Wavelength dependence of dust aerosol single scattering albedo as observed by the Compact Reconnaissance Imaging Spectrometer

By Michael J. Wolff, Michael D. Smith, R. Clancy, R. Arvidson, M. Kahre, Frank P. Seelos, Scott L. Murchie, H. Savijärvi. 2009

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Subfields: Astronomy and Astrophysics, Atmospheric Science, Global and Planetary Change

View Paper: https://www.semanticscholar.org/paper/30b80cfd731fd97b1283caddae661edc3b6be334

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Citations in the corpus

THE MARTIAN ATMOSPHERIC BOUNDARY LAYER (2011, background): “These properties have been mapped globally and locally with a wide set of instruments on several missions, such as MGS TES [Clancy et al., 2003; Wolff et al., 2006], MEx Observatoire pour la Minéralogie, l’Eau, les Glaces et l’Activité (OMEGA) [Vincendon et al., 2007; Määttänen et al., 2009], and MR”
Compact Reconnaissance Imaging Spectrometer for Mars investigation and data set from the Mars Reconnaissance Orbiter's primary science phase (2009, background): “…of EPF measurements acquired during the ''2007 global dust event'' reveals that atmospheric dust has a higher single scattering albedo than previously assumed, providing up to 10°K less atmospheric heating (depending on altitude) than current global circulation models assume [Wolff et al., 2009].”
The Mars Science Laboratory Curiosity rover Mastcam instruments: Preflight and in‐flight calibration, validation, and data archiving (2017, background): “Initial single-scattering albedo as a function of wavelength was updated to values fromWolff et al. [2009], obtained from orbit under global dust storm conditions.”
Revisiting the radiative impact of dust on Mars using the LMD Global Climate Model (2011, methodology): “[5] Thanks to the numerous new missions of the last decade, many improvements have been made in our knowledge of dust radiative properties, ultimately leading to the retrieval of the fundamental refractive index, both in the visible and infrared regions [Wolff et al., 2006, 2009].”
Compact Reconnaissance Imaging Spectrometer observations of water vapor and carbon monoxide (2009, unknown): “In a similar way, for carbon monoxide we have multiplied all terrestrial broadening coefficients by a constant factor of 1.25 to approximate CO2 broadening of CO [ Varanasi, 1975; Sung and Varanasi, 2005].”
Planetary Spectrum Generator: An accurate online radiative transfer suite for atmospheres, comets, small bodies and exoplanets (2018, background): “aerosols [84], or from the HRI (HITRAN Refractory Index [67]) database.”
Eight-year climatology of dust optical depth on Mars (2014, background): “CDOD retrievals have been obtained from nadir observations at wavelengths centred around 900 nm (Wolff et al., 2009).”
NOMAD, an Integrated Suite of Three Spectrometers for the ExoMars Trace Gas Mission: Technical Description, Science Objectives and Expected Performance (2018, methodology): “The refractive indexes that are adopted for the Mie computation are from Warren and Brandt (2008) for H 2 O ice, from Wolff et al. (2009, 2010) for Martian dust and from Hansen (1997, 2005) for CO 2 ice.”
The Atmospheric Chemistry Suite (ACS) of Three Spectrometers for the ExoMars 2016 Trace Gas Orbiter (2018, methodology): “The refraction index was taken from Wolff et al. (2009) and Ockert-Bell et al. (1997).”