Isis 3 Developer Reference
Isis::AtmosModel Class Referenceabstract

Isotropic atmos scattering model. More...

#include <AtmosModel.h>

Inheritance diagram for Isis::AtmosModel:
Inheritance graph
Collaboration diagram for Isis::AtmosModel:
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Public Member Functions

 AtmosModel (Pvl &pvl, PhotoModel &pmodel)
 Create an AtmosModel object. More...
 
virtual ~AtmosModel ()
 Empty destructor. More...
 
void CalcAtmEffect (double pha, double inc, double ema, double *pstd, double *trans, double *trans0, double *sbar, double *transs)
 Calculate the atmospheric scattering effect using photometric angle information. More...
 
virtual void SetStandardConditions (bool standard)
 Used to calculate atmosphere at standard conditions. More...
 
void GenerateAhTable ()
 This method computes the values of the atmospheric Ah table and sets the properties of the atmospheric Ah spline. More...
 
void GenerateHahgTables ()
 This method computes the values of the atmospheric Hahg and Hahg0 tables and sets the properties of the atmospheric Hahg and Hahg0 splines. More...
 
void GenerateHahgTablesShadow ()
 This method is a modified version of the GenerateHahgTables method and is used solely for shadow modeling. More...
 
void SetAtmosAtmSwitch (const int atmswitch)
 Set the switch that controls the function that will be integrated. More...
 
void SetAtmosBha (const double bha)
 Set the Anisotropic Atmospheric function parameter. More...
 
void SetAtmosHga (const double hga)
 Set the Hapke atmospheric function parameter. More...
 
void SetAtmosInc (const double inc)
 Set the incidence angle. More...
 
void SetAtmosNulneg (const string nulneg)
 Set the Atmospheric function parameter. More...
 
void SetAtmosPhi (const double phi)
 Set the azimuth angle. More...
 
void SetAtmosTau (const double tau)
 Set the Atmospheric function parameter. More...
 
void SetAtmosTauref (const double tauref)
 Set the Atmospheric function parameter. More...
 
void SetAtmosWha (const double wha)
 Set the Atmospheric function parameter. More...
 
void SetAtmosHnorm (const double hnorm)
 Set the Atmospheric function parameter. More...
 
void SetAtmosIord (const string offset)
 Set additive offset in fit. More...
 
void SetAtmosEstTau (const string esttau)
 Estimate the optical depth tau using shadows. More...
 
string AlgorithmName () const
 Return atmospheric algorithm name. More...
 
bool AtmosAdditiveOffset () const
 Allow additive offset in fit? More...
 
double AtmosHnorm () const
 Return atmospheric Hnorm value. More...
 
double AtmosBha () const
 Return atmospheric Bha value. More...
 
double AtmosTau () const
 Return atmospheric Tau value. More...
 
double AtmosWha () const
 Return atmospheric Wha value. More...
 
double AtmosHga () const
 Return atmospheric Hga value. More...
 
double AtmosTauref () const
 Return atmospheric Tauref value. More...
 
bool AtmosNulneg () const
 Return atmospheric Nulneg value. More...
 
double AtmosAb () const
 Return atmospheric Ab value. More...
 
double AtmosHahgsb () const
 Return atmospheric Hahgsb value. More...
 
int AtmosNinc () const
 Return atmospheric Ninc value. More...
 
double AtmosMunot () const
 Return atmospheric Munot value. More...
 
vector< double > AtmosIncTable ()
 Return atmospheric IncTable value. More...
 
vector< double > AtmosAhTable ()
 Return atmospheric AhTable value. More...
 
vector< double > AtmosHahgtTable ()
 Return atmospheric HahgtTable value. More...
 
vector< double > AtmosHahgt0Table ()
 Return atmospheric Hahgt0Table value. More...
 
NumericalApproximation AtmosAhSpline ()
 If GenerateAhTable() has been called this returns a clamped cubic spline of the data set (p_atmosIncTable, p_atmosAhTable) with first derivatives of the endpoints equal to 1.0e30. More...
 
NumericalApproximation AtmosHahgtSpline ()
 If GenerateHahgTables() has been called this returns a clamped cubic spline of the data set (p_atmosIncTable, p_atmosHahgtTable) with first derivatives of the endpoints equal to 1.0e30. More...
 
NumericalApproximation AtmosHahgt0Spline ()
 If GenerateHahgTables() has been called this returns a clamped cubic spline of the data set (p_atmosIncTable, p_atmosHahgt0Table) with first derivatives of the endpoints equal to 1.0e30. More...
 

Static Public Member Functions

static double G11Prime (double tau)
 Perform Chandra and Van de Hulst's series approximation for the g'11 function needed in second order scattering theory. More...
 
static double Ei (double x)
 This routine computes the exponential integral, Ei(x). More...
 
static double En (unsigned int n, double x)
 This routine evaluates the generalized exponential integral, En(x). More...
 

Protected Member Functions

virtual void AtmosModelAlgorithm (double phase, double incidence, double emission)=0
 
void SetAlgorithmName (string name)
 
void SetAtmosNulneg (bool nulneg)
 
void SetAtmosIord (bool offset)
 
void SetAtmosEstTau (bool esttau)
 
void SetOldTau (double tau)
 
void SetOldWha (double wha)
 
PhotoModelGetPhotoModel () const
 
bool StandardConditions () const
 
bool TauOrWhaChanged () const
 Checks whether tau or wha have changed. More...
 
double Eulgam () const
 

Protected Attributes

int p_atmosAtmSwitch
 
int p_atmosNinc
 
double p_atmosBha
 
double p_atmosBhasave
 
double p_atmosHgasave
 
double p_atmosTauref
 
double p_atmosTausave
 
double p_atmosWhasave
 
double p_pstd
 Pure atmospheric-scattering term. More...
 
double p_trans
 Transmission of surface reflected light through the atmosphere overall. More...
 
double p_trans0
 Transmission of surface reflected light through the atmosphere with no scatterings in the atmosphere. More...
 
double p_transs
 Transmission of light that must be subtracted from the flat surface model to get the shadow model. More...
 
double p_sbar
 Illumination of the ground by the sky. More...
 
double p_atmosHga
 
double p_atmosTau
 
double p_atmosWha
 
double p_atmosAb
 
double p_atmosHnorm
 Atmospheric shell thickness normalized to planet radius. More...
 
bool p_atmosAddOffset
 Allow additive offset in fit. More...
 
bool p_atmosEstTau
 Estimate optical depth tau using shadows. More...
 
vector< double > p_atmosIncTable
 
vector< double > p_atmosAhTable
 
double p_atmosHahgsb
 
vector< double > p_atmosHahgtTable
 
vector< double > p_atmosHahgt0Table
 
double p_atmosInc
 
double p_atmosPhi
 
double p_atmosMunot
 
double p_atmosSini
 
double p_atmosCosphi
 
double p_atmosEulgam
 
NumericalApproximation p_atmosAhSpline
 Spline object for the atmospheric Ah Table. Properties are set in GenerateAhTable(). More...
 
NumericalApproximation p_atmosHahgtSpline
 Spline object for the atmospheric Hahg Table. Properties are set in GenerateHahgTables(). More...
 
NumericalApproximation p_atmosHahgt0Spline
 Spline object for the atmospheric Hahg0 Table. Properties are set in GenerateHahgTables(). More...
 

Friends

class NumericalAtmosApprox
 

Detailed Description

Isotropic atmos scattering model.

Author
1998-12-21 Randy Kirk

Constructor & Destructor Documentation

◆ AtmosModel()

Isis::AtmosModel::AtmosModel ( Pvl pvl,
PhotoModel pmodel 
)

Create an AtmosModel object.

Because this is a pure virtual class you can not create an AtmosModel class directly. Instead, see the Isis::AtmosModelFactory class.

Parameters
pvlIsis::Pvl object containing a valid AtmosModel specification
pmodelPhotoModel object containing valud AtmosModel data
See also
atmosphericModels.doc

References Isis::PvlObject::findObject(), and Isis::PvlContainer::hasKeyword().

◆ ~AtmosModel()

virtual Isis::AtmosModel::~AtmosModel ( )
inlinevirtual

Empty destructor.

Member Function Documentation

◆ AlgorithmName()

string Isis::AtmosModel::AlgorithmName ( ) const
inline

Return atmospheric algorithm name.

◆ AtmosAb()

double Isis::AtmosModel::AtmosAb ( ) const
inline

◆ AtmosAdditiveOffset()

bool Isis::AtmosModel::AtmosAdditiveOffset ( ) const
inline

Allow additive offset in fit?

◆ AtmosAhSpline()

NumericalApproximation Isis::AtmosModel::AtmosAhSpline ( )
inline

If GenerateAhTable() has been called this returns a clamped cubic spline of the data set (p_atmosIncTable, p_atmosAhTable) with first derivatives of the endpoints equal to 1.0e30.

Otherwise, it is a natural cubic spline with an empty data set.

Returns
NumericalApproximation Cubic spline

Referenced by Isis::AlbedoAtm::AlbedoAtm(), Isis::ShadeAtm::NormModelAlgorithm(), Isis::AlbedoAtm::NormModelAlgorithm(), Isis::TopoAtm::NormModelAlgorithm(), and Isis::TopoAtm::TopoAtm().

◆ AtmosAhTable()

vector<double> Isis::AtmosModel::AtmosAhTable ( )
inline

Return atmospheric AhTable value.

◆ AtmosBha()

double Isis::AtmosModel::AtmosBha ( ) const
inline

Return atmospheric Bha value.

◆ AtmosHahgsb()

double Isis::AtmosModel::AtmosHahgsb ( ) const
inline

Return atmospheric Hahgsb value.

◆ AtmosHahgt0Spline()

NumericalApproximation Isis::AtmosModel::AtmosHahgt0Spline ( )
inline

If GenerateHahgTables() has been called this returns a clamped cubic spline of the data set (p_atmosIncTable, p_atmosHahgt0Table) with first derivatives of the endpoints equal to 1.0e30.

Otherwise, it is a natural cubic spline with an empty data set.

Returns
NumericalApproximation Cubic spline

◆ AtmosHahgt0Table()

vector<double> Isis::AtmosModel::AtmosHahgt0Table ( )
inline

Return atmospheric Hahgt0Table value.

◆ AtmosHahgtSpline()

NumericalApproximation Isis::AtmosModel::AtmosHahgtSpline ( )
inline

If GenerateHahgTables() has been called this returns a clamped cubic spline of the data set (p_atmosIncTable, p_atmosHahgtTable) with first derivatives of the endpoints equal to 1.0e30.

Otherwise, it is a natural cubic spline with an empty data set.

Returns
NumericalApproximation Cubic spline

◆ AtmosHahgtTable()

vector<double> Isis::AtmosModel::AtmosHahgtTable ( )
inline

Return atmospheric HahgtTable value.

◆ AtmosHga()

double Isis::AtmosModel::AtmosHga ( ) const
inline

Return atmospheric Hga value.

Referenced by Isis::NumericalAtmosApprox::InrFunc2Bint().

◆ AtmosHnorm()

double Isis::AtmosModel::AtmosHnorm ( ) const
inline

Return atmospheric Hnorm value.

◆ AtmosIncTable()

vector<double> Isis::AtmosModel::AtmosIncTable ( )
inline

Return atmospheric IncTable value.

◆ AtmosModelAlgorithm()

virtual void Isis::AtmosModel::AtmosModelAlgorithm ( double  phase,
double  incidence,
double  emission 
)
protectedpure virtual

◆ AtmosMunot()

double Isis::AtmosModel::AtmosMunot ( ) const
inline

Return atmospheric Munot value.

◆ AtmosNinc()

int Isis::AtmosModel::AtmosNinc ( ) const
inline

Return atmospheric Ninc value.

◆ AtmosNulneg()

bool Isis::AtmosModel::AtmosNulneg ( ) const
inline

Return atmospheric Nulneg value.

◆ AtmosTau()

double Isis::AtmosModel::AtmosTau ( ) const
inline

Return atmospheric Tau value.

Referenced by Isis::NumericalAtmosApprox::InrFunc2Bint().

◆ AtmosTauref()

double Isis::AtmosModel::AtmosTauref ( ) const
inline

Return atmospheric Tauref value.

◆ AtmosWha()

double Isis::AtmosModel::AtmosWha ( ) const
inline

Return atmospheric Wha value.

Referenced by Isis::HapkeAtm1::AtmosModelAlgorithm(), and Isis::HapkeAtm2::AtmosModelAlgorithm().

◆ CalcAtmEffect()

void Isis::AtmosModel::CalcAtmEffect ( double  pha,
double  inc,
double  ema,
double *  pstd,
double *  trans,
double *  trans0,
double *  sbar,
double *  transs 
)

Calculate the atmospheric scattering effect using photometric angle information.

Parameters
phaphase angle
incincidence angle
emaemission angle
pstdpure atmospheric-scattering term
transtransmission of surface reflected light through the atmosphere overall
trans0transmission of surface reflected light through the atmosphere with no scatterings in the atmosphere
sbarillumination of the ground by the sky
Exceptions
Isis::IException::User"Invalid photometric angles"

Referenced by Isis::AlbedoAtm::AlbedoAtm(), Isis::ShadeAtm::NormModelAlgorithm(), Isis::AlbedoAtm::NormModelAlgorithm(), Isis::TopoAtm::NormModelAlgorithm(), and Isis::TopoAtm::TopoAtm().

◆ Ei()

double Isis::AtmosModel::Ei ( double  x)
static

This routine computes the exponential integral, Ei(x).

This is defined as

\[ Ei(x) = - \int_{-x}^{\infty} \frac{e^{-t}}{t}\mathrm{d}t = \int_{-\infty}^{x} \frac{e^{t}}{t}\mathrm{d}t \]

for x > 0.

For small x, this method uses the power series,

\[ Ei(x) = \gamma + \ln x + \frac{x}{1*1!} + \frac{x^2}{2*2!} + ... \]

where \( \gamma = 0.5772156649... \) is Euler's constant, and for large x, the asymptotic series is used,

\[ Ei(x) \sim \frac{e^x}{x} (1 + \frac{1!}{x} + \frac{2!}{x^2} + ...) \]

See also
mathworld.wolfram.com/ExponentialIntegral.html
Parameters
xValue at which the exponential integral will be computed, x > 0.0
Returns
double The exponential integral for the given x.
Exceptions
Isis::IException::Programmer"Invalid arguments. Definition requires x > 0.0."
Isis::IException::Math"Power series failed to converge"

References _FILEINFO_.

Referenced by Isis::Isotropic2::AtmosModelAlgorithm(), Isis::HapkeAtm2::AtmosModelAlgorithm(), and Isis::Anisotropic2::AtmosModelAlgorithm().

◆ En()

double Isis::AtmosModel::En ( unsigned int  n,
double  x 
)
static

This routine evaluates the generalized exponential integral, En(x).

This is defined as

\[ E_n(x) = \int_{1}^{\infty} \frac{e^{-xt}}{t^n}\mathrm{d}t \mathrm{ for } x \in \mathbb{R }, n \in \mathbb{Z } \mathrm{such that } x \ge 0.0, n \ge 0 \]

Notice that if x = 0, then the equation is not defined for n = 0 or n = 1, as these will result in \( E_n(x) = \infty \).

This method uses the following for cases:

  • For n > 1 and x = 0.0,

    \[ E_n(0) = \frac{1}{n-1} \]

  • For n = 0 and x > 0.0,

    \[ E_0(x) = \frac{e^{-x}}{x} \]

  • For \( x >\sim 1.0 \), Lentz's continued fraction algorithm is used,

    \[ E_n(x) = e^{-x}(\frac{1}{x + n - \frac{1*n}{x + n + 2 - \frac{2(n+1)}{x + n + 4 - ...}}}) \]

  • For \( 0.0 < x <\sim 1.0 \), series representation is used,

    \[ E_n(x) = \frac{(-x)^{n-1}}{(n-1)!}[- \ln x + \psi (n)] - \sum_{m=0, m \neq n-1}^{\infty}\frac{(-x)^m}{(m-n+1)m!} \]

    where \( \psi (1) = \gamma \) and \( \psi (n) = - \gamma + \sum_{m=1}^{n-1} \frac{1}{m}\) and \( \gamma = 0.5772156649... \) is Euler's constant.

The parameter n is of type unsigned int since n cannot be negative.

The routine allows fast evaluation of En(x) to any accuracy, \(\epsilon\), within the reach of your machine's word length for floating-point numbers. The only modification required for increased accuracy is to supply Euler's constant with enough significant digits.

See also
mathworld.wolfram.com/En-Function.html
Parameters
nInteger value at which the exponential integral will be evaluated (n >= 0)
xThe exponential integral En(x) will be evaluated
Returns
double Value of the exponential integral for the give n and x.
Exceptions
Isis::IException::Programmer"Invalid arguments. Definition requires (x > 0.0 and n >=0 ) or (x >= 0.0 and n > 1)." @throws Isis::IException::Math "Continued fraction failed to converge" @throws Isis::IException::Math "Series representation failed to converge"

References _FILEINFO_.

Referenced by Isis::Isotropic1::AtmosModelAlgorithm(), Isis::HapkeAtm1::AtmosModelAlgorithm(), Isis::Isotropic2::AtmosModelAlgorithm(), Isis::Anisotropic1::AtmosModelAlgorithm(), Isis::HapkeAtm2::AtmosModelAlgorithm(), and Isis::Anisotropic2::AtmosModelAlgorithm().

◆ Eulgam()

double Isis::AtmosModel::Eulgam ( ) const
inlineprotected

◆ G11Prime()

double Isis::AtmosModel::G11Prime ( double  tau)
static

Perform Chandra and Van de Hulst's series approximation for the g'11 function needed in second order scattering theory.

Parameters
taunormal optical depth of atmosphere
Returns
double Value of the g'11 function evaluated at the given tau

References MAX, and Isis::PI.

Referenced by Isis::Isotropic2::AtmosModelAlgorithm(), Isis::HapkeAtm2::AtmosModelAlgorithm(), and Isis::Anisotropic2::AtmosModelAlgorithm().

◆ GenerateAhTable()

void Isis::AtmosModel::GenerateAhTable ( )

This method computes the values of the atmospheric Ah table and sets the properties of the atmospheric Ah spline.

It obtains the hemispheric albedo by integrating the photometric function times mu over mu = 0 to 1 and then over phi = 0 to 2*pi to calculate the hemispheric reflectance Ah needed for the photometric model with atmosphere. The Trapezoid rule is applied to the table of Ah to obtain bihemispheric albedo Ab. The parameter p_atmosAtmSwitch is set to 0 to integrate Ah.

References Isis::PI, Isis::NumericalAtmosApprox::RombergsMethod(), and Isis::IString::UpCase().

Referenced by Isis::AlbedoAtm::AlbedoAtm(), Isis::ShadeAtm::NormModelAlgorithm(), and Isis::TopoAtm::TopoAtm().

◆ GenerateHahgTables()

void Isis::AtmosModel::GenerateHahgTables ( )

This method computes the values of the atmospheric Hahg and Hahg0 tables and sets the properties of the atmospheric Hahg and Hahg0 splines.

It integrates functions involving the single particle phase function (assumed to be Hapke Henyey-Greenstein) over mu = 0 to 1 and then over phi = 0 to 2*pi to calculate the corrections needed for the anisotropic photometric model with atmosphere. The Trapezoid rule is applied to the table of Ah to obtain bihemispheric albedo Ab. The parameter p_atmosAtmSwitch is set to 1, 2, 3 to evaluate the 3 required integrals.

References Isis::PI, Isis::NumericalApproximation::Reset(), and Isis::NumericalAtmosApprox::RombergsMethod().

Referenced by Isis::HapkeAtm1::AtmosModelAlgorithm(), and Isis::HapkeAtm2::AtmosModelAlgorithm().

◆ GenerateHahgTablesShadow()

void Isis::AtmosModel::GenerateHahgTablesShadow ( )

This method is a modified version of the GenerateHahgTables method and is used solely for shadow modeling.

Unlike the GenerateHahgTables method, this method does not tabulate the first or third integrals. It only evaluates the middle integral that corrects the sbar variable (illumination of the ground by the sky).

References Isis::PI, Isis::NumericalApproximation::Reset(), and Isis::NumericalAtmosApprox::RombergsMethod().

Referenced by Isis::HapkeAtm1::AtmosModelAlgorithm(), and Isis::HapkeAtm2::AtmosModelAlgorithm().

◆ GetPhotoModel()

PhotoModel* Isis::AtmosModel::GetPhotoModel ( ) const
inlineprotected

◆ SetAlgorithmName()

void Isis::AtmosModel::SetAlgorithmName ( string  name)
inlineprotected

◆ SetAtmosAtmSwitch()

void Isis::AtmosModel::SetAtmosAtmSwitch ( const int  atmswitch)

Set the switch that controls the function that will be integrated.

This method is only used for testing the methods in this class. This parameter is limited to the values 0, 1, 2, and 3.

Parameters
atmswitchInternal atmospheric function parameter, there is no default
Exceptions
Isis::IException::User"Invalid value of atmospheric atmswitch"

References _FILEINFO_.

◆ SetAtmosBha()

void Isis::AtmosModel::SetAtmosBha ( const double  bha)

Set the Anisotropic Atmospheric function parameter.

This is the coefficient of the single particle Legendre phase function. This parameter is limited to values that are >=-1 and <=1.

Parameters
bhaAnisotropic atmospheric function parameter, default is 0.85
Exceptions
Isis::IException::User"Invalid value of atmospheric bha"

References _FILEINFO_.

◆ SetAtmosEstTau() [1/2]

void Isis::AtmosModel::SetAtmosEstTau ( const string  esttau)

Estimate the optical depth tau using shadows.

Author
Janet Barrett (12/16/2011)
Parameters
esttautrue/false

References _FILEINFO_, and Isis::IString::UpCase().

◆ SetAtmosEstTau() [2/2]

void Isis::AtmosModel::SetAtmosEstTau ( bool  esttau)
inlineprotected

◆ SetAtmosHga()

void Isis::AtmosModel::SetAtmosHga ( const double  hga)

Set the Hapke atmospheric function parameter.

This is the coefficient of the single particle Henyey-Greenstein phase function. This parameter is limited to values that are >-1 and <1.

Parameters
hgaHapke atmospheric function parameter, default is 0.68
Exceptions
Isis::IException::User"Invalid value of atmospheric hga"

References _FILEINFO_.

◆ SetAtmosHnorm()

void Isis::AtmosModel::SetAtmosHnorm ( const double  hnorm)

Set the Atmospheric function parameter.

This is the atmospheric shell thickness normalized to the planet radius and is used to modify angles to get more accurate path lengths near the terminator (ratio of scale height to the planetary radius). This parameter is limited to values that are >=0.

Parameters
hnormAtmospheric function parameter, default is 0.003

References _FILEINFO_, and Isis::toString().

◆ SetAtmosInc()

void Isis::AtmosModel::SetAtmosInc ( const double  inc)

Set the incidence angle.

This method is only used for testing the methods in this class. This parameter is limited to values >=0 and <=90.

Parameters
incInternal atmospheric function parameter, there is no default
Exceptions
Isis::IException::User"Invalid value of atmospheric inc"

References _FILEINFO_, and Isis::PI.

◆ SetAtmosIord() [1/2]

void Isis::AtmosModel::SetAtmosIord ( const string  offset)

Set additive offset in fit.

Author
Sharmila Prasad (8/18/2011)
Parameters
offsettrue/false

References _FILEINFO_, and Isis::IString::UpCase().

◆ SetAtmosIord() [2/2]

void Isis::AtmosModel::SetAtmosIord ( bool  offset)
inlineprotected

◆ SetAtmosNulneg() [1/2]

void Isis::AtmosModel::SetAtmosNulneg ( const string  nulneg)

Set the Atmospheric function parameter.

This determines if negative values after removal of atmospheric effects will be set to NULL. This parameter is limited to values of YES or NO.

Parameters
nulnegAtmospheric function parameter, default is NO
Exceptions
Isis::IException::User"Invalid value of atmospheric nulneg"

References _FILEINFO_, and Isis::IString::UpCase().

◆ SetAtmosNulneg() [2/2]

void Isis::AtmosModel::SetAtmosNulneg ( bool  nulneg)
inlineprotected

◆ SetAtmosPhi()

void Isis::AtmosModel::SetAtmosPhi ( const double  phi)

Set the azimuth angle.

This method is only used for testing the methods in this class. This parameter is limited to values >=0 and <=360.

Parameters
phiInternal atmospheric function parameter, there is no default
Exceptions
Isis::IException::User"Invalid value of atmospheric phi"

References _FILEINFO_, and Isis::PI.

◆ SetAtmosTau()

void Isis::AtmosModel::SetAtmosTau ( const double  tau)

Set the Atmospheric function parameter.

This specifies the normal optical depth of the atmosphere. This parameter is limited to values that are >=0.

Parameters
tauAtmospheric function parameter, default is 0.28
Exceptions
Isis::IException::User"Invalid value of atmospheric tau"

References _FILEINFO_.

◆ SetAtmosTauref()

void Isis::AtmosModel::SetAtmosTauref ( const double  tauref)

Set the Atmospheric function parameter.

This specifies the reference optical depth of the atmosphere to which the image will be normalized. This parameter is limited to values that are >=0.

Parameters
taurefAtmospheric function parameter, default is 0.0
Exceptions
Isis::IException::User"Invalid value of atmospheric tauref"

References _FILEINFO_.

◆ SetAtmosWha()

void Isis::AtmosModel::SetAtmosWha ( const double  wha)

Set the Atmospheric function parameter.

This is the single- scattering albedo of atmospheric particles. This parameter is limited to values that are >0 and <=1.

Parameters
whaAtmospheric function parameter, default is 0.95
Exceptions
Isis::IException::User"Invalid value of atmospheric wha"

References _FILEINFO_.

◆ SetOldTau()

◆ SetOldWha()

◆ SetStandardConditions()

void Isis::AtmosModel::SetStandardConditions ( bool  standard)
virtual

Used to calculate atmosphere at standard conditions.

Referenced by Isis::AlbedoAtm::AlbedoAtm(), and Isis::TopoAtm::TopoAtm().

◆ StandardConditions()

bool Isis::AtmosModel::StandardConditions ( ) const
inlineprotected

◆ TauOrWhaChanged()

bool Isis::AtmosModel::TauOrWhaChanged ( ) const
protected

Friends And Related Function Documentation

◆ NumericalAtmosApprox

friend class NumericalAtmosApprox
friend

Member Data Documentation

◆ p_atmosAb

double Isis::AtmosModel::p_atmosAb
protected

◆ p_atmosAddOffset

bool Isis::AtmosModel::p_atmosAddOffset
protected

Allow additive offset in fit.

◆ p_atmosAhSpline

NumericalApproximation Isis::AtmosModel::p_atmosAhSpline
protected

Spline object for the atmospheric Ah Table. Properties are set in GenerateAhTable().

◆ p_atmosAhTable

vector<double> Isis::AtmosModel::p_atmosAhTable
protected

◆ p_atmosAtmSwitch

◆ p_atmosBha

double Isis::AtmosModel::p_atmosBha
protected

◆ p_atmosBhasave

double Isis::AtmosModel::p_atmosBhasave
protected

◆ p_atmosCosphi

double Isis::AtmosModel::p_atmosCosphi
protected

◆ p_atmosEstTau

bool Isis::AtmosModel::p_atmosEstTau
protected

Estimate optical depth tau using shadows.

Referenced by Isis::HapkeAtm1::AtmosModelAlgorithm(), and Isis::HapkeAtm2::AtmosModelAlgorithm().

◆ p_atmosEulgam

double Isis::AtmosModel::p_atmosEulgam
protected

◆ p_atmosHahgsb

double Isis::AtmosModel::p_atmosHahgsb
protected

◆ p_atmosHahgt0Spline

NumericalApproximation Isis::AtmosModel::p_atmosHahgt0Spline
protected

Spline object for the atmospheric Hahg0 Table. Properties are set in GenerateHahgTables().

Referenced by Isis::HapkeAtm1::AtmosModelAlgorithm(), and Isis::HapkeAtm2::AtmosModelAlgorithm().

◆ p_atmosHahgt0Table

vector<double> Isis::AtmosModel::p_atmosHahgt0Table
protected

◆ p_atmosHahgtSpline

NumericalApproximation Isis::AtmosModel::p_atmosHahgtSpline
protected

Spline object for the atmospheric Hahg Table. Properties are set in GenerateHahgTables().

Referenced by Isis::HapkeAtm1::AtmosModelAlgorithm(), and Isis::HapkeAtm2::AtmosModelAlgorithm().

◆ p_atmosHahgtTable

vector<double> Isis::AtmosModel::p_atmosHahgtTable
protected

◆ p_atmosHga

double Isis::AtmosModel::p_atmosHga
protected

◆ p_atmosHgasave

double Isis::AtmosModel::p_atmosHgasave
protected

◆ p_atmosHnorm

◆ p_atmosInc

◆ p_atmosIncTable

vector<double> Isis::AtmosModel::p_atmosIncTable
protected

◆ p_atmosMunot

◆ p_atmosNinc

int Isis::AtmosModel::p_atmosNinc
protected

◆ p_atmosPhi

double Isis::AtmosModel::p_atmosPhi
protected

◆ p_atmosSini

◆ p_atmosTau

◆ p_atmosTauref

double Isis::AtmosModel::p_atmosTauref
protected

◆ p_atmosTausave

double Isis::AtmosModel::p_atmosTausave
protected

◆ p_atmosWha

◆ p_atmosWhasave

double Isis::AtmosModel::p_atmosWhasave
protected

◆ p_pstd

◆ p_sbar

◆ p_trans

◆ p_trans0

double Isis::AtmosModel::p_trans0
protected

◆ p_transs

double Isis::AtmosModel::p_transs
protected

The documentation for this class was generated from the following files: