Near-Band IR Small Scene Star Image Segmentation Based on Partial Histogram Grey Level

Article Preview

Abstract:

The near-band IR star images segmentation and recognition is key technique in day time star navigation. Due to the scene of near-band IR star imaging relative small and stellar with high star grade are limited. Pertinence and dynamic grey level threshold is necessary for image processing arithmetic. In order to enhance near-band IR star images segmentation and recognition in real-time, this paper present the process of partial histogram grey level threshold and improve for actually near-band IR star images with scene of no more than 1.5°×1.5°. It can reduce the calculation of near-band IR star images with adjustable threshold. And get rid of disturbance of small imaging square stars and noise points.

You might also be interested in these eBooks

Info:

Periodical:

Pages:

1834-1839

Citation:

Online since:

January 2014

Authors:

Export:

Price:

Permissions CCC:

Permissions PLS:

Сopyright:

© 2014 Trans Tech Publications Ltd. All Rights Reserved

Share:

Citation:

[1] US 2006/0085130 AI DAYTIME STELLAR FOR ATTITUDE DETERMINATION Conference on Acquisition, Tracking and PointingⅩⅢ, 1999, 3692(4): 269-278.

Google Scholar

[2] Curtis W P, KENNETH K D. A grid algorithm for autonomous star identification[J]. IEEE Transaction on Areospace and Electronic system, 1997, 33(1): 202-213.

Google Scholar

[3] Daniel S C, CURTIS W P. Small field-of-view star identification using Bayesian decision theory[J]. IEEE Transaction on Aerospace and Electronic system, 2000, 36(3)773-783.

Google Scholar

[4] Hong J,DICKENSONJA. Neural-network-based autonomous star identification algorithm[J], Journal of guidance, Control and Dynamics, 2000, 23(4): 728-735.

DOI: 10.2514/2.4589

Google Scholar

[5] Pal A, Bakos G A. Astrometry in Wide-Field Survey[J]. PASP, 2006, 118: 1474-1483 Tabur V. fast algorithem for matching CCD images to a stellar catalogue[J].

Google Scholar

[6] PASA, 2007, 24: 189-198.

Google Scholar

[7] Mortari,D. K-vector range searching techniques. Adv. Astronaut. Sci. 2000. 105, 449-464.

Google Scholar

[8] T. k. Alex VKoteswara. CCD-Star Sensor for Indian Rebote Sensing Satellites[P]. Rao Laboratory for Electro-Optics, ISRO Bangalore-560058, 2002: 89~121.

Google Scholar

[9] Javier Portilla, Vasily Strela. Image denoising using scale mixtures Gaussians in the wavelet domain[J]. IEEE Transaction on Image Processing. 2003, 12(11): 1338-1351.

DOI: 10.1109/tip.2003.818640

Google Scholar