This class handles the solar Doppler stretch to calculate the shift of the solar lines with respect to the telluric lines. More...

#include <solar_doppler_shift_l1b.h>

Inheritance diagram for FullPhysics::SolarDopplerShiftL1b:

Collaboration diagram for FullPhysics::SolarDopplerShiftL1b:

Public Member Functions
	SolarDopplerShiftL1b (const DoubleWithUnit &Solar_distance, const DoubleWithUnit &Solar_relative_velocity, bool Apply_doppler_shift=true)
	Create a SolarDopplerShiftL1b. More...

virtual	~SolarDopplerShiftL1b ()

double	doppler_shift () const

virtual SpectralDomain	doppler_stretch (const SpectralDomain &Spec_domain) const
	Shift wavenumbers to account for doppler stretch. More...

virtual void	print (std::ostream &Os) const
	Print description of object. More...

std::string	print_to_string () const
	Print to string. More...

virtual DoubleWithUnit	solar_distance () const
	Return Earth-Sun distance. More...

DoubleWithUnit	solar_relative_velocity () const
	Velocity of the sounding to the center of the sun. More...

Detailed Description

This class handles the solar Doppler stretch to calculate the shift of the solar lines with respect to the telluric lines.

This implementation gets the Level 1b solar velocity and solar distance passed to it.

Definition at line 17 of file solar_doppler_shift_l1b.h.

Constructor & Destructor Documentation

◆ SolarDopplerShiftL1b()

SolarDopplerShiftL1b::SolarDopplerShiftL1b	(	const DoubleWithUnit &	Solar_distance,
		const DoubleWithUnit &	Solar_relative_velocity,
		bool	Apply_doppler_shift = `true`
	)

Create a SolarDopplerShiftL1b.

Parameters

Solar_distance	The distance between observed surface and sun
Solar_relative_velocity	The velocity of the sun along the observed sounding location/sun vector. This includes the rotation of the earth. Positive indicates the sun is moving away from the point.
Apply_doppler_shift	Indicates if we should apply the doppler shift or not. If this is false, then we just pass the wave numbers through unchanged in doppler_stretch.

Definition at line 25 of file solar_doppler_shift_l1b.cc.

◆ ~SolarDopplerShiftL1b()

virtual FullPhysics::SolarDopplerShiftL1b::~SolarDopplerShiftL1b ( )

inlinevirtual

Definition at line 23 of file solar_doppler_shift_l1b.h.

Member Function Documentation

◆ doppler_shift()

double FullPhysics::SolarDopplerShiftL1b::doppler_shift ( ) const

inline

Definition at line 44 of file solar_doppler_shift_l1b.h.

◆ doppler_stretch()

SpectralDomain SolarDopplerShiftL1b::doppler_stretch ( const SpectralDomain & Spec_domain ) const

virtual

Shift wavenumbers to account for doppler stretch.

Parameters

Spec_domain wavenumber/wavelength

Returns: Wavenumber/wavelength with Doppler stretch.

Implements FullPhysics::SolarDopplerShift.

Definition at line 51 of file solar_doppler_shift_l1b.cc.

◆ print()

void SolarDopplerShiftL1b::print ( std::ostream & Os ) const

virtual

Print description of object.

Reimplemented from FullPhysics::SolarDopplerShift.

Definition at line 42 of file solar_doppler_shift_l1b.cc.

◆ print_to_string()

std::string FullPhysics::Printable< SolarDopplerShift >::print_to_string ( ) const

inlineinherited

Print to string.

This is primarily useful for SWIG wrappers to this class, e.g. a to_s method in ruby.

Definition at line 31 of file printable.h.

◆ solar_distance()

virtual DoubleWithUnit FullPhysics::SolarDopplerShiftL1b::solar_distance ( ) const

inlinevirtual

Return Earth-Sun distance.

Returns: Earth-Sun distance.

Implements FullPhysics::SolarDopplerShift.

Definition at line 30 of file solar_doppler_shift_l1b.h.

◆ solar_relative_velocity()

DoubleWithUnit FullPhysics::SolarDopplerShiftL1b::solar_relative_velocity ( ) const