IGARSS 2020 - 2020 IEEE International Geoscience and Remote Sensing Symposium 2020
DOI: 10.1109/igarss39084.2020.9323176
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Clarreo Pathfinder: Mission Overview and Current Status

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Cited by 25 publications
(21 citation statements)
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“…The SBG VSWIR reference orbit remained the same as Scenario One, Two, and Three. CLARREO-Pathfinder will operate on the International Space Station (ISS) at an altitude of approximately 400 km with an inclination of 52° with a swath width of 70 km (Shea et al, 2020; https://clarreo-pathfinder.larc.nasa.gov/mission-overview/; https://www.eoportal.org/satellite-missions/iss-clarreo#mission-capabilities) while SBG VSWIR is at an inclination of approximately 98°. The orbital planes of these two missions are nearly perpendicular and result in The SBG CVWG orbital simulations for SBG VSWIR and TIR instruments reveal some key findings regarding inter-calibration among cooperating missions for enabling science quality data.…”
Section: Scenario Five: Descending Sbg Vswir and International Space ...mentioning
confidence: 99%
“…The SBG VSWIR reference orbit remained the same as Scenario One, Two, and Three. CLARREO-Pathfinder will operate on the International Space Station (ISS) at an altitude of approximately 400 km with an inclination of 52° with a swath width of 70 km (Shea et al, 2020; https://clarreo-pathfinder.larc.nasa.gov/mission-overview/; https://www.eoportal.org/satellite-missions/iss-clarreo#mission-capabilities) while SBG VSWIR is at an inclination of approximately 98°. The orbital planes of these two missions are nearly perpendicular and result in The SBG CVWG orbital simulations for SBG VSWIR and TIR instruments reveal some key findings regarding inter-calibration among cooperating missions for enabling science quality data.…”
Section: Scenario Five: Descending Sbg Vswir and International Space ...mentioning
confidence: 99%
“…The uncertainties chosen to evaluate in this study include uncertainty levels of previous and operational Earth‐viewing sensors and uncertainty levels that will be achieved by future systems. For example, the Climate Absolute Radiance and Refractivity Pathfinder (CLARREO Pathfinder) (Shea et al., 2020) and Traceable Radiometry Underpinning Terrestrial‐ and Helio‐Studies (TRUTHS) (Fox et al., 2011) reflected solar spectrometers are being designed to have a 0.3% ( k = 1) and 0.3% ( k = 2) uncertainty in reflectance, respectively. The Ocean Color Instrument that is part of the Plankton, Aerosol, Cloud, ocean Ecosystem (PACE) mission (Werdell et al., 2019) is being designed to achieve 0.5% ( k = 1) uncertainty.…”
Section: Observed and Simulated Reflectancementioning
confidence: 99%
“…The credible expectation for ACCP is that a hyperspectral solar measurement implementation ought to be in the form of a small class sensor. In the coming years, the CLARREO pathfinder (CPF; Shea et al, 2020) plans to provide traceable, accurate spectra by direct solar calibration; see Kopp et al, (2017) against which other observing systems would be benchmarked. The characteristics of the proposed ACCP spectrometer is expected to largely duplicate those of the CPF.…”
Section: Vswir Spectrometry In the Accp Eramentioning
confidence: 99%