Abstract
An observing station based on the Magneto-Optical-Filter (MOF) technology is being installed at Osservatorio Astronomico di Capodimonte, in Napoli. In this paper, the main characteristics and goals of this new instrument are discussed, and several velocity and magnetic observations from a test campaign are shown.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Cacciani, A., Moretti, P.F., (1994), in “Instrumentation in Astronomy VIII”, 2198, 219, ed. SPIE, Washington, USA
Cacciani, A., Moretti, P.F. (1995), in “GONG′94: Helio-and asteroseismology from Earth and Space” 1995, 76, 440, R.K. Ulrich, E.J. Rhodes Jr. & W. Däppen (eds.), ASP Conference Series
Marmolino, C., Oliviero, M., Severino, G., and Smaldone L.A. (1996), A&A, submitted
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1997 Springer Science+Business Media Dordrecht
About this chapter
Cite this chapter
Moretti, P.F. et al. (1997). The Magneto-Optical Filter in Napoli: Perspectives and Test Observations. In: Pijpers, F.P., Christensen-Dalsgaard, J., Rosenthal, C.S. (eds) SCORe ’96: Solar Convection and Oscillations and their Relationship. Astrophysics and Space Science Library, vol 225. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5167-2_32
Download citation
DOI: https://doi.org/10.1007/978-94-011-5167-2_32
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-6172-8
Online ISBN: 978-94-011-5167-2
eBook Packages: Springer Book Archive