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