Reconstruction of post-adaptive images of Io observed with LBTI and - - PowerPoint PPT Presentation

reconstruction of post adaptive images of io observed
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Reconstruction of post-adaptive images of Io observed with LBTI and - - PowerPoint PPT Presentation

Reconstruction of post-adaptive images of Io observed with LBTI and KECK M. Bertero. P. Boccacci e A. La Camera DIBRIS, Universit di Genova ADONI2016 - Firenze 12-14 Marzo 2016 Strumentazione prevista LBC Red/Blue (2006-7) LUCIFER


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Reconstruction of post-adaptive images of Io observed with LBTI and KECK

  • M. Bertero. P. Boccacci e A. La Camera

DIBRIS, Università di Genova ADONI2016 - Firenze 12-14 Marzo 2016

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LBC Red/Blue (2006-7) LBTI (2009) LINC-NIRVANA (2009) MODS 1&2 (2008-9) LUCIFER 1&2 (2008-9) PEPSI (2009)

Strumentazione prevista

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Ideal Fizeau interferometric PSF

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Observations at different angles are required 22.8 m 8.4 m for obtaining, by means of suitable algorithms, a unique image with a uniform resolution of a 22.8m mirror

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The PSF derived from an image of the star HD-78141

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The 7 images of Io observed with LBTI, December 24, 2015

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First reconstructions sent on May 5, 2014 A quick reply by John Spencer, Boulder, …..

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All circles correspond to existing volcanos…plus one

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Proiection on the lat-long plane of both the local reconstruction and the Voyager image of Loki and their superposition; due hot spots, presumably one permanent ad the other due to a ‘’resurfacing’’ process.

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Improved reconstruction obtained with a multi-step approach

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Identified volcanos and artifacts

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January 4, 2015

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February 5, 2015

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1 unknown 7 Janus patera 13 Culam patera 2 unknown 8 Sigurd patera 14 Prometheus * * 3 Zal ? 9 Itzamma patera 4 Amirani * * 10 Dark patera 5 Gish Bar patera 11 unknown 6 Tanhaki patera 12 Malik patera

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Io observed with Keck II: Pillan eruption, August 14, 2007 J-band H-band K-band

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L-band M-band Reconstructions with the multi-step approach

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THANK YOU !