Dispersion sensitivity of large-scale axial gradient index glass for spherochromat doublets

Author(s):  
Paul K. Manhart ◽  
Boyd V. Hunter ◽  
Richard Blankenbecler
1996 ◽  
Author(s):  
Mary G. Turner ◽  
Kenneth E. Moore

1985 ◽  
Vol 24 (24) ◽  
pp. 4321 ◽  
Author(s):  
Yasuhiro Koike ◽  
Hiroshi Hidaka ◽  
Yasuji Ohtsuka

2016 ◽  
Vol 53 (2) ◽  
pp. 022202
Author(s):  
韩培仙 Han Peixian ◽  
金光 Jin Gang ◽  
钟兴 Zhong Xing ◽  
夏春秋 Xia Chunqiu

1987 ◽  
Author(s):  
Paul O. McLaughlin ◽  
Minoru Toyama ◽  
Ichiro Kitano

1999 ◽  
Vol 173 ◽  
pp. 243-248
Author(s):  
D. Kubáček ◽  
A. Galád ◽  
A. Pravda

AbstractUnusual short-period comet 29P/Schwassmann-Wachmann 1 inspired many observers to explain its unpredictable outbursts. In this paper large scale structures and features from the inner part of the coma in time periods around outbursts are studied. CCD images were taken at Whipple Observatory, Mt. Hopkins, in 1989 and at Astronomical Observatory, Modra, from 1995 to 1998. Photographic plates of the comet were taken at Harvard College Observatory, Oak Ridge, from 1974 to 1982. The latter were digitized at first to apply the same techniques of image processing for optimizing the visibility of features in the coma during outbursts. Outbursts and coma structures show various shapes.


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