Optical Payloads for Space Missions
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Optical Payloads for Space Missions

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eBook - ePub

Optical Payloads for Space Missions

About this book

Optical Payloads for Space Missions is a comprehensive collection of optical spacecraft payloads with contributions by leading international rocket-scientists and instrument builders.

  • Covers various applications, including earth observation, communications, navigation, weather, and science satellites and deep space exploration
  • Each chapter covers one or more specific optical payload
  • Contains a review chapter which provides readers with an overview on the background, current status, trends, and future prospects of the optical payloads
  • Provides information on the principles of the optical spacecraft payloads, missions' background, motivation and challenges, as well as the scientific returns, benefits and applications

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Part One
Overview

1
Review of Spaceborne Optical Payloads

Shen-En Qian

1.1 Introduction

The objectives of a space mission are accomplished by the hardware (i.e., instruments) and software, which are referred to as payloads, onboard the platform of a spacecraft. Payloads sense or interact with the subject, are typically unique to each mission, and are the fundamental reason that the spacecraft is flown. The purpose of the rest of the subsystems is to keep the payloads healthy, happy, and pointed in the right direction. The payloads largely determine the mission’s cost, complexity, and effectiveness. A critical part of a mission analysis and design is to understand what drives a particular set of payloads so that these demands can become part of the overall system trade process designed to meet mission objectives at minimum cost and risk.
Payloads of space missions can be roughly classified into two categories in terms of the wavelength of their operating: optical and microwave. Optical payloads, or sensors, measure reflective light in wavelength range from ultraviolet, visible, to infrared (including near infrared, intermediate infrared, thermal infrared), while microwave sensors measure microwaves whose wavelength is longer than visible light and infrared (IR) rays. Microwaves are radio waves with wavelengths ranging from as long as 1 m to as short as 1 mm, or equivalently, with frequencies between 300 MHz (0.3 GHz) and 300 GHz. The observation of microwave sensors is not affected by day, night, or weather. Radar sensors and synthetic aperture radar (SAR) sensors are the typical microwave sensors.
There are two types of observation methods for both optical and microwave payloads: passive and active. Passive payloads detect and measure natural radiation that is emitted or reflected by the objects or surrounding area being observed. Reflected sunlight is the most common source of radiation measured by passive sensors. Active sensors, on the other hand, emit energy in order to scan the area of objects and then detect and measure the radiation that is reflected or backscattered from the objects. Radar and lidar sensors are active sensors, where the time delay between emission and return is measured, establishing the location, height, speed, and direction of an object.
The focus of this book is optical payloads for space missions. Radar payloads are beyond the scope of this book.
Optical payloads can be roughly classified into following six types based on their functions:
  1. Panchromatic sensors
  2. Multispectral sensors
  3. Imaging spectroscopy sensors
  4. Fourier transform spectroscopy sensors
  5. Light detection and ranging (lidar) sensors
  6. Spectrometers and radiometers
This book consists of eight parts (Part OnePart Eight) and covers all these six types of optical payloads. Part One (Chapter 1) is the overview of spaceborne optical sensors. Parts Two through Six each describe one type of optical sensors except for the panchromatic sensors, which are included in Part Two or Part Three together with their hyperspectral or multispectral sensors onboard the same platform. Part Seven describes spaceborne optical sensors other than these six types. Part Eight describes optical sensors onboard microsatellites and nanosatellites.

1.1.1 Panchromatic Sensors

Panchromatic refers to black and white imagery exposed by all visible light. However, a spaceborne panchromatic sensor often acquires visible light within a wavelength range typically between 0.50 and 0.80 μm using a minus blue filter to reduce the scattering that occurs in the blue wavelengths. A panchromatic sensor produces images with a much finer ground footprint size (or spatial resolution) than those produced by the multispectral sensor or hyperspectral sensor onboard the same satellite. For example, the QuickBird satellite produces panchromatic imagery having a ground footprint size of 0.6 m × 0.6 m, while the multispectral pixels represent an area of 2.4 m × 2.4 m.

1.1.2 Multispectral Sensors

Unlike a panchromatic sensor that records the total intensity of radiation falling on each pixel and generates only a panchromatic image, a multispectral sensor acquires multiple images of the scene simultaneously at specific spectral bands, or wavelength ranges. Multispectral images acquired by multispectral sensors are the main type of remote sensing images. Usually, a multispectral sensor has three or more spectral imagers (Landsat 7 has seven). Each one is a scene image in a band of visible spectra, ranging from 0.4 μm to 0.7 μm, called red (635–700 nm), green (490–560 nm), and blue (450–490 nm) (RGB) region, and going to IR wavelengths of 0.8 μm to 10 μm or longer, classified as near infrared (NIR), middle infrared (MIR), and far infrared (FIR or thermal). In the case of Landsat 7, the acquired images comprise seven-band multispectral images. A list of spaceborne multispectral sensors together with their satellite platforms and detailed technical information can be found in Table 1.1 of Reference 1.
Table 1.1 Summary of Optical payloads collected in the book
No.Ch.Payload TypePayload nameAcronym namePlatform or MissionLaunch yearActive? (in Dec. 2014)Country
12Imaging Spectroscopy SensorHyperspectral Imager for the Coastal OceanHICOInternational Space Station2009until Sept. 2014DoD, USA
23Moderate Resolution Imaging SpectroradiometerMODISTerra, Aqua1999, 2002YesNASA, USA
34Medium Resolution Imaging Spectrometer for Ocean ColorMERISENVISAT2002Until 2012ESA
45Visible and Near-infrared Imaging SpectrometerVNISChang’E 32013YesChina
56Hyperspectral Imager HySIHySIIMS-12008YesIndia
67Environmental Mapping and Analysis ProgramEnMapEnMap2018Germany
78PRecursore IperSpettrale della Missione ApplicativaPRISMAPRISMA2017Italy
89Hyperspectral Imager SuiteHISUIHISUI2018Japan
910Ocean and Land Color ImagerOLCISentinel–32015ESA
1011Spaceborne Hyperspectral Applicative Land and Ocean MissionSHALOMSHALOM2020Israel
1112Hyperspectral and Luminescence ObserverHALOMars RoverCanada
1213Multispectral SensorInfrared ScannerIRSHJ-1-B2008YesChina
1314MUX Multispectral CameraMUXCAMCBERS 42014YesBrazil
1415Multispectral camera MXMXIMS-12008YesIndia
1516WFI Wide Field ImagerWFICAMCBERS 42014YesBrazil
1617Remote Sensing InstrumentRSIFORMOSAT-22004YesROC
(Taiwan)
1718Fourier Transform SpectrometerWIND Imaging InterferometerWINDIINASA UARS1991Until 2003Canada
1819Atmospheric Chemistry Experiment - Fourier Transform SpectrometerACE-FTSSCISAT2003YesCanada
1920Cross-track Infrared SounderCrISSuomi NPP/JPSS2011YesNOAA, USA
2021Thermal And Near infrared Sensor for carbon Observation Fourier Transform SpectrometerTANSO-FTSGOSAT2009YesJapan
2122Geostatio...

Table of contents

  1. Cover
  2. Title Page
  3. Table of Contents
  4. Contributors List
  5. Preface
  6. Part One: Overview
  7. Part Two: Imaging Spectrometers
  8. Part Three: Multispectral Sensors
  9. Part Four: Fourier Transform Spectrometers
  10. Part Five: Lidar and Active Sensors
  11. Part Six: Spectrometers and Radiometers
  12. Part Seven: Other Types of Optical Sensors
  13. Part Eight: Nanosatellites and Microsatellites
  14. Index
  15. End User License Agreement

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