SCINTILLATIONS OF RADIO SOURCE 4C21.53 AT DECAMETER WAVELENGTHS AND ELONGATIONS 43&deg;&minus;138&deg;

Nikolai Nikolaevich Kalinichenko

doi:10.1615/RadioPhysicsRadioAstronomy.v3.i2.50

无线电物理和天文学期刊

总编辑: Leonid M. Lytvynenko (open in a new tab)

副总编辑s: Alexandr A. Konovalenko (open in a new tab) Valery M. Shulga (open in a new tab) Alexei A. Kostenko (open in a new tab)

每年出版 4 期

ISSN 打印: 2152-274X

ISSN 在线: 2152-2758

SCINTILLATIONS OF RADIO SOURCE 4C21.53 AT DECAMETER WAVELENGTHS AND ELONGATIONS 43°−138°

卷 3, 册 2, 2012, pp. 131-138

DOI: 10.1615/RadioPhysicsRadioAstronomy.v3.i2.50

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Nikolai Nikolaevich Kalinichenko
Institute of Radio Astronomy, National Academy Sciences of Ukraine

摘要

The statistical quantities of interplanetary scintillations at decameter wavelengths (scintillation index, power spectrum, cross-correlation function, probability density function) for the strong and weak scattering cases are estimated by analyzing the observations of 4C21.53 radio source scintillations. The obtained results can be used to test the models applied for analyzing interplanetary scintillations data at decameter wavelengths. The high efficiency of the DSP-z wide-band digital spectrum analyzer for interplanetary scintillations observations at decameter wavelengths is shown.

键词: interplanetary scintillations, decameter wavelengths, digital spectrum analyzer

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