Continuous high-resolution observation system using high-speed gaze and focus control with wide-angle triangulation

2020 ◽  
Author(s):  
Tomohiro Sueishi ◽  
Takuya Ogawa ◽  
Shoji Yachida ◽  
Masatoshi Ishikawa
Keyword(s):  
High Resolution ◽  
High Speed ◽  
Observation System ◽  
Wide Angle ◽  
Resolution Observation ◽  
High Resolution Observation

Application of K-FADOF in Solar High-Resolution Observation

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
Keyword(s):  
High Resolution ◽  
Resolution Observation ◽  
High Resolution Observation

High resolution observation of 3C 66B

1992 ◽  
Author(s):  
W. B. Sparks ◽  
F. Macchetto ◽  
N. J. Jackson ◽  
G. K. Miley
Keyword(s):  
High Resolution ◽  
Resolution Observation ◽  
High Resolution Observation

In Situ High-Resolution Observation for Decomposition of NaAlH4

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

Iue high-resolution observation of the Venus dayglow spectrum 1280-1380 Å

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

scholarly journals Interferometric Techniques Applied to High Resolution Observation of the Solar Granulation

1979 ◽  
Vol 50 ◽  
pp. 30-1-30-6
Author(s):  
Claude Aime
Keyword(s):  
High Resolution ◽  
Power Spectrum ◽  
Statistical Properties ◽  
Two Dimensional ◽  
Solar Granulation ◽  
One Dimensional ◽  
Resolution Observation ◽  
Stellar Interferometry ◽  
High Resolution Observation

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

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