High resolution observations: The state of the art and beyond

Details High resolution observations: The state of the art and beyond High resolution observations: The state of the art and beyond

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.344....9t&link_type=abstract

In ESA, Solar Physics and Astrophysics at Interferometric Resolution p 9-14 (SEE N93-10901 01-90)

Physics

Optics

1

High Resolution, Imaging Techniques, Observation, Solar Instruments, Solar Physics, Adaptive Optics, Magnetic Signatures, Polarimetry, Solar Granulation, Sunspots

Scientific paper

The meaning of high resolution and its scientific importance with regard to solar observations is discussed. The state of the art is reviewed, looking into Solar Optical Universal Polarimeter (SOUP) observations, image selection techniques, and adaptive optics. It is concluded that until there are observations in space, complete understanding of processes in the solar photosphere, chromosphere, transition region, and corona will be impossible. The importance of high resolution is considered with regard to solar surface and convection, solar photosphere inside and outside magnetic fields, and sunspot geometry.

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