N Souaidia

Comparison of laser-based and conventional calibrations of sun photometers

Sun photometers are used to characterize the radiative properties of the atmosphere. They measure both the incident solar irradiance as well as the sky radiance (from scattered incident flux). Global networks of sun photometers provide data products such as aerosol optical thickness derived from these measurements. Instruments are typically calibrated for irradiance responsivity by cross-calibration against a primary reference sun photometer and for radiance responsivity using a lamp-illuminated integrating sphere source. A laser-based facility for Spectral Irradiance and Radiance Responsivity Calibrations using Uniform Sources (SIRCUS) has been developed at the National Institute of Standards and Technology. Sensors can be calibrated in this facility for absolute spectral irradiance and radiance responsivity with combined expanded (k = 2) uncertainties ranging from 0.15% to 0.25%. Two multi-channel filter radiometers used in the Sensor Intercomparison and Merger for Biological and Interdisciplinary Oceanic Studies (SIMBIOS) program of the National Aeronautics and Space Administration (NASA) at the Goddard Space Flight Center (GSFC) were calibrated for radiance and irradiance responsivity using conventional approaches and using laser-illuminated integrating spheres on SIRCUS. The different calibration methods are compared, the uncertainties are evaluated, and the impact on remote sensing applications is discussed.

Stray light and ocean-color remote sensing

Instruments used to make radiometric measurements of the ocean are typically calibrated against incandescent sources with a spectral distribution that peaks in the near-infrared while the radiant flux from the ocean peaks in the blue to green spectral region. Because of the different spectral distributions between the calibration source and the ocean color, stray light (or spectral out-of-band) in an instruments response can cause significant systematic errors in the measurement of optical properties of the ocean. Approaches to the stray-light characterization and correction of instrumentation used to develop remotely sensed ocean color data products are presented in this work. The goal is to reduce the variance in radiometric measurements of ocean color to produce more consistent long-term, multi-sensor (both ground- and satellite-based) data sets that may lead to increased understanding of bio-physical processes in the oceans.