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
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- 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
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- 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.