SpectralRadianceUnitType
- class pyarts.arts.SpectralRadianceUnitType(*args, **kwargs)
Choice of spectral radiance unit in conversions.
The conversion to one of these units is expected to happen from the internal representation of
spectral_radiance
, which is [W / m Hz sr].For the description below,
is the speed of light, is the Boltzmann constant, is the frequency, is the Planck constant, is the conversion function, and is the internal representation ofspectral_radiance
.For Rayleigh-Jeans brightness temperature the conversion is:
For Planck brightness temperature the conversion is:
The spectral radiance per wavelength [W / m
m sr] is:The spectral radiance per wavenumber [W / m
m sr] is:Lastly, the unit option of course just retains the current state [W / m
Hz sr].Valid options:
"RJBT"
or"Tr"
: Rayleigh-Jeans brightness temperature [K]"PlanckBT"
or"Tb"
: Planck brightness temperature [K]"W_m2_m_sr"
or"W/(m^2 m sr)"
: Spectral radiance wavelength [W / m m sr]"W_m2_m1_sr"
or"W/(m^2 m-1 sr)"
: Spectral radiance wavenumber [W / m m sr]"unit"
or"1"
: Unit spectral radiance [W / m Hz sr]
Workspace variables of type SpectralRadianceUnitType
Overview
Method
Read variable from file
Method
Saves variable to file
Static Method
Create variable from file
Static Method
Get a list of all options
Static Method
Get a list of all options as strings
Static Data
pyarts.arts.SpectralRadianceUnitType.PlanckBT
“PlanckBT” -
SpectralRadianceUnitType
Static Data
pyarts.arts.SpectralRadianceUnitType.RJBT
“RJBT” -
SpectralRadianceUnitType
Static Data
pyarts.arts.SpectralRadianceUnitType.Tb
“PlanckBT” -
SpectralRadianceUnitType
Static Data
pyarts.arts.SpectralRadianceUnitType.Tr
“RJBT” -
SpectralRadianceUnitType
Static Data
pyarts.arts.SpectralRadianceUnitType.W_m2_m1_sr
“W_m2_m1_sr” -
SpectralRadianceUnitType
Static Data
pyarts.arts.SpectralRadianceUnitType.W_m2_m_sr
“W_m2_m_sr” -
SpectralRadianceUnitType
Static Data
pyarts.arts.SpectralRadianceUnitType.unit
“unit” -
SpectralRadianceUnitType
Operator
self == other
Operator
Default object formatter.
Operator
self >= other
Operator
__getstate__(self) -> tuple[str]
Operator
self > other
Operator
Allows hashing
Operator
__init__(self, arg: str, /) -> None
Operator
self <= other
Operator
self < other
Operator
self != other
Operator
__repr__(self) -> str
Operator
__setstate__(self, arg: tuple[str], /) -> None
Operator
__str__(self) -> str
Constructors
- __init__(self) None
- __init__(self, arg: pyarts.arts.SpectralRadianceUnitType) None
- __init__(self, arg: str, /) None
Methods
- readxml(self, file: str) None
Read variable from file
- Parameters:
file (str) – A file that can be read
- On Error:
Throws RuntimeError for any failure to read
- savexml(self, file: str, type: str = 'ascii', clobber: bool = True) None
Saves variable to file
- Parameters:
- On Error:
Throws RuntimeError for any failure to save
Static Methods
- fromxml(file: str) pyarts.arts.SpectralRadianceUnitType
Create variable from file
- Parameters:
file (str) – A file that can be read
- On Error:
Throws RuntimeError for any failure to read
- get_options() list[pyarts.arts.SpectralRadianceUnitType]
Get a list of all options
Operators
- __eq__(self, arg: pyarts.arts.SpectralRadianceUnitType, /) bool
self == other
- __format__(format_spec, /)
Default object formatter.
Return str(self) if format_spec is empty. Raise TypeError otherwise.
- __ge__(self, arg: pyarts.arts.SpectralRadianceUnitType, /) bool
self >= other
- __gt__(self, arg: pyarts.arts.SpectralRadianceUnitType, /) bool
self > other
- __init__(self) None
- __init__(self, arg: pyarts.arts.SpectralRadianceUnitType) None
- __init__(self, arg: str, /) None
- __le__(self, arg: pyarts.arts.SpectralRadianceUnitType, /) bool
self <= other
- __lt__(self, arg: pyarts.arts.SpectralRadianceUnitType, /) bool
self < other
- __ne__(self, arg: pyarts.arts.SpectralRadianceUnitType, /) bool
self != other