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Monitoring of interplanetary and ionosphere scintillations at frequency 110 MHz 

Authors: V. I. Shishov a;  S. A. Tyul'bashev a;  I. A. Subaev a; I. V. Chashei a
Affiliation:   a Pushchino Radio Astronomy Observatory of ASC of P.N. Lebedev Physical Institute, Russia
DOI: 10.1080/10556790701610381
Publication Frequency: 6 issues per year
Published in: journal Astronomical & Astrophysical Transactions, Volume 26, Issue 6 December 2007 , pages 677 - 681
Formats available: HTML (English) : PDF (English)

The circumstances under which this title is published have changed:

Reason for change: Changed Publisher
Date of change: 2008



Abstract

Large Phased Array of the P.N. Lebedev Physical Institute is the most sensitive in the world at the metre waveband. It allows simultaneous observation of two independent diagrams each consisting of 16 beams. We are planning to introduce a program of monitoring interplanetary and ionospheric scintillation using observations of radio sources by one multi-beam diagram. The methods of observations and data reduction are discussed. We present the first results of seven day test observations for a strip of the sky in a region with declinations between 28° and 32° by using an eight-beam diagram.
Keywords: Solar wind; Interplanetary scintillation; Ionospheric scintillation
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