Full text: XVIIIth Congress (Part B3)

    
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KEYWORDS: 
SYSTEMATIC CORRECTION MECHANISM OF GEOMETRIC DISTORTIONS 
IN THE KITSAT-1 CCD EARTH IMAGES 
Impyeong Leet, Taejung Kimt, Soon D. Choi# 
Research Fellowt, Directort 
Satellite Technology Research Center (SaTReC) 
Korea Advanced Institute of Science and Technology(KAIST) 
373-1, Kusung-dong, Yusung-Ku, Taejon, 305-701, Korea 
e-mail: iplee 9 satrec.kaist.ac.kr, tjkim 9 satrec.kaist.ac.kr 
Commission Ill, Working Group III /1 
ABSTRACT 
Remote Sensing, Correction, Modeling, Distortion, Satellite, Geometric, Precision 
The CCD Earth Image Experiment (CEIE) is one of the main payload of the KITSAT-1, an experimental micro-satellite. 
Since it was launched on Oct. 10, 1992, the CEIE has taken more than 500 images on the Earth surface world-wide so 
far. An image from space is very different from a feature on the real Earth surface due to diverse radiometric and 
geometric 
distortions. Preprocessing to remove those distortions has to take place before the image data is processed 
and analyzed further for various applications. The images from the KITSAT-1 are dramatically distorted due to very poor 
pointing ability of the satellite. Moreover, the attitude determination and control system (ADCS) of the KITSAT-1 does 
not give sufficiently accurate attitude information because it cannot have attitude sensors enough to do it due to the 
strict limitation of weight and volume like many other micro-satellites. Since many systematic geometric correction 
mechanisms developed previously use fully accurate attitude information, they could not be appropriate for images from 
micro-satellites such as the KITSAT-1. A new mechanism described here estimates attitude and position information 
reversibly using ground control points selected from satellite images and maps. Then, It establishes a geometric model 
based on the estimated information. This paper describes the procedure to perform geometric correction of the KITSAT- 
1 CCD earth images and shows the result from this mechanism. 
[A] 
(&m, Bm) 
9, T] 
01,02,03 
(Xm, ym) 
A 
B 
C1 
C2 
C3 
C4 
C 
Lco 
Lca 
L 
M 
R 
R23 
Nomenclature 
the nth element of a matrix A. 
the coordinates of the mth map ground control 
points 
the longitude and latitude of satellite ground 
position in C4 system 
satellite attitude parameters, rotation angles for 
three axis : 
the coordinates of the mth image ground control 
points 
a point on the CCD sensor 
a point on the center of the lens 
the coordinate system defined on the CCD 
sensor 
the coordinate system defined on the satellite 
the coordinate system defined on the orbit 
the coordinate system defined on the Earth 
a point on the surface of the Earth 
the L vector expressed in C2 system 
the L vector expressed in C4 system 
a vector from the point A to the point B 
a vector from the point B to the point C 
the radius of the Earth 
a rotation matrix between C2 system and C3 
system 
a rotation matrix between C3 system and C4 
system 
the focal length of the lens 
satellite altitude 
the next predicted parameters from the current 
ones. 
International Archives of Photogrammetry and Remote Sensing. Vol. XXXI, Part B3. Vienna 1996 
Pn the current estimated parameters 
p a vector including six geometric model 
parameters (64, 62, 63, à, N, h) 
1. Introduction 
The KITSAT-1, an experimental microsatellite, was 
launched successfully on Oct. 10, 1992 by Ariane v52. Its 
total mass is about 48.6 Kg and its dimension is 35.2 x 
35.6 x 67.0 cm“. Four payloads are on board it to carry 
out scientific and engineering experiments. They are CCD 
Earth Image Experiment (CEIE), Digital Signal Processing 
Experiment (DSPE), Cosmic Ray Experiment (CRE), and 
Digital Store and Forward Communication Experiment 
(DSFCE). All the payloads have worked well without any 
failure and shown interesting results so far.(Kim et. 
al,1993)(Lee et. al., 1993) 
The CEIE consists of two different camera systems and a 
transputer based image processing system. The CCD 
camera systems use two aerial CCD sensor and capture 
meteorological scale monochrome images in a 568x576 
pixel format. One of them has a wide view angle(96°) and 
low resolution(4 kmx4 km per pixel). The other has a 
narrow view angle(12°) and high resolution(400mx400m 
per pixel).(Yoo, 1994) 
Since the KITSAT-1 was launched, the CEIE has taken of 
more than 500 images world-wide so far. However, some 
of them include abnormalities due to hardware and also 
many images have much cloud cover. Consequently, 
about 150 images were used for developing this 
geometric correction mechanism. 
429 
MSc E MERE ASIE E Lcd Mh S US 
  
SE 
 
	        
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