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Proceedings Paper

Diffraction effects on very large space instruments: a detailed analysis to solar coronagraphy
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Paper Abstract

Recent possibility of building clusters of micro-satellites have increased the interest on extremely large space instruments. Since this growing is not merely a change of scale, performance of these new instruments has to be critically re-analyzed under this new perspective. As an example, diffraction effects can lead to new levels of signal-to-noise ratio, greatly increasing the possible performance of classical optical instruments. In this work we have analyzed the diffraction behavior of an opaque disc acting as external occulter in a space solar coronagraph. Since the occulter can be set at great distance from the telescope, improvements on signal-to-noise ratio are obtained. Moreover, this analysis can lead to a determination of a potential apodization function for the occulter.

Paper Details

Date Published: 18 August 2005
PDF: 7 pages
Proc. SPIE 5901, Solar Physics and Space Weather Instrumentation, 59011C (18 August 2005); doi: 10.1117/12.620292
Show Author Affiliations
Fabio Frassetto, Univ. of Padova (Italy)
CNR-INFM (Italy)
Giampiero Naletto, Univ. of Padova (Italy)
CNR-INFM (Italy)

Published in SPIE Proceedings Vol. 5901:
Solar Physics and Space Weather Instrumentation
Silvano Fineschi; Rodney A. Viereck, Editor(s)

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