Cavallini, F. and Berrilli, F. and Cantarano, S. and Egidi, A. (2002) IBIS (Interferometric BIdimensional spectrometer). Il nuovo cimento C, 25 (5\6). pp. 673-679. ISSN 1826-9885
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Abstract
IBIS is a new instrument for solar bidimensional spectroscopy, now under construction at the Arcetri Astrophysical Observatory. It essentially consists of two Fabry-Perot interferometers, piezo-scanned and capacity servo-controlled, which are used in classic mount and in axial-mode, in series with a narrow-band interference filter. This instrument will operate on a large field of view (80����) and on a large wavelength range (5800–8600 ˚A), with high spectral (λ/Δλ � 250000), spatial (�0.2) and temporal (� 5 frames s−1) resolution. When completed in 2002, it will be one of the leading instruments for solar research, well suited for a new generation telescopes such as THEMIS.
Item Type: | Article |
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Additional Information: | Paper presented at the International Meeting on THEMIS and the New Frontiers of Solar Atmosphere Dynamics, Rome, Italy, March 19-21, 2001. |
Uncontrolled Keywords: | Solar physics ; Solar instruments ; Photometric, polarimetric, and spectroscopic instrumentation ; Conference proceedings |
Subjects: | 500 Scienze naturali e Matematica > 530 Fisica |
Depositing User: | Marina Spanti |
Date Deposited: | 12 Mar 2020 16:58 |
Last Modified: | 12 Mar 2020 16:58 |
URI: | http://eprints.bice.rm.cnr.it/id/eprint/14878 |
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