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chapter 5, Imaging Introduction

Author(s): William L. Wolfe
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Chapter Contents

  • 5.1 The Field of View
  • 5.2 Scanners
  • 5.3 Strip Mappers
  • 5.4 Pushbroom Scanners
  • 5.5 Whiskbroom Scanners

Excerpt

Since this text discusses imaging spectrometers, it is necessary that some of the basics of imaging be explored. Two types of images may be defined: a two-dimensional, fixed, rectangular frame and a strip map that is two dimensional but with one dimension arbitrarily long.

5.1 The Field of View

The field of view may be considered as a collection of picture elements (pixels) or resolution elements (reselms). This field can be imaged onto an array of detector elements in a focal plane array (FPA), or it may be imaged by a single detector or small array that is scanned over the field.

I will call the field elements pixels, whether they are measured in linear or angular dimensions. The linear pixel is sometimes called a GSD, for ground spatial distance. The individual detector elements will be called elements. The FPA may be viewed as an array of detector elements, and the idea is to obtain a one-to-one, linear mapping of the pixels onto the elements—or the elements onto the pixels. If there are as many detector elements in the array as there are pixels in the field of view, then the system is called a starer. If not, then some scanning is necessary, and it is called a scanner. The field of view is illustrated in Fig. 5.1.

The required electronic bandwidth for such a system is determined by the Shannon sampling theorem, and is

math
where the bandwidth is B, the dwell time on a pixel is td, Nv and Nh are the number of pixels and mv and mh are the number of detector elements in the vertical and horizontal directions, and tf is the frame time. In a staring system, the dwell time is equal to the frame time tf.



©1997 Society of Photo-Optical Instrumentation Engineers
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BOOK DATA

Print ISBN:

9780819422606

Print ISBN:

0819422606

eISBN:

9780819478542

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