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Universal Anisotropy and Inhomogeneity of Space

  • Roland Pabisch
Part of the Linzer Universitätsschriften book series (LINZUNIVERS, volume 00)

Abstract

In 1968 Heer and Kohl [26] presented a paper about a “Theory for the measurement of the earth’s velocity through the 3°K cosmic radiation”. Already in 1969 Conklin [27] and then in 1977 Smoot, Gorenstein and Muller [1] reported about an experimentally observed dipol anisotropy in the cosmic microwave background radiation. This observation was readily interpreted as due to the motion of Earth relative to the radiation with a mean velocity of 390 ± 60 kms-1 [1]. More recent measurements yielded |uEarth| = 350kms-1 towards the constellation Leo (right ascension α = 1lh.2 and declination δ = -6°.l) [17].

Keywords

Fundamental Property Blackbody Radiation Separation Line Absolute Velocity Tangential Velocity Component 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Linzer Universitätsschriften-Verein 1999

Authors and Affiliations

  • Roland Pabisch
    • 1
  1. 1.Johannes Kepler Universität LinzLinz/DonauAustria

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