Pulsar diffractive scintillation at 1.4 and 4.8GHz

Q4 Physics and Astronomy
V. Malofeev, O. Malov, W. Sieber, A. Jessner, S. Tyul'Bashev, B. Klein, R. Wielebinski
{"title":"Pulsar diffractive scintillation at 1.4 and 4.8GHz","authors":"V. Malofeev, O. Malov, W. Sieber, A. Jessner, S. Tyul'Bashev, B. Klein, R. Wielebinski","doi":"10.1080/10556790701614755","DOIUrl":null,"url":null,"abstract":"Abstract The diffractive interstellar scintillation of 11 pulsars at 1410 MHz and of five pulsars at 4800 MHz was analysed to estimate the spectrum of the electron density fluctuations as well as the ACF, CCF and the structure function. We present dynamic spectra for a few pulsars at high frequencies in the strong and weak regime and show that a lensing effect probably exists for pulsar PSR B2020+28 at 1410 MHz. The mean value of the indexes of the power law spectra for an ensemble of pulsars is in good agreement with a Kolmogorov spectrum.","PeriodicalId":52135,"journal":{"name":"Astronomical and Astrophysical Transactions","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2007-12-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomical and Astrophysical Transactions","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1080/10556790701614755","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"Physics and Astronomy","Score":null,"Total":0}
引用次数: 0

Abstract

Abstract The diffractive interstellar scintillation of 11 pulsars at 1410 MHz and of five pulsars at 4800 MHz was analysed to estimate the spectrum of the electron density fluctuations as well as the ACF, CCF and the structure function. We present dynamic spectra for a few pulsars at high frequencies in the strong and weak regime and show that a lensing effect probably exists for pulsar PSR B2020+28 at 1410 MHz. The mean value of the indexes of the power law spectra for an ensemble of pulsars is in good agreement with a Kolmogorov spectrum.
脉冲星在1.4和4.8GHz的衍射闪烁
分析了11颗1410 MHz脉冲星和5颗4800 MHz脉冲星的衍射星际闪烁,估计了电子密度波动谱、ACF、CCF和结构函数。我们给出了几颗脉冲星在强和弱波段的高频动态光谱,并表明PSR B2020+28在1410 MHz波段可能存在透镜效应。脉冲星系综幂律谱指标的平均值与柯尔莫哥洛夫谱吻合较好。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 求助全文
来源期刊
Astronomical and Astrophysical Transactions
Astronomical and Astrophysical Transactions Physics and Astronomy-Instrumentation
CiteScore
0.40
自引率
0.00%
发文量
16
期刊介绍: Astronomical and Astrophysical Transactions (AApTr) journal is being published jointly by the Euro-Asian Astronomical Society and Cambridge Scientific Publishers, The journal provides a forum for the rapid publication of material from all modern and classical fields of astronomy and astrophysics, as well as material concerned with astronomical instrumentation and related fundamental sciences. It includes both theoretical and experimental original research papers, short communications, review papers and conference reports.
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信