STELLAR SPECKLE IMAGING BY REFERENCE TO DIFFERENT-COLORED SPECKLEGRAMS

被引：2

作者：

BABA, N ^{[1
]}

KUWAMURA, S ^{[1
]}

MIURA, N ^{[1
]}

NORIMOTO, Y ^{[1
]}

机构：

[1] OKAYAMA ASTROPHYS OBSERV,KAMOGATA 71902,JAPAN

来源：

OPTICS LETTERS | 1995年 / 20卷 / 10期

关键词：

D O I：

10.1364/OL.20.001175

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

Stellar specklegrams at different wavelengths are examined. The position of the brightest speckle at one wavelength is shown to coincide nearly with that at a widely separated wavelength. The shift-and-add operation for specklegrams at one wavelength produces a high-resolution stellar image at the other wavelength. We show that the shift-and-add operation at 450 nm results in a high-resolution image at 800 nm by use of observational speckle data from which specklegrams at these wavelengths are taken simultaneously.

引用

页码：1175 / 1177

页数：3

共 12 条

[1]

ALLOIN DM, 1989, DIFFRACTION LTD IMAG, P141

[2] WIDEBAND SPECKLE SPECTROSCOPY BASED ON THE SHIFT-AND-ADD METHOD [J].