脉冲星在1.4和4.8GHz的衍射闪烁

Q4 Physics and Astronomy Astronomical and Astrophysical Transactions Pub Date : 2007-12-13 DOI:10.1080/10556790701614755
V. Malofeev, O. Malov, W. Sieber, A. Jessner, S. Tyul'Bashev, B. Klein, R. Wielebinski
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引用次数: 0

摘要

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。
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Pulsar diffractive scintillation at 1.4 and 4.8GHz
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.
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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.
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