ReFRACtor
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This class drives the LRAD code, which gives a polarization correction to scalar intensity and jacobians. More...
#include <l_rad_rt.h>
Public Types | |
enum | BrdfType { LAMBERTIAN = 1, COXMUNK = 2, BPDFVEGN = 3, BPDFSOIL = 4 } |
Public Member Functions | |
LRadRt (const boost::shared_ptr< RadiativeTransferSingleWn > &Rt, const SpectralBound &Spec_bound, const blitz::Array< double, 1 > &Sza, const blitz::Array< double, 1 > &Zen, const blitz::Array< double, 1 > &Azm, bool Pure_nadir, bool Use_first_order_scatt_calc=true, bool Do_second_order=false, double Spectrum_spacing=0.01, const LRadDriver::PsMode ps_mode=LRadDriver::DETECT) | |
Constructor. More... | |
LRadRt (const boost::shared_ptr< StokesCoefficient > &Stokes_coef, const boost::shared_ptr< RtAtmosphere > &Atm, const SpectralBound &Spec_bound, const blitz::Array< double, 1 > &Sza, const blitz::Array< double, 1 > &Zen, const blitz::Array< double, 1 > &Azm, bool Pure_nadir, int Number_stokes, bool Do_second_order=false, int Number_stream=4, double Spectrum_spacing=0.01, const LRadDriver::PsMode ps_mode=LRadDriver::DETECT) | |
Constructor. More... | |
virtual void | add_observer (Observer< std::vector< boost::shared_ptr< NamedSpectrum > > > &Obs) |
Required observable functions. More... | |
void | add_observer_and_keep_reference (boost::shared_ptr< Observer< std::vector< boost::shared_ptr< NamedSpectrum > > > > &Obs) |
Add an observer and keep a reference to it. More... | |
const boost::shared_ptr< RtAtmosphere > & | atmosphere () const |
boost::shared_ptr< RtAtmosphere > | atmosphere_ptr () const |
ArrayAd< double, 2 > | interp_z_matrix (double Wn) |
Return an interpolated z_matrix value for use in offline testing. More... | |
virtual void | notify_add (RtAtmosphere &Observed_object) |
Called when an object is added to an Observable. More... | |
virtual void | notify_add () |
virtual void | notify_remove (RtAtmosphere &Observed_object) |
Called when an object is removed from an Observable. More... | |
virtual void | notify_remove () |
void | notify_update (const RtAtmosphere &atm) |
For performance, we cache some data as we calculate it. More... | |
virtual int | number_spectrometer () const |
Number of spectrometer we have. More... | |
virtual int | number_stokes () const |
Number of stokes parameters we will return in stokes and stokes_and_jacobian. More... | |
virtual int | number_stream () const |
Number of streams to use in processing. More... | |
virtual void | print (std::ostream &Os, bool Short_form=false) const |
Print to stream. More... | |
std::string | print_to_string () const |
Print to string. More... | |
const boost::shared_ptr< RadiativeTransferSingleWn > & | radiative_transfer () const |
virtual Spectrum | reflectance (const SpectralDomain &Spec_domain, int Spec_index, bool Skip_jacobian=false) const |
Calculate reflectance for the given set of wavenumbers/wavelengths. More... | |
virtual void | remove_observer (Observer< std::vector< boost::shared_ptr< NamedSpectrum > > > &Obs) |
Remove an observer. More... | |
virtual blitz::Array< double, 2 > | stokes (const SpectralDomain &Spec_domain, int Spec_index) const |
Calculate stokes vector for the given set of wavenumbers/wavelengths. More... | |
virtual ArrayAd< double, 2 > | stokes_and_jacobian (const SpectralDomain &Spec_domain, int Spec_index) const |
Calculate stokes vector for the given set of wavenumbers/wavelengths. More... | |
virtual ArrayAd< double, 1 > | stokes_and_jacobian_single_wn (double Wn, int Spec_index, const ArrayAd< double, 2 > &Iv) const |
Calculate stokes vector and Jacobian for the given wavenumber. More... | |
const boost::shared_ptr< StokesCoefficient > & | stokes_coefficient () const |
Stokes coefficients used to go from Stokes vector to scalar reflectance. More... | |
virtual blitz::Array< double, 1 > | stokes_single_wn (double Wn, int Spec_index, const ArrayAd< double, 2 > &Iv) const |
Calculate stokes vector for the given wavenumber. More... | |
virtual int | surface_type () const |
Returns an integer with l_rad's representation of surface type. More... | |
Protected Member Functions | |
void | add_observer_do (Observer< std::vector< boost::shared_ptr< NamedSpectrum > > > &Obs, std::vector< boost::shared_ptr< NamedSpectrum > > &t) |
Add an observer. More... | |
void | add_observer_do (Observer< std::vector< boost::shared_ptr< NamedSpectrum > > > &Obs) |
void | clean_dead_ptr () |
Remove any dead pointers. More... | |
void | notify_update_do (const std::vector< boost::shared_ptr< NamedSpectrum > > &Self) |
Function to call to notify Observers of a state change. More... | |
boost::shared_ptr< boost::progress_display > | progress_display (const blitz::Array< double, 1 > &wn) const |
Helper routine, creates a progress meter. More... | |
void | remove_observer_do (Observer< std::vector< boost::shared_ptr< NamedSpectrum > > > &Obs, std::vector< boost::shared_ptr< NamedSpectrum > > &t) |
Remove an observer. More... | |
void | remove_observer_do (Observer< std::vector< boost::shared_ptr< NamedSpectrum > > > &Obs) |
Protected Attributes | |
boost::shared_ptr< RtAtmosphere > | atm |
std::list< boost::weak_ptr< Observer< std::vector< boost::shared_ptr< NamedSpectrum > > > > > | olist |
std::vector< boost::shared_ptr< Observer< std::vector< boost::shared_ptr< NamedSpectrum > > > > > | ref_list |
boost::shared_ptr< StokesCoefficient > | stokes_coef |
Object to go from stokes vector to reflectance. More... | |
Static Protected Attributes | |
static AccumulatedTimer | timer |
This class drives the LRAD code, which gives a polarization correction to scalar intensity and jacobians.
This can also be used on its own to provide a single scatter approximation to the RadiativeTransfer (i.e., without also running LIDORT).
Definition at line 19 of file l_rad_rt.h.
Enumerator | |
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LAMBERTIAN | |
COXMUNK | |
BPDFVEGN | |
BPDFSOIL |
Definition at line 24 of file l_rad_rt.h.
LRadRt::LRadRt | ( | const boost::shared_ptr< RadiativeTransferSingleWn > & | Rt, |
const SpectralBound & | Spec_bound, | ||
const blitz::Array< double, 1 > & | Sza, | ||
const blitz::Array< double, 1 > & | Zen, | ||
const blitz::Array< double, 1 > & | Azm, | ||
bool | Pure_nadir, | ||
bool | Use_first_order_scatt_calc = true , |
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bool | Do_second_order = false , |
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double | Spectrum_spacing = 0.01 , |
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const LRadDriver::PsMode | ps_mode = LRadDriver::DETECT |
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Constructor.
Note that we can run in two modes, either we are doing a polarization correction to an underlying multi-scatter RT code, or we are just doing a single-scatter calculation in the LRad alone. This constructor sets up for the mult-scatter correction.
Rt | RT to apply polarization correction to. |
Spec_bound | Spectral window bounds for each spectrometer. |
Sza | Solar zenith angle. This is in degrees, and should be in the range 0 to 90, and have size number_spectrometer() |
Zen | Zenith angle (degrees), in range 0 to 90, and have size number_spectrometer() |
Azm | Azimuth angle (degrees), in range 0 to 360, and have size number_spectrometer() |
Pure_nadir | If true then scene is purely nadir |
Use_first_order_scatt_calc | Use the first order of scattering calculation from LRad since it is a faster calculation than by most other radiative transfers. If using two RTs together the other RT must only calculate the multiple scattering component of the stokes vector. |
Do_second_order | If true, we do second order corrections |
Spectrum_spacing | The spectrum spacing |
ps_mode | Which pseudo spherical mode to use: REGULAR, ENHANCED, PLANE_PARALLEL, DETECT |
Definition at line 67 of file l_rad_rt.cc.
LRadRt::LRadRt | ( | const boost::shared_ptr< StokesCoefficient > & | Stokes_coef, |
const boost::shared_ptr< RtAtmosphere > & | Atm, | ||
const SpectralBound & | Spec_bound, | ||
const blitz::Array< double, 1 > & | Sza, | ||
const blitz::Array< double, 1 > & | Zen, | ||
const blitz::Array< double, 1 > & | Azm, | ||
bool | Pure_nadir, | ||
int | Number_stokes, | ||
bool | Do_second_order = false , |
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int | Number_stream = 4 , |
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double | Spectrum_spacing = 0.01 , |
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const LRadDriver::PsMode | ps_mode = LRadDriver::DETECT |
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Constructor.
Note that we can run in two modes, either we are doing a polarization correction to an underlying multi-scatter RT code, or we are just doing a single-scatter calculation in the LRad alone. This constructor sets up for the single-scatter calculation only, without a multi-scatter RT.
Stokes_coef | The stokes coefficients to go from vector stokes parameters to reflectance. This should be number_spectrometer() x 4. |
Atm | The RtAtmosphere to use. |
Number_stream | The number of streams to calculate with. Note that this is the "half streams" more commonly used rather than the "full streams" used in LIDORT 3.0. |
Spec_bound | Spectral window bounds for each spectrometer. |
Sza | Solar zenith angle. This is in degrees, and should be in the range 0 to 90, and have size number_spectrometer() |
Zen | Zenith angle (degrees), in range 0 to 90, and have size number_spectrometer() |
Azm | Azimuth angle (degrees), in range 0 to 360, and have size number_spectrometer() |
Pure_nadir | If true then scene is purely nadir |
Number_stokes | Number of stokes coefficients to use. |
Do_second_order | If true, we do second order corrections |
Spectrum_spacing | The spectrum spacing |
ps_mode | Which pseudo spherical mode to use: REGULAR, ENHANCED, PLANE_PARALLEL, DETECT |
Definition at line 128 of file l_rad_rt.cc.
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inlinevirtualinherited |
Required observable functions.
Implements FullPhysics::Observable< std::vector< boost::shared_ptr< NamedSpectrum > > >.
Definition at line 42 of file radiative_transfer_fixed_stokes_coefficient.h.
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inlineinherited |
Add an observer and keep a reference to it.
See the discussion in the Observer class description for details.
Definition at line 107 of file observer.h.
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inlineprotectedinherited |
Add an observer.
Definition at line 148 of file observer.h.
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inlineprotectedinherited |
Definition at line 159 of file observer.h.
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inlineinherited |
Definition at line 77 of file radiative_transfer_single_wn.h.
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inlineinherited |
Definition at line 26 of file radiative_transfer_single_wn.h.
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inlineprotectedinherited |
Remove any dead pointers.
Definition at line 196 of file observer.h.
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inline |
Return an interpolated z_matrix value for use in offline testing.
Definition at line 62 of file l_rad_rt.h.
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inlinevirtualinherited |
Called when an object is added to an Observable.
Default is to do nothing.
Definition at line 47 of file observer.h.
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inlinevirtualinherited |
Definition at line 48 of file observer.h.
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inlinevirtualinherited |
Called when an object is removed from an Observable.
Default is to do nothing.
Definition at line 55 of file observer.h.
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inlinevirtualinherited |
Definition at line 56 of file observer.h.
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inlinevirtual |
For performance, we cache some data as we calculate it.
This becomes stale when the Atmosphere is changed, so we observe atm and mark the cache when it changes.
Reimplemented from FullPhysics::Observer< RtAtmosphere >.
Definition at line 71 of file l_rad_rt.h.
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inlineprotectedinherited |
Function to call to notify Observers of a state change.
The object should pass itself to this function, so it can be passed to the Observers.
Definition at line 121 of file observer.h.
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inlinevirtualinherited |
Number of spectrometer we have.
Implements FullPhysics::RadiativeTransfer.
Definition at line 31 of file radiative_transfer_fixed_stokes_coefficient.h.
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inlinevirtual |
Number of stokes parameters we will return in stokes and stokes_and_jacobian.
Implements FullPhysics::RadiativeTransfer.
Definition at line 55 of file l_rad_rt.h.
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inlinevirtual |
Number of streams to use in processing.
Note that Lidort 3.0 used a less common "full streams" that was twice the more commonly used "half streams". This function returns the later. This is the same as what is used in Lidort 3.5 and LRad. The "full streams" used in Lidort 3.0 would be twice this.
Implements FullPhysics::RadiativeTransferSingleWn.
Definition at line 56 of file l_rad_rt.h.
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virtual |
Print to stream.
Reimplemented from FullPhysics::RadiativeTransferSingleWn.
Definition at line 493 of file l_rad_rt.cc.
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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.
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protectedinherited |
Helper routine, creates a progress meter.
This will return 0 if we aren't logging, or if we don't have enough points to bother with.
Definition at line 19 of file radiative_transfer.cc.
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inline |
Definition at line 76 of file l_rad_rt.h.
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virtualinherited |
Calculate reflectance for the given set of wavenumbers/wavelengths.
Spec_domain | List of wavenumber/wavelength to calculate for. |
Spec_index | The Spectral index |
Skip_jacobian | If true, don't do the Jacobian calculation. Often this is significantly faster to calculate. |
Implements FullPhysics::RadiativeTransfer.
Definition at line 12 of file radiative_transfer_fixed_stokes_coefficient.cc.
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inlinevirtualinherited |
Remove an observer.
Implements FullPhysics::Observable< std::vector< boost::shared_ptr< NamedSpectrum > > >.
Definition at line 44 of file radiative_transfer_fixed_stokes_coefficient.h.
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inlineprotectedinherited |
Remove an observer.
Definition at line 173 of file observer.h.
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inlineprotectedinherited |
Definition at line 181 of file observer.h.
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virtualinherited |
Calculate stokes vector for the given set of wavenumbers/wavelengths.
Spec_domain | List of wavenumber/wavelength to calculate for. |
Spec_index | The Spectral index |
Implements FullPhysics::RadiativeTransfer.
Definition at line 7 of file radiative_transfer_single_wn.cc.
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virtualinherited |
Calculate stokes vector for the given set of wavenumbers/wavelengths.
This also calculates the Jacobian of the stokes with respect to the state vector elements.
Spec_domain | List of wavenumber/wavelength to calculate for. |
Spec_index | The Spectral index |
Implements FullPhysics::RadiativeTransfer.
Definition at line 22 of file radiative_transfer_single_wn.cc.
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virtual |
Calculate stokes vector and Jacobian for the given wavenumber.
You can optionally supply a set of intermediate atmosphere variables (e.g., taug, taur, taua_i) to use instead of with atmosphere_ptr() to calculate this.
Wn | Wavenumber to calculate for. This should be in cm^-1 |
Spec_index | The Spectral index |
Iv | Optional intermediate variables to use, rather than calculating. |
Implements FullPhysics::RadiativeTransferSingleWn.
Definition at line 405 of file l_rad_rt.cc.
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inlineinherited |
Stokes coefficients used to go from Stokes vector to scalar reflectance.
Definition at line 24 of file radiative_transfer_fixed_stokes_coefficient.h.
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virtual |
Calculate stokes vector for the given wavenumber.
You can optionally supply a set of intermediate atmosphere variables (e.g., taug, taur, taua_i) to use instead of with atmosphere_ptr() to calculate this.
Wn | Wavenumber to calculate for. This should be in cm^-1 |
Spec_index | The Spectral index |
Iv | Optional intermediate variables to use, rather than calculating. |
Implements FullPhysics::RadiativeTransferSingleWn.
Definition at line 330 of file l_rad_rt.cc.
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inlinevirtual |
Returns an integer with l_rad's representation of surface type.
Definition at line 59 of file l_rad_rt.h.
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protectedinherited |
Definition at line 98 of file radiative_transfer_single_wn.h.
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protectedinherited |
Definition at line 200 of file observer.h.
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protectedinherited |
Definition at line 201 of file observer.h.
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protectedinherited |
Object to go from stokes vector to reflectance.
Definition at line 65 of file radiative_transfer_fixed_stokes_coefficient.h.
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staticprotectedinherited |
Definition at line 92 of file radiative_transfer.h.