THE SUFFICIENT AREA CONDITION OF AN OBJECT FOR A SPOT- DETECTOR
F. Cheng* and Ph. Hartl
Institute for Navigation, University of Stuttgart, Stuttgart, Germany
KEY WORDS: SPOT-pixel, spatial resolution
ABSTRACT:
Some objects can not be found or identified on a SPOT-image due to their too small areas. An Object on the ground
must be large enough so that it can be detected vertically by a SPOT-detector and recorded as a complete pixel in a
SPOT-image. This condition, defined as the sufficient area condition, has been not studied yet. In this paper the
condition is theoretically analysed and quantitatively calculated. It may be expressed as follows: 1) the area of an object
on the ground must include an ellipse, whose long axis e, is in the direction with the greatest ground slope € and
equal to 2R/ cos€ , and whose short axis e, is horizontal and equal to 2R; 2) if the ground is smooth (€ =0), the
ellipse becomes a circle with the radius R. Here R is the diagonal length of a SPOT-image's pixel: 10/2 m or 20/2 m.
1. INTRODUCTION
Some objects can not be found or identified on a SPOT-
image due to their too small areas. How large should the
area of an object on the ground be, so that it can be
detected at least by a SPOT-detector? Many people
have met such a question in their works, especially in
classifying or identifying objects on satellite images.
Some of them hope to use satellite data with smaller pixel
size or higher spatial resolution in order to obtain better
results (Begni 1988, Dowman et al 1989, Moore et al
1989, Jensen et al 1993, Manavalan et al 1993, Cheng et
al 1995, Hartl et al 1995).
There are two types of SPOT-images: vertical and oblique
viewing images. Here only the former is discussed. The
area of an object on the ground, which makes the object
to be vertically detected at least by a SPOT-detector and
be recorded as a complete pixel in a SPOT-image, is
defined as the sufficient area condition. This paper shows
the study of the condition and gives its mathematical
expression.
2. THE SUFFICIENT AREA CONDITION
ON THE SMOOTH GROUND
2.1 Position change of grids
The figure 1 shows a square grid, which represents the
corresponding area of a SPOT-detector on the smooth
ground. Here we call it a SPOT-detector-grid (G- side
length; d- diagonal length). Suppose that there is a
circular object C, with the radius R on the ground. On
the object a Cartesian coordinate system oxy is set up,
whose origin o is at the center of the object and whose y-
axis points north. Suppose that the center of a SPOT-
detector-grid (p) is just overlapped with the object's center
and f,, f,, ...f, are the eight neighbour grids of the grid
p (figure 2). In this situation the object can be detected at
"Present address: Company for applied Remote Sensing
(GAF), 80636 Munich, Germany
36
least by a complete SPOT-detector-grid, if its radius R
meets the following condition:
gaz 1
2 t (1)
This is a special situation. But it may be supposed that
the grids' position shown in the figure 2 is the original
position. The position of the grids on the ground generally
changes after a revolving period of the satellite. The
figure 3(1) shows such a change. The grids have left the
original position in a new revolving period. We may only
consider the position change of the grid p instead of all
the grids, because the relative position between the
different grids is fixed. The position change of the grid p
shown in the figure 3(1) can be resolved into a shift and a
turn around the origin o. i) The grid p shifts first from o to
p' and then ii) it turns around o from p' to p" (figure 3(2)).
In fact any position change of the grids can be resolved
as above.
Suppose that the grid p shifts first from the original
position (0,0) to an other position (xp, yp) (figure 4(1)). The
shift amount is equal to the distance between the two
points. We define X as the component of this distance
on the x-axis and Y as its component on the y-axis. Then
the following equalities are tenable: X =Ixp| and Y =lypl.
In the situation shown in the figure 4(1) the object C, can
be detected by a complete SPOT-detector-grid, if its
radius R meets:
a: 22 ap
R=] Cre ++) | (2)
See the figure 4(2). The grid p turns around o in the
next revolving period of the satellite. Then R should
meet:
2
[ a ie. ti
R= (X3 cos p + +3) sin p | +
2
are) X42) si
( 3 cos p — ( +2) sin p
2
International Archives of Photogrammetry and Remote Sensing. Vol. XXXI, Part B1. Vienna 1996
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