Spectral data set factor analysis and end-member recovery: Application to analysis of Martian atmospheric particulates

By J. Bandfield, Philip R. Christensen, Michael D. Smith. 2000

148 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/cd4aea2f3a701b71b0289a89be6ea57bd80cc010

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Aerospace Engineering

1. V. Hamilton
2. Michael D. Smith
3. Philip R. Christensen
4. J. Bandfield
5. W. Koeppen
6. H. McSween
7. Michael J. Wolff
8. R. Clancy

In Astronomy and Astrophysics

1. V. Hamilton
2. Michael D. Smith
3. Philip R. Christensen
4. J. Bandfield
5. W. Koeppen
6. H. McSween
7. Michael J. Wolff
8. R. Clancy

In Atmospheric Science

1. Michael D. Smith
2. V. Hamilton
3. Michael J. Wolff
4. J. Bandfield
5. R. Clancy
6. Philip R. Christensen
7. W. Koeppen
8. S. Ruff

Citations in the corpus

• Constraints on the size of Martian aerosols from Thermal Emission Spectrometer observations (2003, methodology): “[56] The TES team optical depth retrieval process employs a single wavelength dependence or ‘‘shape’’ of the surface emissivity, which is representative of the typical southern hemisphere basaltic surface [Bandfield et al., 2000; Smith et al., 2000b].”
• Constraints on dust aerosols from the Mars Exploration Rovers using MGS overflights and Mini‐TES (2006, methodology): “ Bandfield et al., 2000; Smith et al., 2000].”
• Global mapping of Martian hematite mineral deposits: Remnants of water‐driven processes on early Mars (2001, background): “…the surface and atmospheric components of the radiance from Mars, which allows detailed analysis and interpretation of surface mineralogy [Christensen et al., 2000b; Bandfield et al., 2000a; Christensen et al., 2000c], is described previously by Smith et al. [2000] and Bandfield et al. [2000b].”
• Identification of quartzofeldspathic materials on Mars (2004, methodology): “[19] The deconvolution surface-atmosphere separation also provides areal mineral and spectral unit abundances that can be used for compositional analysis [Smith et al., 2000; Bandfield et al., 2000a; Bandfield, 2002; Hamilton et al., 2003].”
• Global distribution, composition, and abundance of olivine on the surface of Mars from thermal infrared data (2008, methodology): “The atmospheric dust and water ice spectral shapes derived from TES data by target transformation are relatively invariant except for some features attributed to CO2 and H2O gas [ Bandfield et al., 2000a ], and they can be used as spectral end-members in the deconvolution algorithm to simultaneously”
• Bright and dark regions on Mars: Particle size and mineralogical characteristics based on thermal emission spectrometer data (2002, methodology): “To date, surface studies using TES spectra have focused on dark regions, where basalt, basaltic andesite, and hematiterich materials have been identified [Bandfield et al., 2000a; Christensen et al., 2000a, 2000b].”
• Global mineral distributions on Mars (2002, methodology): “Global mapping revealed two major distinct spectral units within Martian low-albedo regions [Bandfield et al., 2000a].”
• Interannual variability in TES atmospheric observations of Mars during 1999–2003 (2004, methodology): “nadir and emission phase function (EPF) data (Smith et al., 2000b; Bandfield et al., 2000a; Bandfield and Smith, 2003).”