Abstract

Earth remote sensing optical satellite systems are often divided into two categories—geosynchronous and sun-synchronous. Geosynchronous systems essentially rotate with the Earth and continuously observe the same region of the Earth. Sun-synchronous systems are generally in a polar orbit and view differing regions of the Earth at the same local time. Although similar in instrument design, there are enough differences in these two types of missions that often the calibration of the instruments can be substantially different. Thus, respective calibration teams develop independent methods and do not interact regularly or often. Yet, there are numerous areas of overlap and much to learn from one another. To address this issue, a panel of experts from both types of systems was convened to discover common areas of concern, areas where improvements can be made, and recommendations for the future. As a result of the panelist’s efforts, a set of eight recommendations were developed. Those that are related to improvements of current technologies include maintaining sun-synchronous orbits (not allowing orbital decay), standardization of spectral bandpasses, and expanded use of well-developed calibration techniques such as deep convective clouds, pseudo invariant calibration sites, and lunar methodologies. New techniques for expanded calibration capability include using geosynchronous instruments as transfer radiometers, continued development of ground-based prelaunch calibration technologies, expansion of RadCalNet, and development of space-based calibration radiometer systems.

Highlights

  • Two main categories of optical Earth observation satellites are geosynchronous and sun-synchronous

  • Low Earth Orbit (LEO) orbits are ideal for Earth remote sensing because near-polar orbits can be sun-synchronous—that is, the satellite crosses the equator at the same local time during each orbit

  • The results show an excellent agreement with those obtained from direct ray-matching between these two instruments over all-sky tropical ocean scenes

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Summary

Introduction

Two main categories of optical Earth observation satellites are geosynchronous (those that continuously stare at the same area of the Earth’s surface) and sun-synchronous (or polar-orbiting—those that can observe differing areas of the Earth’s surface at the same time each day). The workshop concept was to bring together a panel of experts to discuss capabilities and limitations that define the current practice in the calibration of sun-synchronous and geosynchronous optical remote sensing satellites and to determine a path forward for calibration improvement based on synergies identified between the two groups. Panel members presented their perspectives on the topic and interacted extensively with the goal of producing recommendations useful for both calibration communities, as well as for broader implementation. A set of summary and conclusion statements finishes the paper

Background
Criticality of Maintaining Current Sun-Synchronous Orbit
Spectral Standardization
Expanded DCC-Based Calibration
Extended Pseudo Invariant Calibration Sites Techniques
Improved Lunar Calibration
Methodologies
Cross-calibration of the SNPP and NOAA-20 VIIRS Methodology
Results
Summary of Lunar Calibration Techniques
Using GEO as a Transfer Radiometer
Goddard Laser for the Absolute Measurement of Radiance
RadCalNet Extension
SI Traceable Hyperspectral Sensor Missions
Findings
Discussion
Conclusions
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