Skip to content
Snippets Groups Projects
Commit 5b7a15c7 authored by mendrok's avatar mendrok
Browse files

* ARTS-XML-DATA-2-2-5

	* scattering/README, planets/Venus/SAT/README, planets/Mars/SAT/README:
	READMEs for folders missing them so far.

	* spectroscopy/Perrin_artscat34/README, planets/Venus/MPS/README,
	planets/Mars/MPS/README, planets/Earth/Fascod/README:
	Minor corrections/updates.



git-svn-id: https://radiativetransfer.org/svn/rt/arts-xml-data/branches/arts-xml-data-2.2@9335 aaf1aab0-4228-0410-ad68-8dceda47f409
parent 321eb15f
No related branches found
No related tags found
No related merge requests found
2015-06-17 Jana Mendrok <jana.mendrok@ltu.se>
* ARTS-XML-DATA-2-2-5
* scattering/README, planets/Venus/SAT/README, planets/Mars/SAT/README:
READMEs for folders missing them so far.
* spectroscopy/Perrin_artscat34/README, planets/Venus/MPS/README,
planets/Mars/MPS/README, planets/Earth/Fascod/README:
Minor corrections/updates.
2015-06-17 Jana Mendrok <jana.mendrok@ltu.se> 2015-06-17 Jana Mendrok <jana.mendrok@ltu.se>
* ARTS-XML-DATA-2-2-4 * ARTS-XML-DATA-2-2-4
......
This directory contains planet characterization data (atmospheric profiles, This directory contains planet characterization data (atmospheric profiles,
surface properties, and the like) for Mars surface properties, and the like) for Mars
Mars.meanRefIndex.n.xml Mars.surface_complex_refr_index_field.xml
----------------------- -----------------------
- global field of surface refractive index - global field of surface refractive index
- originating from dielectric constant data (real part only; hence imag. part - originating from dielectric constant data (real part only; hence imag. part
......
This directory contains cloud and dust data (single scattering properties and
particle number density fields) for Mars
Mars.Ls[0,90,180,270].[day,night].dust-[low,medium,high]/*.pnd_field__*.xml
-----------------------
- 1D number density fields for different cloud/dust types and cases
- available for 4 seasons, day/night, and 3 dust loadings (corresponding to
atmospheric cases, except negligible dependence on solar activity; note that
atm case dependence only refers to different p-z-relation during
seasons/daytimes; it does so far NOT consider different cloud/dust conditions
in different seasons/daytimes)
- data created by J. Mendrok (LTU) within ESA Planetary study
- for more details see TechnicalNote3 of the ESA Planetary study
Mars.scat_data__*.xml
-----------------------
- single scattering data for different cloud/dust types and cases
- data created by J. Mendrok (LTU) within ESA Planetary study
- for more details see TechnicalNote3 of the ESA Planetary study
NOTE: single scattering data and number density fields form paired groups, which
are linked by cloud category (CO2ice or H2Oice or Dust) and bulk type (e.g.,
*-size-bulk). within the groups, one can choose different dielectric property
assumptions (RI-*) for the single scattering data and different altitude
distributions (e.g., *-mixed, *-profile) for the number density fields.
See Consolidated Design Document of the ESA Planetary study for details on the
relation of single scattering and number density data and on the file name
layout.
...@@ -2,14 +2,14 @@ This directory contains planet characterization data (atmospheric profiles, ...@@ -2,14 +2,14 @@ This directory contains planet characterization data (atmospheric profiles,
surface properties, and the like) for Venus provided by MPS within ESA Planetary surface properties, and the like) for Venus provided by MPS within ESA Planetary
study. For more details see TechnicalNote2 of the ESA Planetary study. study. For more details see TechnicalNote2 of the ESA Planetary study.
Venus.meanRefIndex.n.xml Venus.surface_complex_refr_index_field.xml
------------------------ ------------------------
- global field of surface refractive index - global field of surface refractive index
- originating from dielectric constant data (real part only; hence imag. part - originating from dielectric constant data (real part only; hence imag. part
set to 0) set to 0)
- for more details see TechnicalNote2 of the ESA Planetary study - for more details see TechnicalNote2 of the ESA Planetary study
Mars.t_surface.xml Venus.t_surface.xml
----------------------- -----------------------
- global field of surface (=skin) temperature - global field of surface (=skin) temperature
- single, mean condition field - single, mean condition field
...@@ -31,7 +31,7 @@ For a couple of reasons finally selected data is taken from a number of differen ...@@ -31,7 +31,7 @@ For a couple of reasons finally selected data is taken from a number of differen
- We need, however consistent, full-coverage (i.e., covering both the vmr and el.dens. regions) z and T data. This is available from the latest (ext*) data sets, hence we get z and T fields from those instead of merging them ourselves from the original data, where vmr/T and el.dens. come with their own z fields. - We need, however consistent, full-coverage (i.e., covering both the vmr and el.dens. regions) z and T data. This is available from the latest (ext*) data sets, hence we get z and T fields from those instead of merging them ourselves from the original data, where vmr/T and el.dens. come with their own z fields.
- In the orginal el.dens. data, there are only 3 sets (day, night, night_cold) instead of the 5 scenarios (vira.day, vira.day_highlat, vira.night, spicav.night, spicav.night_cold) given, and assignment between the 3 and 5 cases is not claer. The latest (ext*) el.dens. data set contains data for all 5 scenarios (though originally sorted into day/ and night/ folders instead of into the 5 scenario folders) and seems to agree well with the T-fields for the different cases (assuming/indicating the el.dens.-over-z is not scenario dependend). Hence, we take the el.dens. fields from the ext* data. - In the orginal el.dens. data, there are only 3 sets (day, night, night_cold) instead of the 5 scenarios (vira.day, vira.day_highlat, vira.night, spicav.night, spicav.night_cold) given, and assignment between the 3 and 5 cases is not clear. The latest (ext*) el.dens. data set contains data for all 5 scenarios (though originally sorted into day/ and night/ folders instead of into the 5 scenario folders) and seems to agree well with the T-fields for the different cases (assuming/indicating the el.dens.-over-z is not scenario dependend). Hence, we take the el.dens. fields from the ext* data.
In the following we document, which version (date) of the individual data is taken: In the following we document, which version (date) of the individual data is taken:
......
This directory contains cloud and haze data (single scattering properties and
particle number density fields) for Venus
Venus.[vira,spicav].[day,day_highlat,night,night_cold]/*.pnd_field__*.xml
-----------------------
- 1D number density fields for different cloud/haze layers, modes, and cases
- available for 5 scenarios from different data sources (VIRA and SPICAV),
for 2 times of day (day,night). note that scenario dependence only refers to
different p-z-relation; it does so far NOT reflect possible different cloud
conditions, e.g., in different daytimes.
- data created by J. Mendrok (LTU) within ESA Planetary study
- for more details see TechnicalNote3 of the ESA Planetary study
Venus.scat_data__*.xml
-----------------------
- single scattering data for different cloud/haze layers and modes
- data created by J. Mendrok (LTU) within ESA Planetary study
- for more details see TechnicalNote3 of the ESA Planetary study
NOTE: single scattering data and number density fields form paired groups, which
are linked by cloud category (H2SO4) and bulk type (layer and mode, *-bulk).
within the groups, one can choose different altitude distributions (*-profile)
for the number density fields.
See Consolidated Design Document of the ESA Planetary study for details on the
relation of single scattering and number density data and on the file name
layout.
This directory data related to running scattering calculations. Major part is
single scattering data for different types of (well-defined) scattering particles.
H2O_liquid/*.xml
-----------------------
- single scattering data (*.um.xml) and corresponding meta data (*um.meta.xml)
- liquid water particles (e.g. for Earth liquid clouds and rain)
- range of sizes (0.1-10,000um), all assumed as spheres
- data created by ARTS developers using atmlab routines (Maetzler's matlab Mie code; dielectric property routines)
- for more details data headers
H2O_ice/*.xml
-----------------------
- single scattering data (*.um.xml) and corresponding meta data (*um.meta.xml)
- water ice particles (e.g. for Earth ice clouds, hail, snow)
- range of sizes (0.1-10,000um), all assumed as solid spheres
- data created by ARTS developers using atmlab routines (Maetzler's matlab Mie code; dielectric property routines)
- for more details data headers
fosangles_360.xml
-----------------------
- set of directions/angles (polar and azimuth angles) for FOS calculations
(radiation path directions)
- directions are equally distributed over the sphere, each representing a solid
angle of 4Pi/360 sr
- data created by P. Eriksson (Chalmers)
SingleScatteringFile_allH2Oice-allH2Oliquid.xml
ScatteringMetaFile_allH2Oice-allH2Oliquid.xml
-----------------------
- list of scattering data and meta data files for use with
ScatteringParticleTypeAndMetaRead
- covers all liquid water and water ice particles (all sizes) given in the
subfolders
This directory contains a spectroscopic line catalogue.
- prepared as part of ESA ESA Planetary Toolbox study. For more information see
the ESA study's Technical Note 3.
- specifically prepared for planetary radiative transfer
- covers data for frequencies <3THz
Species overview Species overview
================ ================
......
0% Loading or .
You are about to add 0 people to the discussion. Proceed with caution.
Please register or to comment