Table information for 'omega_cubes.epn_core'

General

Table Description: Mars Express - Omega Cubes

This table is available for ADQL queries and through the TAP endpoint.

Resource Description: *** PSUP Omega Cubes *** The database contains all the OMEGA observations acquired with the C channel. Filtering processes have been implemented to remove some instrumental artefacts and observational conditions. OMEGA C channel data cubes are corrected for atmospheric and aerosol contributions. OMEGA is the spectro-imaging instrument of the ESA Mars-Express mission, inserted on the martian orbit the 25th of December 2003. The Observatories of Paris Sud (OSUPS) and Lyon (OSUL) have implemented a portal,called PSUP (Planetary SUrface Portal), for providing users with efficient and easy access to data products dedicated to the Martian surface. *** Scientific interest ***

For a list of all services and tables belonging to this table's resource, see Information on resource 'L3 Omega Cubes - Mars Express'

Resource Reference URL: http://psup.ias.u-psud.fr

Citing this table

To cite the table as such, we suggest the following BibTeX entry:

@MISC{vo:omega_cubes_epn_,
  year=2018,
  title={L3 Omega Cubes - Mars Express},
  author={{IDOC}},
  url={https://idoc-dachs.ias.u-psud.fr/tableinfo/omega_cubes.epn_core},
  howpublished={{VO} resource provided by the {IDOC}: Integrated Data and Operating Center}
}

Columns

Sorted by DB column index. [Sort alphabetically]

NameTable Head DescriptionUnitUCD
granule_uid Granule_uid Internal table row index, which must be unique within the table. Can be alphanumeric. N/A meta.id
granule_gid Granule_gid Common to granules of same type (e.g. same map projection, or geometry data products). Can be alphanumeric. N/A meta.id
obs_id Obs_id Associates granules derived from the same data (e.g. various representations/processing levels). Can be alphanumeric, may be the ID of original observation. N/A meta.id;obs
dataproduct_type Dataproduct_type The high-level organization of the data product, from a controlled vocabulary (e.g., 'im' for image, sp for spectrum). Multiple terms may be used, separated by # characters. [Note et_prod] N/A meta.code.class
target_name Target_name Standard IAU name of target (from a list related to target class), case sensitive N/A meta.id;src
target_class Target_class Type of target, from a controlled vocabulary. N/A src.class
time_min Time_min Acquisition start time (in JD), as UTC at time_refposition d time.start;obs
time_max Time_max Acquisition stop time (in JD), as UTC at time_refposition d time.end;obs
time_sampling_step_min Time_sampling_step_min Sampling time for measurements of dynamical phenomena, lower limit. s time.resolution;stat.min
time_sampling_step_max Time_sampling_step_max Sampling time for measurements of dynamical phenomena, upper limit s time.resolution;stat.max
time_exp_min Time_exp_min Integration time of the measurement, lower limit. s time.duration;obs.exposure;stat.min
time_exp_max Time_exp_max Integration time of the measurement, upper limit s time.duration;obs.exposure;stat.max
spectral_range_min Spectral_range_min Spectral range (frequency), lower limit. Hz em.freq;stat.min
spectral_range_max Spectral_range_max Spectral range (frequency), upper limit Hz em.freq;stat.max
spectral_sampling_step_min Spectral_sampling_step_min Spectral sampling step, lower limit. Hz em.freq;spect.binSize;stat.min
spectral_sampling_step_max Spectral_sampling_step_max Spectral sampling step, upper limit Hz em.freq;spect.binSize;stat.max
spectral_resolution_min Spectral_resolution_min Spectral resolution, lower limit. N/A spect.resolution;stat.min
spectral_resolution_max Spectral_resolution_max Spectral resolution, upper limit N/A spect.resolution;stat.max
c1min C1min Longitude on body, lower limit. deg pos.bodyrc.lon;stat.min
c1max C1max Longitude on body, upper limit deg pos.bodyrc.lon;stat.max
c2min C2min Latitude on body, lower limit. deg pos.bodyrc.lat;stat.min
c2max C2max Latitude on body, upper limit deg pos.bodyrc.lat;stat.max
c3min C3min Altitude from reference surface, lower limit. km pos.bodyrc.alt;stat.min
c3max C3max Altitude from reference surface, upper limit km pos.bodyrc.alt;stat.max
s_region S_region ObsCore-like footprint, valid for celestial, spherical, or body-fixed frames N/A pos.outline;obs.field
c1_resol_min C1_resol_min Resolution in the first coordinate, lower limit. deg pos.angResolution;stat.min
c1_resol_max C1_resol_max Resolution in the first coordinate, upper limit deg pos.angResolution;stat.max
c2_resol_min C2_resol_min Resolution in the second coordinate, lower limit. deg pos.angResolution;stat.min
c2_resol_max C2_resol_max Resolution in the second coordinate, upper limit deg pos.angResolution;stat.max
c3_resol_min C3_resol_min Resolution in the third coordinate, lower limit. km pos.resolution;stat.min
c3_resol_max C3_resol_max Resolution in the third coordinate, upper limit km pos.resolution;stat.max
spatial_frame_type Spatial_frame_type Flavor of coordinate system, defines the nature of coordinates. From a controlled vocabulary, where 'none' means undefined. N/A meta.code.class;pos.frame
incidence_min Incidence_min Incidence angle (solar zenithal angle) during data acquisition, lower limit. deg pos.incidenceAng;stat.min
incidence_max Incidence_max Incidence angle (solar zenithal angle) during data acquisition, upper limit deg pos.incidenceAng;stat.max
emergence_min Emergence_min Emergence angle during data acquisition, lower limit. deg pos.emergenceAng;stat.min
emergence_max Emergence_max Emergence angle during data acquisition, upper limit deg pos.emergenceAng;stat.max
phase_min Phase_min Phase angle during data acquisition, lower limit. deg pos.phaseAng;stat.min
phase_max Phase_max Phase angle during data acquisition, upper limit deg pos.phaseAng;stat.max
instrument_host_name Instrument_host_name Standard name of the observatory or spacecraft N/A meta.id;instr.obsty
instrument_name Instrument_name Standard name of instrument N/A meta.id;instr
measurement_type Measurement_type UCD(s) defining the data, with multiple entries separated by hash (#) characters. N/A meta.ucd
processing_level Processing_level Dataset-related encoding, or simplified CODMAC calibration level [Note et_cal] N/A meta.calibLevel
creation_date Creation_date Date of first entry of this granule N/A time.creation
modification_date Modification_date Date of last modification (used to handle mirroring) N/A time.processing
release_date Release_date Start of public access period N/A time.release
service_title Service_title Title of resource (an acronym really, will be used to handle multiservice results) N/A meta.title
access_url Access_url URL of the data file, case sensitive. If present, then access_format and access_estsize are mandatory. N/A meta.ref.url;meta.file
access_format Access_format File format type (RFC 6838 Media Type a.k.a. MIME type) N/A meta.code.mime
access_estsize Access_estsize Estimated file size in kbyte. kbyte phys.size;meta.file
file_name File_name Name of the data file only, case sensitive N/A meta.id;meta.file
publisher Publisher A short string identifying the entity running the data service used N/A meta.curation
orbit_number orbit_number The martian orbit number. N/A meta.id
cube_number cube_number The cube number on the specified orbit_number, depends on pixel numbers before projection. N/A meta.id
altitude_min altitude_min The miminum altitude (in m) (MOLA ? ellipsoid as reference). m pos.bodyrc.alt;stat.min
altitude_max altitude_max The maximum altitude (in m) (MOLA ? ellipsoid as reference). m pos.bodyrc.alt;stat.max
watericelin_min watericelin_min The minimum watericelin index value. This criterion, described in Langevin et al. (2007) is based on the 1.5 ?m band depth. It can be used to detect icy frost presence at the surface and thick clouds in the atmosphere. Every OMEGA pixel with a watericelin value > 1.5% should be excluded. N/A meta.id;stat.min
watericelin_max watericelin_max The maximum watericelin index value. This criterion, described in Langevin et al. (2007) is based on the 1.5 ?m band depth. It can be used to detect icy frost presence at the surface and thick clouds in the atmosphere. Every OMEGA pixel with a watericelin value > 1.5% should be excluded. N/A meta.id;stat.max
icecloud_index_min icecloud_index_min The minimum icecloud index. This criterion (reflectance at 3.4 ?m divided by reflectance at 3.52 ?m) is described in Langevin et al. (2007) to identify the presence of water ice clouds. Its values range from 0.5 to 1.0. The smallest values unambiguously indicate the presence of icy clouds. We usually exclude any OMEGA pixel with a value strictly inferior to 0.8. N/A meta.id;stat.min
icecloud_index_max icecloud_index_max The maximum icecloud index. This criterion (reflectance at 3.4 ?m divided by reflectance at 3.52 ?m) is described in Langevin et al. (2007) to identify the presence of water ice clouds. Its values range from 0.5 to 1.0. The smallest values unambiguously indicate the presence of icy clouds. We usually exclude any OMEGA pixel with a value strictly inferior to 0.8. N/A meta.id;stat.max
tau_min tau_min The minimum effective dust opacity at a given longitude and latitude as τeff = τMER/cos i, where i is the solar incidence angle and τMER is the dust opacity measured by the Mars Exploration Rovers (MERs) during the same solar longitude and Martian year as the OMEGA observation (see Audouard et al. J. Geophys. Res. Planets, 119, 1969–1989 for more details). N/A meta.id;stat.min
tau_max tau_max The maximum effective dust opacity at a given longitude and latitude as τeff = τMER/cos i, where i is the solar incidence angle and τMER is the dust opacity measured by the Mars Exploration Rovers (MERs) during the same solar longitude and Martian year as the OMEGA observation (see Audouard et al. J. Geophys. Res. Planets, 119, 1969–1989 for more details). N/A meta.id;stat.max

Columns that are parts of indices are marked like this.

VOResource

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Notes

Copyright and such: This research have been made using PSUP database at IDOC.