, Wei-Yang]'s Articles
[Peng, Bo]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[Lu, Ji-Guang]'s Articles
[Wang, Wei-Yang]'s Articles
[Peng, Bo]'s Articles
Terms of Use
No data!
Social Bookmark/Share
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.