found::SphericalDistanceDeterminationAlgorithm Class Reference

The DistanceDeterminationAlgorithm class houses the Distance Determination Algorithm. More...

#include <distance.hpp>

Inheritance diagram for found::SphericalDistanceDeterminationAlgorithm:

Collaboration diagram for found::SphericalDistanceDeterminationAlgorithm:

Public Member Functions
	SphericalDistanceDeterminationAlgorithm (decimal radius, Camera &&cam)
	Creates a SphericalDeterminationAlgorithm, which deduces the Position vector of a sattelite from Earth by modeling Earth as a sphere.
	~SphericalDistanceDeterminationAlgorithm ()
PositionVector	Run (const Points &p) override
	Obtains the position of the planet relative to the camera.
Public Member Functions inherited from found::DistanceDeterminationAlgorithm
	DistanceDeterminationAlgorithm ()=default
virtual	~DistanceDeterminationAlgorithm ()
Public Member Functions inherited from found::Stage< Points, PositionVector >
	Stage ()=default
	Constructs a new Stage.
virtual	~Stage ()=default
	Destroys this.
void	DoAction () override
	Executes Run (with a stored input and storing the output)
Points &	GetResource ()
	Returns the stored input of this.
PositionVector *&	GetProduct ()
	Returns the stored output of this.

Protected Member Functions
Vec3	getCenter (Vec3 *spats)
	Returns the center of earth as a 3d Vector.
PreciseDecimal	getRadius (Vec3 *spats, Vec3 center)
	Returns the radius of the calculated "earth" (normalized)
PreciseDecimal	getDistance (PreciseDecimal r, PreciseDecimal c)
	Returns the scaled distance from earth.

Protected Attributes
Camera	cam_
	cam_ field instance describes the camera settings used for the photo taken
decimal	radius_
	radius_ field instance describes the defined radius of earth.
Protected Attributes inherited from found::Stage< Points, PositionVector >
Points	resource
	The stored input for this.
PositionVector *	product
	The pointer to the stored output for this.

Detailed Description

The DistanceDeterminationAlgorithm class houses the Distance Determination Algorithm.

This algorithm calculates the distance from Earth based on the pixels of Earth's Edge found in the image.

Note

This class assumes that Earth is a perfect sphere

Constructor & Destructor Documentation

SphericalDistanceDeterminationAlgorithm()

found::SphericalDistanceDeterminationAlgorithm::SphericalDistanceDeterminationAlgorithm ( decimal  radius, Camera &&  cam  )

inline

Creates a SphericalDeterminationAlgorithm, which deduces the Position vector of a sattelite from Earth by modeling Earth as a sphere.

Parameters

radius	The radius of Earth
cam	The camera used to capture the picture of Earth

~SphericalDistanceDeterminationAlgorithm()

found::SphericalDistanceDeterminationAlgorithm::~SphericalDistanceDeterminationAlgorithm ( )

inline

Member Function Documentation

getCenter()

Vec3 found::SphericalDistanceDeterminationAlgorithm::getCenter ( Vec3 *  spats )

protected

Returns the center of earth as a 3d Vector.

Parameters

spats

The normalized spatial coordinates used to find the center

Returns

The center of earth as a 3d Vector

CirclePt is a vector that points to a point on the plane. We also know the center vector should point to a point on the plane. So, we get (circlePt - center) * circleN = 0. This is equivalent to (center * circleN) = (circlePt * circleN)

We have (center - mid1/mid2) gives us the vector perpendicular to the mid1N/mid2N vector. Hence, (center - mid1)*mid1N = 0. This becomes (mid1N * center) = (mid1N * mid1). (This is the same for mid2) So we have: circleN * center = circleN * circlePt mid1N * center = mid1N * mid1 mid2N * center = mid2N * mid2 This becomes a systems of linear equation

getDistance()

PreciseDecimal found::SphericalDistanceDeterminationAlgorithm::getDistance ( PreciseDecimal  r, PreciseDecimal  c  )

protected

Returns the scaled distance from earth.

Parameters

r	The normalized radius
c	The distance to the center of the small circle

Returns

The distance from earth as a Scalar

getRadius()

PreciseDecimal found::SphericalDistanceDeterminationAlgorithm::getRadius ( Vec3 *  spats, Vec3  center  )

protected

Returns the radius of the calculated "earth" (normalized)

Parameters

spats	The normalized spatial coordinates
center	The center of the earth as a 3d Vector

Returns

The radius of earth normalized

Run()

PositionVector found::SphericalDistanceDeterminationAlgorithm::Run ( const Points &  p )

overridevirtual

Obtains the position of the planet relative to the camera.

Parameters

p	The points on the edge of Earth (in the image taken by the camera given to this)

Returns

PositionVector The position vector of the Earth relative to the camera

Precondition

p must refer to points taken by the camera that was passed to this

Postcondition

If p.size() < 3, then the result is exactly the zero vector

Implements found::Stage< Points, PositionVector >.

Member Data Documentation

cam_

Camera found::SphericalDistanceDeterminationAlgorithm::cam_

protected

cam_ field instance describes the camera settings used for the photo taken

radius_

decimal found::SphericalDistanceDeterminationAlgorithm::radius_

protected

radius_ field instance describes the defined radius of earth.

Should be 6378.0 (km)

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

• src/distance/distance.hpp
• src/distance/distance.cpp