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The atmospheric profile is computed from a combination of input parameters
and physical laws. The shape of the atmosphere density and pressure are
defined by the physical laws (hydrostatic equilibrium + mixture of ideal
gas). The shape of the temperature profile is defined by the following two
parameters.
- Troposperic lapse rate,
- which is used to fix the temperature
gradient up to the tropopause. Its recommanded value is -5.6 K/km.
- Atmospheric type,
- which is used to reproduce the shape of the
temperature profile above the tropopause. For Pico Veleta and Plateau de
Bure, it should be the well defined mid-latitude averaged
profiles for summer and winter. Continuity of the temperature atmospheric
profile is enforced at the tropopause.
The atmospheric model is computed assuming a plane-parallel geometry
defined by the following three parameters.
- Atmospheric upper boundary,
- which is the maximum altitude of the
modeled atmosphere, typically 48 km.
- Primary pressure step,
- which is the pressure step used to define the
height of the first atmospheric layer, typically 10 mb.
- Pressure step factor,
- which is the multiplicative factor used to
define the next pressure step from the current one, typically 1.2.
The atmospheric profile of the minor components is defined by the following
two parameters.
- Water vapor scale height,
- which is used to define the exponential
distribution of water, typically 2 km (could be between 1.5 and 3 km).
- Atmospheric type,
- which is also used to define the profile
repartition of the other minor components (e.g. ozone) of the
atmosphere.
For our applications (calibrating radio-astronomy data), most of these
parameters should have a minor impact (still to be checked). The 3
remaining parameters, i.e. the ground temperature and pressure at the
telescope as well as the amount of precipitable water vapor at zenith, are
used to hook the atmospheric profile defined above to the current
conditions at the telescope site. These three parameters thus have a major
impact on the modeled results.
Next: (Sub-)mm radiative transfer
Up: Description of ATM 2009
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Gildas manager
2014-07-01