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AstroAtmosphere-1.6
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مشاهده بیشترتوضیحات
Collection of equations for refractive index, refraction and dispersion calculations of atmospheric air.
| ویژگی | مقدار |
|---|---|
| سیستم عامل | - |
| نام فایل | AstroAtmosphere-1.6 |
| نام | AstroAtmosphere |
| نسخه کتابخانه | 1.6 |
| نگهدارنده | [] |
| ایمیل نگهدارنده | [] |
| نویسنده | Joost van den Born |
| ایمیل نویسنده | born@astron.nl |
| آدرس صفحه اصلی | https://gitlab.astro-wise.org/micado/atmosphericmodel |
| آدرس اینترنتی | https://pypi.org/project/AstroAtmosphere/ |
| مجوز | GNU General Public License v3 |
# AstroAtmosphere
**Note:**
It would be appreciated if a reference to the following work, for which this package was originally build, is included whenever this code is used for a publication:
*Quantification of the expected residual dispersion of the MICADO Near-IR imaging instrument*, van den Born & Jellema, 2020, MNRAS, DOI: [10.1093/mnras/staa1870](https://doi.org/10.1093/mnras/staa1870).
**Author info**: *Joost van den Born*, *born@astron.nl*
## Example
A minimal working example to calculate the atmospheric dispersion at Cerro Armazones between 1.49 and 1.78 micron.
```python
from AstroAtmosphere import *
# Parameters at Cerro Armazones
T = 279.65 # k
P = 71200 # Pa
H = 0.22
xc = 450 # ppm
lat = -24.5983 # degrees
h = 3064 # m
l1 = 1.49 # micron
l2 = 1.78 # micron
z0 = 30
# Initializing dispersion model
at = Observatory()
# Calculating indices of refraction for l1 and l2
n1 = at.n_tph(l=l1, T=T, p=P, RH=H, xc=xc)
n2 = at.n_tph(l=l2, T=T, p=P, RH=H, xc=xc)
# Density of the atmosphere (following CIPM-81/91 equations)
rho = at.rho(p=P, T=T, RH=H, xc=xc)
# Initializing refraction model and setting the reduced height
disp = dispersion(lat, h)
disp.setReducedHeight(P, rho)
# Calculation of the atmopheric dipsersion
atm_dispersion = disp.cassini(n1, n2, z0) * 3.6e6
print ('The dispersion is %.03f milli arc seconds' %(atm_dispersion))
```
## Installation
The package is available through Git-Lab and through PyPI. The package may be installed using the `setup.py` file, but easier is to install using `pip`.
```bash
pip install AstroAtmosphere
```
## Contents of the AstroAtmosphere package
The package contains the following files:
- `/data/1976USSA.txt` : Data file of the 1976 US Standard Atmosphere.
- `ciddorModel.py` : Contains the `Observatory()` class to calculate the refractive index of atmospheric air, using the Ciddor (1996) model.
- `dispersionModels.py` : Contains various atmospheric models that can be used to calculate the atmospheric dispersion
- `misc.py` : Contains several miscellaneous functions, e.g. to quickly calculate the refractive index.
- `neoslalib.py` : Contains a Python native port of the `pyslalib.SLA_REFRO()` routine, translated from the original FORTRAN code.
- `observatories.py` : Contains a dictionary with the average atmospheric conditions for various large observatories around the world.
- `refractionModels.py` : Contains various atmospheric models that can be used to calculate the atmospheric refraction
- `refractivityModels.py` : Contains various functions from literature to calculate the refractive index. Some examples of works included are Ciddor (1996), Barrell & Sears (1939), SLALIB, Owens (1967) and Edlen (1966).
## The Ciddor refractivity model
The refractivity model from Ciddor, 1996, calculates the index of refraction of air using the following parameters:
- T - Temperature in Kelvin
- p - Pressure in Pascal
- RH - Relative humidity in fractional units
- xc - CO2 density in parts per million
It is invoked by first initializing an `Observatory()` object. The atmospheric conditions can be parsed into the `n_tph()` function.
```python
at = Observatory()
n = at.n_tph(l=0.55, T=273.15, p=101325, RH=0.2, xc=300)
```
Basic functionality of other refractivity models is included as well and is discussed below.
## The atmospheric refraction and atmospheric dispersion models
If the atmospheric refraction is denoted as R(n), then atmospheric dispersion is defined as R(n1) - R(n2). Thus they are very similar in function and use.
The available models in this package:
- `refractionIntegral()` - Full integration using the refractive integral (requires detailed information about the atmosphere, e.g. `AstroAtmosphere/data/1976USSA.txt`)
- `planeParallel()` - Plane-parallel atmosphere refraction model
- `cassini()` - Cassini's homogeneous atmosphere refraction model
- `oriani()` - Oriani's theorem ( Atan(z) + Btan^3(z) )
- `tan5()` - Oriani's theorem expanded ( Atan(z) + Btan^3(z) + Ctan^5(z) )
- `corbard()` - Error function refraction model
- `matharExponential()` - Barometric exponential model by R. Mathar.
The package also includes a python native port of the `SLA_REFRO()` FORTRAN routine, ported from pyslalib. See below for more information.
Input parameters for the spherical atmosphere models (all but the first):
- T - Temperature [K]
- p - Pressure [Pa]
- RH - Relative humidity
- xc - CO2 density [ppm]
- lat - Latitude [deg]
- h - Height above sea level [m]
- l - Wavelength(s) [μm]
- z - Zenith angle [deg]
An example - To calculate the atmospheric refraction we set up a `refraction()` object. This requires the latitude and altitude of the observer. The atmospheric dispersion is calculated similarly, but by exchanging the `refraction()` object by a `dispersion()` object and parsing two refractive indices into the `cassini()` function.
```python
# Density of the atmosphere (following CIPM-81/91 equations)
rho = at.rho(p=101325, T=273.15, RH=0.2, xc=300)
# Initializing refraction model and setting the reduced height
ref = refraction(lat=30, h=2200)
ref.setReducedHeight(p=101325, rho=rho)
# Calculating the atmospheric refraction
atm_ref = ref.cassini(n, zenith=30)
```
## Analytical error propagation
Full analytical error propagation is available for the Ciddor dispersion model (`Observatory.dn_tph()`), for the Cassini refraction model (`refraction.cassiniError()`) and for the Cassini dispersion model (`dispersion.cassiniError()`).
The results agree well with a Monte Carlo simulation, suggesting that if additional errors have not been considered, they are of neglible importance.
Uncertainties that are considered:
Ciddor dispersion model:
| Param. | Description | Unit |
| ------ | ------ | ------ |
| dl | Wavelength | um |
| dT | Temperature | K |
| dP | Pressure | Pa |
| dRH | Relative Humidity | |
| dCO2 | CO2 density | ppm |
Cassini refraction model:
| Param. | Description | Unit |
| ------ | ------ | ------ |
| dn | Refractive index | |
| dz | Zenith angle | deg |
Cassini dispersion model:
| Param. | Description | Unit |
| ------ | ------ | ------ |
| dl1, dl2 | Wavelength(s) | um |
| dT | Temperature | K |
| dP | Pressure | Pa |
| dRH | Relative Humidity | |
| dCO2 | CO2 density | ppm |
| dz | Zenith angle | deg |
An example of its use is given in the code snippet here:
```python
# Initializing dispersion object
disp = dispersion(lat, h)
disp.setReducedHeight(P, rho)
# Atmospheric dispersion
dispersion_obs = disp.cassini(n1, n2, zenith_obs)
# Uncertainty in the atmospheric dispersion
dispersion_unc = disp.cassiniError(zenith_obs, l1, l2, T, P, H, xc,
dl1=0.001, dl2=0.001, dT=0.2, dP=30, dRH=0.03, dCO2=25, dz=1/3600) * 3.6e6
```
## Other refractivity models
The package also includes limited functionality of other refractivity models. These are not as extensive, work only under standard atmospheric conditions, or over a limited wavelength range, compared to the Ciddor model.
Included are
| Model name | Function | Remarks |
| ---------- | -------- | ------- |
| Barrell & Sears (1939) | `BarrellAndSears()` | Outdated model, especially poor for short wavelengths. |
| Ciddor (1996) | `Ciddor()` | Only at standard atmosphere. CO2 density can be changed. |
| Edlen (1953) | `Edlen1953()` | The equation by Edlèn, 1953, combined with modification from Barrel (1951), to include temperature, pressure and humidity dependence. |
| Edlen (1966) | `Edlen1966()` | Allows for any temperature, pressure, humidity and CO2 density.|
| Owens (1967) | `Owens()` | Allows for any temperature, pressure, humidity. |
| Bonsch & Potulski (1998) | `BonschPotulski()` | Allows for any temperature, pressure, humidity and CO2 density. |
| Birch & Downs (1994) | `BirchDowns()` | Only at standard atmosphere. Function requires wavelength only. |
| Peck & Reeder (1972) | `PeckReeder()` | Only at standard atmosphere. Function requires wavelength only. |
| Mathar (2006) | `Mathar()` | Allows for temperature, pressure and humidity specification. Works best at wavelengths above 1.4 μm. |
| Hohenkerk & Sinclair (1985) | `HohenkerkAndSinclair()` | Based on Barrell & Sears equation. Generally, gives slightly larger values.|
| Hohenkerk & Sinclair (1985) | `slalib()` | Uses pySLALIB to retrieve the refractive index at standard atmospheric conditions.|
The last function extracts the refractive index from the `pyslalib.sla_refro()` function and thus requires [pyslalib](https://pypi.org/project/pySLALIB/). This is an optional dependency for the setup of AstroAtmosphere.
## Quick functions
Some functions can make use of the `observatories` dictionary as input. These include default average conditions of the atmosphere at these locations. When these are used, only the wavelength and zenith angle are required to calculate the refraction and dispersion.
```python
# Quick refractive index
nq = quick_refractive_index(l=1.49, conditions='STANDARD')
# Quick refraction
rq = quick_refraction(l1, zenith_obs, conditions='STANDARD')
# Quick dispersion
dq = quick_dispersion(l1, l2, zenith_obs, conditions='STANDARD')
```
Presently, several observatories are known. These can all be found in the `observatories` dictionary. Contact the author to add additional standard conditions.
| Observatory | Flag | Notes |
| --------------------------------------------- | ----------------- | --------------------------------------------- |
| Standard conditions | `STANDARD` | |
| Cerro Armazones | `CERRO_ARMAZONES` | Location of the future ELT |
| Cerro Paranal | `CERRO_PARANAL` | Location of the VLT, VISTA, VST, NGTS and SSO |
| Roque de los Muchachos Observatory (La Palma) | `LA_PALMA` | GTC, INT, WHT, NOT, and others. |
| La Silla Observatory | `LA_SILLA` | ESO 3.6m telescope, NTG, BlackGEM and others. |
| Las Campanas Observatory | `LAS_CAMPANAS` | Site of the future GMT. |
| Mauna Kea Observatory (Hawaii) | `MAUNA_KEA` | Location of Keck, Subaru, Gemini North and others.|
## Other
This package also contains a python native port of the `SLA_REFRO()` routine of the pyslalib package, which was originally written in FORTRAN by P.T. Wallace. It can be called directly using `sla_refro()`. When using the same units as the other refraction functions, you might prefer using `slalib_refraction()` or `slalib_dispersion()`. Do note that this implementation is slower than the (compiled) FORTRAN implementation.
Finally, the dispersion model used by Alexei Filippenko in 1982 is also included. This model is a combination of the (modified) Edlèn equation and a plane-parallel atmospheric geometry. This calculation can be accessed by calling the `Filippenko1982()` function.
نحوه نصب
نصب پکیج whl AstroAtmosphere-1.6:
pip install AstroAtmosphere-1.6.whl
نصب پکیج tar.gz AstroAtmosphere-1.6:
pip install AstroAtmosphere-1.6.tar.gz