Optimal two-mirror system for laser radiation focusing

2009 ◽  
Vol 39 (10) ◽  
pp. 977-980 ◽  
Author(s):  
Andrey V Gitin
2020 ◽  
Vol 83 (11) ◽  
pp. 1533-1537
Author(s):  
S. A. Krat ◽  
A. P. Kharina ◽  
I. A. Sorokin ◽  
V. A. Kostyushin ◽  
E. D. Vovchenko ◽  
...  

2013 ◽  
Vol 425 (5) ◽  
pp. 052022 ◽  
Author(s):  
H Yumoto ◽  
H Mimura ◽  
S Matsuyama ◽  
T Koyama ◽  
Y Hachisu ◽  
...  

1978 ◽  
Vol 48 ◽  
pp. 271-278
Author(s):  
Chr. Kühne

The PZT according to MARKOWITZ, undoubtedly one of the most accurate measuring instruments, has become an integral part of astronomy in the last years. Yet there are two reasons why I still tried to improve the MARKOWITZ basic idea.For the MARKOWITZ process the use of a lens objective is imperative. Because of the diameter limitations of the lens objectives the magnitude is reduced. Although a 65 cm PZT has been put into operation in Washington recently, the thermal difficulties encountered made it necessary to control the temperature actively. In addition, the 65 cm diameter of a lens equipped with 4 elements can be considered as the very limit, but not for a mirror system.In addition there are still more disadvantages using lens objectives. The useable field is restricted by astigmatism, reducing the range of declination. The transmission, especially in the blue wavelengths, decreases very rapidly with the thickness of lenses. For large multilens objectives the transmission is less than for a mirror system.


1983 ◽  
Vol 44 (C2) ◽  
pp. C2-19-C2-25
Author(s):  
M. C. Gower ◽  
R. G. Caro

1980 ◽  
Vol 41 (C4) ◽  
pp. C4-31-C4-36
Author(s):  
J. R. Meyer ◽  
F. J. Bartoli ◽  
M. R. Kruer

1974 ◽  
Vol 113 (7) ◽  
pp. 385 ◽  
Author(s):  
V.S. Letokhov ◽  
V.P. Chebotaev

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