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Anisotropy of Hectometric Cosmic Background

Published online by Cambridge University Press:  26 May 2016

Y.V. Tokarev ,
M.L. Kaiser ,
G.N. Boiko  and
P.V. Gustov
Y.V. Tokarev
Affiliation:
1 Radiophysical Research Institute, 25/14 Bolśhaya Pecherskaya st., Nizhny Novgorod, 603600, RF
M.L. Kaiser
Affiliation:
2NASA, Goddard Space Flight Center, Greenbelt, MD 20771, USA
G.N. Boiko
Affiliation:
1 Radiophysical Research Institute, 25/14 Bolśhaya Pecherskaya st., Nizhny Novgorod, 603600, RF
P.V. Gustov
Affiliation:
1 Radiophysical Research Institute, 25/14 Bolśhaya Pecherskaya st., Nizhny Novgorod, 603600, RF

Abstract

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The results of investigation of the low-frequency cosmic background by the WIND spacecraft near the L1 point during the deepest phase of the last solar activity minimum are presented. The antenna temperature modulation index and the ecliptic longitude of the primary area of radiation for frequencies 260, 516, 772, and 1028 kHz were measured by means of a dipole on the spacecraft which is rotated in ecliptic plane. Our results correct and complement the conclusions of the previous measurements made with IMP-6.

Type
Part 5: Galactic Surveys and Extended Emission
Information
Symposium - International Astronomical Union , Volume 199: The Universe at Low Radio Frequencies , 2002 , pp. 315 - 316
Copyright
Copyright © Astronomical Society of the Pacific 2002 

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