High resolution spectroscopy of active regions with adaptive optic

Details High resolution spectroscopy of active regions with adaptive optic High resolution spectroscopy of active regions with adaptive optic

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000spd....31.0304s&link_type=abstract

American Astronomical Society, SPD Meeting #31, #03.04; Bulletin of the American Astronomical Society, Vol. 32, p.834

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With the NSO low-order adaptive optic system at the NSO Dunn Solar Telescope it is now possible to perform spectroscopic measurements at high angular resolution and high signal-to-noise level. The performance of the AO system for spectroscopic investigations will be demonstrated. By using a dual Fabry-Perot spectrometer we obtained spectral line scans of active regions with a spatial resolution of 0.3 arcsec at 557nm. We use these data to adress questions of magnetoconvection in active regions. This work is supported by NSO/AURA

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