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The Magneto-Optical Filter at Kanzelhöhe

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Motions in the Solar Atmosphere

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 239))

Abstract

An observing station based on the Magneto-Optical Filter (MOF) technology has been installed at Kanzelhöhe at the beginning of 1997. In this paper, the main characteristics of this instrument are discussed and a one day solar velocity observing run is shown.

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References

  • Cacciani A. and Moretti P.F. (1994), Instrumentation in Astronomy VIII, Proceedings of the SPIE Vol. 2198, Washington, USA, 219.

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  • Cacciani A. and Moretti P.F. (1995), in GON694: Helio and Asteroseismology from Earth and Space,R.K. Ulrich, E.J. Rhodes and W. Dappen (eds.), ASP Conference Series 76, 440.

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  • Cacciani A., Moretti P.F. and Rodgers W.E. (1997), Solar Phys. 174, 115.

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© 1999 Springer Science+Business Media Dordrecht

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Cacciani, A., Moretti, P.F., Messerotti, M., Hanslmeier, A., Otruba, W., Pettauer, T.V. (1999). The Magneto-Optical Filter at Kanzelhöhe. In: Hanslmeier, A., Messerotti, M. (eds) Motions in the Solar Atmosphere. Astrophysics and Space Science Library, vol 239. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-9331-1_26

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  • DOI: https://doi.org/10.1007/978-94-015-9331-1_26

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-90-481-5151-6

  • Online ISBN: 978-94-015-9331-1

  • eBook Packages: Springer Book Archive

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