Abstract
A precise two-dimensional positioning device has been developed for use in conjunction with a resonant scattering spectrometer to study the spatial distribution of solar velocity fields. The principle of operation and constructional details are discussed and the experimental performance is evaluated. As an illustration of its use preliminary data obtained from a meridional scan are presented.
Proceedings of the 14th ESLAB Symposium on Physics of Solar Variations, 16–19 September 1980, Scheveningen, The Netherlands.
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Brookes, J. R., Isaak, G. R., and van der Raay, H. B.: 1976, Nature 259, 92.
Brookes, J. R., Isaak, G. R., and van der Raay, H. B.: 1978, Monthly Notices Roy. Astron. Soc. 185, 1.
Claverie, A., Isaak, G. R., McLeod, C. P., van der Raay, H. B. and Roca Cortes, T.: 1979, Nature 282, 591.
Claverie, A., Isaak, G. R., McLeod, C. P., van der Raay, H. B., and Roca Cortes, T.: 1980, Astron. Astrophys. 91, L9.
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© 1981 Springer Science+Business Media Dordrecht
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Brookes, J.R., Isaak, G.R., Van der Raay, H.B. (1981). A Two-Dimensional Solar Spectrometer. In: Domingo, V. (eds) Physics of Solar Variations. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-9633-1_44
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DOI: https://doi.org/10.1007/978-94-010-9633-1_44
Publisher Name: Springer, Dordrecht
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