Calibration of an IR prism spectrometer with an echelette grating

1967 ◽  
Vol 7 (6) ◽  
pp. 623-624
Author(s):  
E. A. Yakovlev
Keyword(s):  
Echelette Grating

Reflexion von Clusterstrahlen an einem Echelettegitter / Reflection of Cluster Beams on an Echelette Grating

1973 ◽  
Vol 28 (10) ◽  
pp. 1733-1734
Author(s):  
H. Mayer
Keyword(s):  
Surface Structure ◽  
Flux Distribution ◽  
The Mean ◽  
Cluster Beams ◽  
Reflection Characteristics ◽  
Echelette Grating

Nitrogen cluster beams are reflected from an Echelette grating to investigate the influence of the surface structure on the reflection characteristics. If the mean cluster diameter is greater than the effective grating constant the same flux distribution is found as for a polished reflector. However, the flux distribution clearly spreads out in the plane of incidence if the cluster diameter becomes almost equal to the effective grating constant.

Concerning the Echelette Grating

1911 ◽  
Vol 34 ◽  
pp. 317
Author(s):  
A. Trowbridge
Keyword(s):  
Echelette Grating

Structure of the spectral image produced by an echelette grating

1990 ◽  
Vol 50 (5) ◽  
pp. 1834-1841
Author(s):  
E. A. Begovatov ◽  
V. V. Kuindzhi ◽  
T. S. Saamova ◽  
S. A. Strezhnev
Keyword(s):  
Spectral Image ◽  
Echelette Grating

Optical theory of the echelette grating

1947 ◽  
Vol 43 (2) ◽  
pp. 240-253 ◽  
Author(s):  
G. K. T. Conn
Keyword(s):  
Optical Properties ◽  
Optical System ◽  
Wave Length ◽  
Practical Importance ◽  
Resolving Power ◽  
Relative Importance ◽  
Available Energy ◽  
Length Relationship ◽  
Infra Red ◽  
Echelette Grating

The optical properties of reflecting echelette gratings, used in the infra-red region of the spectrum, are discussed theoretically. Expressions are derived for various important characteristics including the wave-length relationship, the dispersion and the resolving power of spectrometers using such gratings. The intensity distribution is discussed and illustrated by reference to a particular spectrometer fitted with a grating of 1200 lines to the inch. The relative importance of other factors such as the variation of available energy with wave-length, the dispersion of the preliminary optical system, etc., is considered and tabulated. Particular consideration is given to the properties of such gratings when used in much higher orders of interference than are common at present. With large aperture spectrometers, this possibility of using comparatively coarse gratings with a high order of interference is of great practical importance.

Theory of the Echelette Grating II*

1958 ◽  
Vol 48 (10) ◽  
pp. 704 ◽  
Author(s):  
John H. Rohrbaugh ◽  
Robert D. Hatcher
Keyword(s):  
Echelette Grating

Theory of the Echelette Grating III*

1958 ◽  
Vol 48 (10) ◽  
pp. 710 ◽  
Author(s):  
John H. Rohrbaugh ◽  
Charles Pine ◽  
William G. Zoellner ◽  
Robert D. Hatcher
Keyword(s):  
Echelette Grating

Theory of the Echelette Grating I*

1956 ◽  
Vol 46 (2) ◽  
pp. 104 ◽  
Author(s):  
Robert D. Hatcher ◽  
John H. Rohrbaugh
Keyword(s):  
Echelette Grating
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