High resolution solar imaging

Details High resolution solar imaging High resolution solar imaging

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003jalpo..45c..16g&link_type=abstract

Journal of the Association of Lunar & Planetary Observers, The Strolling Astronomer (ISSN 0039-2502), Vol. 45, No. 3, p. 16 - 20

Physics

Optics

1

Solar Imaging

Scientific paper

Solar imaging is such like lunar and planetary imaging in that quality optics, a stable mount and long focal lengths are needed to achieve good results. Reduction of glare and both infrared and ultraviolet radiation is the primary difference. This can work to the observer's advantage by allowing very short shutter speeds, even at extremely long focal lengths. Apertures from 6 to 10 inches and larger can produce professional results.

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