Abstract
Solar physics requires more and more multiwavelength observations, not only with high spatial and time resolution, but also with wide coverage in space and time. We review briefly instruments dedicated to the solar interior, visible layers and the corona. In addition to the accuracy of spectroscopy and polarization measurements, we emphasize the coverage of data sets in the k − ω diagram. New image restoration methods are reviewed, in the context of the best compromise between spatial resolution and isoplanetic field of view. Ambitious projects do exist, as well as new generation telescopes under construction. Progress in the establishment of data bases and easier data exchange between observatories using complementary facilities look very promising for the future.
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Mein, P. (1997). New ground-based solar instrumentation. In: Simnett, G.M., Alissandrakis, C.E., Vlahos, L. (eds) Solar and Heliospheric Plasma Physics. Lecture Notes in Physics, vol 489. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0105679
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DOI: https://doi.org/10.1007/BFb0105679
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