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Brightness Fluctuations and Global Oscillations of the Sun (DIFOS Experiment)

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The Coronas-F Space Mission

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 400))

Abstract

The results of brightness observations of the Sun as a star by DIFOS experiment onboard CORONAS satellite are presented. The observations are performed in six spectral channels, namely 350, 500, 650, 850, 1,100, and 1,500 nm. The description of DIFOS multichannel photometer is provided. Data processing was done by analytic signal transformation. The theory of analytic signal transformation is presented.

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Authors and Affiliations

  1. Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation RAS (IZMIRAN), Troitsk, Moscow, Russia

    Yu. D. Zhugzhda, V. D. Kuznetsov & N. I. Lebedev

Authors
  1. Yu. D. Zhugzhda
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  2. V. D. Kuznetsov
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  3. N. I. Lebedev
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Corresponding author

Correspondence to Yu. D. Zhugzhda .

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Editors and Affiliations

  1. IZMIRAN, Troitsk, Russia

    Vladimir Kuznetsov

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Zhugzhda, Y.D., Kuznetsov, V.D., Lebedev, N.I. (2014). Brightness Fluctuations and Global Oscillations of the Sun (DIFOS Experiment). In: Kuznetsov, V. (eds) The Coronas-F Space Mission. Astrophysics and Space Science Library, vol 400. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-39268-9_2

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  • DOI: https://doi.org/10.1007/978-3-642-39268-9_2

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-642-39267-2

  • Online ISBN: 978-3-642-39268-9

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