Collection Information
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IDENTIFIER |
urn:nasa:pds:mgs_tes_atmos_dust-ice:data_derived_vis-dust-optical-depth::1.0
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NAME |
MGS TES Visible Column Dust Optical Depth Derived Data Collection
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TYPE |
Data
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DESCRIPTION |
Atmospheric visible column dust optical depths retrieved from MGS TES observations. Visible optical depths are retrieved from solar band emergence phase function sequences and reported at a reference wavelength of 0.67 micron.
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SEARCH/ACCESS DATA |
Mars Global Surveyor (MGS) Thermal Emission Spectrometer (TES) Atmospheric Column Optical Depths for Dust and Water Ice Online
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Citation |
DIGITAL OBJECT IDENTIFIER (DOI) |
10.17189/kwez-jq47 (from parent bundle)
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AUTHOR LIST |
Montabone, L., Smith, M., Wolff, M., Cantor, B.
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EDITOR LIST |
Neakrase, L., Huber, L.
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PUBLICATION YEAR |
2023
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DESCRIPTION |
Atmospheric visible column dust optical depths retrieved from MGS TES observations. Visible optical depths are retrieved from solar band emergence phase function sequences and reported at a reference wavelength of 0.67 micron.
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Context |
START DATE TIME |
1999-03-12T03:47:53.149Z
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STOP DATE TIME |
2004-08-28T08:24:47.998Z
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LOCAL MEAN SOLAR TIME |
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LOCAL TRUE SOLAR TIME |
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SOLAR LONGITUDE |
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PRIMARY RESULT PURPOSE |
SCIENCE
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PRIMARY RESULT PROCESSING LEVEL |
Derived
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PRIMARY RESULT DESCRIPTION |
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PRIMARY RESULT WAVELENGTH RANGE |
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PRIMARY RESULT DOMAIN |
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PRIMARY RESULT DISCIPLINE NAME |
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INVESTIGATION |
MARS GLOBAL SURVEYOR
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OBSERVING SYSTEM |
MGS
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OBSERVING SYSTEM COMPONENT |
MGS
TES
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TARGET |
MARS
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REFERENCES |
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