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각 영상별 칩 개수는 Table 3에 제시된 바대로 아리랑 3호의
경우 약 140여개, 아리랑 2호의 경우 108개에서 139개이다.

아리랑 3호의 경우 영상의 면적이 더 크기 때문에 보다 많은
라이다 칩이 포함된 이유이다.
Fig. 영상 범위가 라이다 데이터의 영역보다 크기 때문에
라이다 칩 매칭점 분포도가 아리랑 2호의
경우에 비해 상대적으로 좋지 않다. Fig. 7(a)와 (b)는 아리랑 2호의 경우를 나타낸 것으로서, 좌측
하단부의 경우 Fig. A0, A1, A2 와 B0, B1, B2 : coefficients of the affine model for shift, drift and systematic
errors, l, s : the computed image coordinates of a point (sample and line),
l′, s′ : the correct coordinates of the point. 2)와 같이 구성되어 있으며, 분모는 두 영상에서 추출되는
에지 픽셀의 총 수의 합계를 나타내고, 분자는
두 영상 모두에서 에지인 픽셀의 총 수이다.

즉, 라이다 점밀도가 1제곱미터당 3포인트인 경우에는 3번이 아닌 1번의
영상 투영을 수행하므로 연산시간을 1/3로 절감할 수 있다.

Fig. 7에서는 각각의 영상 영역 내에서 라이다 칩이 매칭이 성공한
위치를 사각형으로 나타내었고 , 검사점의 위치 및 오차를 삼각형과 화살표로 나타내었다 .
3에 나타낸 바와 같이 총 182개의 구&#54925전체 영역
대비 약 24&#65285이 라이다 칩으로 선택되어 저장되었다 .
반사강도 정보를 가지고 있는 라이다 칩은 같이 저장된 수치표고모 델의
높이값을 이용하여 고해상도 위성영상 공간으로 투영된다.
쉽게 말해 벡터형태인 라이다 포인트 별
반사강도 정보를 이용하여 설정된 공간해상도 로 래스터화하 는 것이다.

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