Understanding the WMAP results: low-order multipoles and dust in the vicinity 
of the solar system

Dikarev, V.; Preuss, O.; Solanki, S. K.; Krüger, H.; Krivov, A.

doi:10.1007/s11038-007-9172-4

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Understanding the WMAP results: low-order multipoles and dust in the vicinity of the solar system

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Dikarev, V.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

/persons/resource/persons104137

Preuss, O.
IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society;

/persons/resource/persons104218

Solanki, S. K.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Krüger, H.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Dikarev, V., Preuss, O., Solanki, S. K., Krüger, H., & Krivov, A. (2007). Understanding the WMAP results: low-order multipoles and dust in the vicinity of the solar system. Earth, Moon and Planets, 102, 555-561. doi:10.1007/s11038-007-9172-4.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0014-FE1B-F

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