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El prisma de Wolaston en la determinación del magnetismo solar por el método de Leighton
Abstract
Se calcularon las aberraciones introducidas por un prisma Wolaston en un haz convergente y se propone un sistema compensador para dichas aberraciones, siendo las aberraciones residuales un astigmatismo menor que 60 y una distorsión 1/1000.
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http://sedici.unlp.edu.ar/handle/10915/99083
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49 and 115 St - Ex Liceo Apt. Floor 1
La Plata, Buenos Aires (C.P. 1900)
Phone: +54 0221 6447282
Tel: +54 0221 6696/6677 (int. 141)
La Plata, Buenos Aires (C.P. 1900)
Phone: +54 0221 6447282
Tel: +54 0221 6696/6677 (int. 141)
