High resolution observation of 3C 66B

1992 ◽  
Author(s):  
W. B. Sparks ◽  
F. Macchetto ◽  
N. J. Jackson ◽  
G. K. Miley
2012 ◽  
Vol 39 (8) ◽  
pp. 0808003
Author(s):  
张俊 Zhang Jun ◽  
杨勇 Yang Yong ◽  
程学武 Cheng Xuewu ◽  
杨尚斌 Yang Shangbin ◽  
龚威 Gong Wei

2007 ◽  
pp. 1621-1624
Author(s):  
Hiroshi Kawasaki ◽  
Somei Ohnuki ◽  
Takanori Suda ◽  
Naoyuki Hashimoto ◽  
Yoshitsugu Kojima

1981 ◽  
Vol 8 (1) ◽  
pp. 111-112 ◽  
Author(s):  
Samuel T. Durrance ◽  
Robert R. Conway ◽  
Charles A. Barth ◽  
A. L. Lane

1979 ◽  
Vol 50 ◽  
pp. 30-1-30-6
Author(s):  
Claude Aime

AbstractMichelson,one-dimensional, and two-dimensional apertures are used to obtain the statistical properties of the solar granulation. The calibration of the power spectrum is performed via Michelson stellar interferometry as well as by the use of changes in seeing conditions during speckle-interferometric measurements. The correction of 40 analyses, determined with Fried's parameter ro ranging between 2.5 cm and 11.5 cm, provides satisfactory convergence for frequencies up to 3 cycles per arc second


2001 ◽  
Vol 123 (43) ◽  
pp. 10786-10787 ◽  
Author(s):  
K. Takegoshi ◽  
Tomomi Yano ◽  
Kazuyuki Takeda ◽  
Takehiko Terao

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