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On the visibility of the libration clouds

  • S. Röser
1 Zodiacal Light 1.3 Models and Interpretations
Part of the Lecture Notes in Physics book series (LNP, volume 48)

Keywords

Radiation Pressure Orbital Element Libration Point Surface Brightness Interplanetary Dust 
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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References

  1. Burnett, G.B.; Sparrow, J.G. and Ney, E.P.; Is the Zodiacal Light intensity steady? Nature 249, 639 (1974).Google Scholar
  2. Bruman, J.R.; A Lunar Libration Point Experiment. Icarus 10, 197 (1969).Google Scholar
  3. Fechtig, H.; Gentner, W.; Hartung, J.B.; Nagel, K.; Neukum, G.; Schneider E.; and Storzer, D.; Microcraters on lunar samples. Soviet-American Conference on Cosmochemistry of the moon and the planets, Moscow, 1974.Google Scholar
  4. Hughes, D.W.;Interplanetary Dust and its influx to the Earth's Surface, XVI Plenary Meeting of Cospar, Konstanz, 1973.Google Scholar
  5. Matas, V.; Periodic Solutions of a Disturbed Elliptic Restricted Three-Body-Problem. BACz, 25, 129 (1974).Google Scholar
  6. Roach, J.R.; Counterglow from the Earth-Moon Libration Points, Planetary and Space Science, 23, 173 (1975).Google Scholar
  7. Robertson, H.P.; Dynamical effects of radiation in the solar system MNRAS, 97, 423 (1937).Google Scholar
  8. Shapiro, I.I.; Lautman, D.A.; and Colombo, G.; The Earth's dust belt: Fact or fiction? JGR 71, 5695 (1966).Google Scholar

Copyright information

© Springer-Verlag 1976

Authors and Affiliations

  • S. Röser
    • 1
  1. 1.Max-Planck-Institut für AstronomieHeidelberg-KönigstuhlGermany

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