Examples of Rotation

com.barrybecker4.puzzle.tantrix.model.Rotation
Turns a tree into a string via in order traversal. Implements visitor pattern @author Barry Becker
com.jcloisterzone.board.Rotation
com.khorn.terraincontrol.util.Rotation
com.sencha.gxt.chart.client.draw.Rotation
Represents a two dimensional rotation.
de.christopherstock.lib.Lib.Rotation
fcagnin.jgltut.tut06.Rotation
b.com/integeruser/jgltut for info, updates and license terms.
Part II. Positioning Chapter 6. Objects in Motion http://www.arcsynthesis.org/gltut/Positioning/Tutorial%2006.html @author integeruser
net.lightstone.model.Rotation
An immutable class which represents a rotation in the in-game world. @author Graham Edgecombe
ofc4j.model.axis.Label.Rotation
org.apache.commons.math.geometry.Rotation
This class implements rotations in a three-dimensional space.
Rotations can be represented by several different mathematical entities (matrices, axe and angle, Cardan or Euler angles, quaternions). This class presents an higher level abstraction, more user-oriented and hiding this implementation details. Well, for the curious, we use quaternions for the internal representation. The user can build a rotation from any of these representations, and any of these representations can be retrieved from a Rotation instance (see the various constructors and getters). In addition, a rotation can also be built implicitly from a set of vectors and their image.

This implies that this class can be used to convert from one representation to another one. For example, converting a rotation matrix into a set of Cardan angles from can be done using the following single line of code:
```
 double[] angles = new Rotation(matrix, 1.0e-10).getAngles(RotationOrder.XYZ); 
```
Focus is oriented on what a rotation do rather than on its underlying representation. Once it has been built, and regardless of its internal representation, a rotation is an operator which basically transforms three dimensional {@link Vector3D vectors} into other threedimensional {@link Vector3D vectors}. Depending on the application, the meaning of these vectors may vary and the semantics of the rotation also.

For example in an spacecraft attitude simulation tool, users will often consider the vectors are fixed (say the Earth direction for example) and the frames change. The rotation transforms the coordinates of the vector in inertial frame into the coordinates of the same vector in satellite frame. In this case, the rotation implicitly defines the relation between the two frames.

Another example could be a telescope control application, where the rotation would transform the sighting direction at rest into the desired observing direction when the telescope is pointed towards an object of interest. In this case the rotation transforms the direction at rest in a topocentric frame into the sighting direction in the same topocentric frame. This implies in this case the frame is fixed and the vector moves.

In many case, both approaches will be combined. In our telescope example, we will probably also need to transform the observing direction in the topocentric frame into the observing direction in inertial frame taking into account the observatory location and the Earth rotation, which would essentially be an application of the first approach.

These examples show that a rotation is what the user wants it to be. This class does not push the user towards one specific definition and hence does not provide methods like projectVectorIntoDestinationFrame or computeTransformedDirection. It provides simpler and more generic methods: {@link #applyTo(Vector3D) applyTo(Vector3D)} and {@link #applyInverseTo(Vector3D) applyInverseTo(Vector3D)}.

Since a rotation is basically a vectorial operator, several rotations can be composed together and the composite operation r = r₁ o r₂ (which means that for each vector u, r(u) = r₁(r₂(u))) is also a rotation. Hence we can consider that in addition to vectors, a rotation can be applied to other rotations as well (or to itself). With our previous notations, we would say we can apply r₁ to r₂ and the result we get is r = r₁ o r₂. For this purpose, the class provides the methods: {@link #applyTo(Rotation) applyTo(Rotation)} and{@link #applyInverseTo(Rotation) applyInverseTo(Rotation)}.

Rotations are guaranteed to be immutable objects.
@version $Revision: 1067500 $ $Date: 2011-02-05 21:11:30 +0100 (sam. 05 févr. 2011) $ @see Vector3D @see RotationOrder @since 1.2
org.apache.commons.math3.geometry.euclidean.threed.Rotation
This class implements rotations in a three-dimensional space.
Rotations can be represented by several different mathematical entities (matrices, axe and angle, Cardan or Euler angles, quaternions). This class presents an higher level abstraction, more user-oriented and hiding this implementation details. Well, for the curious, we use quaternions for the internal representation. The user can build a rotation from any of these representations, and any of these representations can be retrieved from a Rotation instance (see the various constructors and getters). In addition, a rotation can also be built implicitly from a set of vectors and their image.

This implies that this class can be used to convert from one representation to another one. For example, converting a rotation matrix into a set of Cardan angles from can be done using the following single line of code:
```
 double[] angles = new Rotation(matrix, 1.0e-10).getAngles(RotationOrder.XYZ); 
```
Focus is oriented on what a rotation do rather than on its underlying representation. Once it has been built, and regardless of its internal representation, a rotation is an operator which basically transforms three dimensional {@link Vector3D vectors} into other threedimensional {@link Vector3D vectors}. Depending on the application, the meaning of these vectors may vary and the semantics of the rotation also.

For example in an spacecraft attitude simulation tool, users will often consider the vectors are fixed (say the Earth direction for example) and the frames change. The rotation transforms the coordinates of the vector in inertial frame into the coordinates of the same vector in satellite frame. In this case, the rotation implicitly defines the relation between the two frames.

Another example could be a telescope control application, where the rotation would transform the sighting direction at rest into the desired observing direction when the telescope is pointed towards an object of interest. In this case the rotation transforms the direction at rest in a topocentric frame into the sighting direction in the same topocentric frame. This implies in this case the frame is fixed and the vector moves.

In many case, both approaches will be combined. In our telescope example, we will probably also need to transform the observing direction in the topocentric frame into the observing direction in inertial frame taking into account the observatory location and the Earth rotation, which would essentially be an application of the first approach.

These examples show that a rotation is what the user wants it to be. This class does not push the user towards one specific definition and hence does not provide methods like projectVectorIntoDestinationFrame or computeTransformedDirection. It provides simpler and more generic methods: {@link #applyTo(Vector3D) applyTo(Vector3D)} and {@link #applyInverseTo(Vector3D) applyInverseTo(Vector3D)}.

Since a rotation is basically a vectorial operator, several rotations can be composed together and the composite operation r = r₁ o r₂ (which means that for each vector u, r(u) = r₁(r₂(u))) is also a rotation. Hence we can consider that in addition to vectors, a rotation can be applied to other rotations as well (or to itself). With our previous notations, we would say we can apply r₁ to r₂ and the result we get is r = r₁ o r₂. For this purpose, the class provides the methods: {@link #applyTo(Rotation) applyTo(Rotation)} and{@link #applyInverseTo(Rotation) applyInverseTo(Rotation)}.

Rotations are guaranteed to be immutable objects.
@see Vector3D @see RotationOrder @since 1.2
org.jfree.chart.util.Rotation
org.jfree.util.Rotation
Represents a direction of rotation (CLOCKWISE or ANTICLOCKWISE). @author David Gilbert
org.terasology.math.Rotation
Rotation provides easy access to 90 degree increments of rotations - intended for block-related rotations.
Uses the fly weight pattern to cache the 64 combinations of rotation. @author Immortius
peasy.org.apache.commons.math.geometry.Rotation
This class implements rotations in a three-dimensional space.
Rotations can be represented by several different mathematical entities (matrices, axe and angle, Cardan or Euler angles, quaternions). This class presents an higher level abstraction, more user-oriented and hiding this implementation details. Well, for the curious, we use quaternions for the internal representation. The user can build a rotation from any of these representations, and any of these representations can be retrieved from a Rotation instance (see the various constructors and getters). In addition, a rotation can also be built implicitely from a set of vectors and their image.

This implies that this class can be used to convert from one representation to another one. For example, converting a rotation matrix into a set of Cardan angles from can be done using the followong single line of code:
```
 double[] angles = new Rotation(matrix, 1.0e-10).getAngles(RotationOrder.XYZ); 
```
Focus is oriented on what a rotation do rather than on its underlying representation. Once it has been built, and regardless of its internal representation, a rotation is an operator which basically transforms three dimensional {@link Vector3D vectors} into other threedimensional {@link Vector3D vectors}. Depending on the application, the meaning of these vectors may vary and the semantics of the rotation also.

For example in an spacecraft attitude simulation tool, users will often consider the vectors are fixed (say the Earth direction for example) and the rotation transforms the coordinates coordinates of this vector in inertial frame into the coordinates of the same vector in satellite frame. In this case, the rotation implicitely defines the relation between the two frames. Another example could be a telescope control application, where the rotation would transform the sighting direction at rest into the desired observing direction when the telescope is pointed towards an object of interest. In this case the rotation transforms the directionf at rest in a topocentric frame into the sighting direction in the same topocentric frame. In many case, both approaches will be combined, in our telescope example, we will probably also need to transform the observing direction in the topocentric frame into the observing direction in inertial frame taking into account the observatory location and the Earth rotation.

These examples show that a rotation is what the user wants it to be, so this class does not push the user towards one specific definition and hence does not provide methods like projectVectorIntoDestinationFrame or computeTransformedDirection. It provides simpler and more generic methods: {@link #applyTo(Vector3D) applyTo(Vector3D)} and{@link #applyInverseTo(Vector3D) applyInverseTo(Vector3D)}.

Since a rotation is basically a vectorial operator, several rotations can be composed together and the composite operation r = r₁ o r₂ (which means that for each vector u, r(u) = r₁(r₂(u))) is also a rotation. Hence we can consider that in addition to vectors, a rotation can be applied to other rotations as well (or to itself). With our previous notations, we would say we can apply r₁ to r₂ and the result we get is r = r₁ o r₂. For this purpose, the class provides the methods: {@link #applyTo(Rotation) applyTo(Rotation)} and{@link #applyInverseTo(Rotation) applyInverseTo(Rotation)}.

Rotations are guaranteed to be immutable objects.
@version $Revision: 627994 $ $Date: 2008-02-15 03:16:05 -0700 (Fri, 15 Feb2008) $ @see Vector3D @see RotationOrder @since 1.2
plotter.Rotation
purrpackagedemo.Transformation.Rotation

Examples of peasy.org.apache.commons.math.geometry.Rotation

      final double lookAtZ, final double distance) {
    this.p = parent;
    this.g  = pg;
    this.startCenter = this.center = new Vector3D(lookAtX, lookAtY, lookAtZ);
    this.startDistance = this.distance = distance;
    this.rotation = new Rotation();
    this.originalMatrix = parent.getMatrix((PMatrix3D)null);


    feed();


    rotateX = new DampedAction(this) {
      @Override
      protected void behave(final double velocity) {
        rotation = rotation.applyTo(new Rotation(Vector3D.plusI, velocity));
      }
    };


    rotateY = new DampedAction(this) {
      @Override
      protected void behave(final double velocity) {
        rotation = rotation.applyTo(new Rotation(Vector3D.plusJ, velocity));
      }
    };


    rotateZ = new DampedAction(this) {
      @Override
      protected void behave(final double velocity) {
        rotation = rotation.applyTo(new Rotation(Vector3D.plusK, velocity));
      }
    };


    dampedZoom = new DampedAction(this) {
      @Override

View Full Code Here

Examples of peasy.org.apache.commons.math.geometry.Rotation

  public void reset() {
    reset(300);
  }


  public void reset(final long animationTimeInMillis) {
    setState(new CameraState(new Rotation(), startCenter, startDistance),
        animationTimeInMillis);
  }

View Full Code Here

Examples of peasy.org.apache.commons.math.geometry.Rotation

    center = center.add(rotation.applyTo(new Vector3D(dx, dy, 0)));
    feed();
  }


  public void rotateX(final double angle) {
    rotation = rotation.applyTo(new Rotation(Vector3D.plusI, angle));
    feed();
  }

View Full Code Here

Examples of peasy.org.apache.commons.math.geometry.Rotation

    rotation = rotation.applyTo(new Rotation(Vector3D.plusI, angle));
    feed();
  }


  public void rotateY(final double angle) {
    rotation = rotation.applyTo(new Rotation(Vector3D.plusJ, angle));
    feed();
  }

View Full Code Here

Examples of peasy.org.apache.commons.math.geometry.Rotation

    rotation = rotation.applyTo(new Rotation(Vector3D.plusJ, angle));
    feed();
  }


  public void rotateZ(final double angle) {
    rotation = rotation.applyTo(new Rotation(Vector3D.plusK, angle));
    feed();
  }

View Full Code Here

Examples of peasy.org.apache.commons.math.geometry.Rotation

    feed();
  }


  public void setRotations(final double pitch, final double yaw, final double roll) {
    rotationInterps.cancelInterpolation();
    this.rotation = new Rotation(RotationOrder.XYZ, pitch, yaw, roll);
    feed();
  }

View Full Code Here

Examples of peasy.org.apache.commons.math.geometry.Rotation

      w2 = Math.sin(t * theta) / sinTheta;
    } else {
      w1 = 1.0 - t;
      w2 = t;
    }
    return new Rotation(w1 * a0 + w2 * b0, w1 * a1 + w2 * b1, w1 * a2 + w2 * b2, w1
        * a3 + w2 * b3, true);
  }

View Full Code Here

Examples of plotter.Rotation

    if (format.getClass().equals(DateNumberFormat.class)) {
      GregorianCalendar gc = new GregorianCalendar();
      gc.setTimeInMillis((long) value);
      label.setToolTipText(format.format(value) +" " + gc.get(Calendar.YEAR) );
    }
    Rotation labelRotation = getLabelRotation();
    if(labelRotation != null) {
      label.putClientProperty(Rotation.class.getName(), labelRotation);
    }
    label.setUI(MultiLineLabelUI.labelUI);
    label.setForeground(getForeground());

View Full Code Here

Examples of purrpackagedemo.Transformation.Rotation

  public void testTransformationsOnPoints() {
    Translation t = new Translation( 3, -2.5 );
    assertPointEquals( new Point( 3, -2.5 ), t.apply( Point.ORIGIN ));
    assertPointEquals( new Point( 4, -1.5 ), t.apply( new Point( 1, 1 ) ) );
    
    Rotation r = new Rotation( Math.PI / 2.0 );
    assertPointEquals( new Point( 0, 1 ), r.apply( new Point( 1, 0 )) );
    assertPointEquals( new Point( -2, 0 ), r.apply( r.apply( new Point( 2, 0 ))) );
    
    Expansion z = new Expansion( -2 );
    assertPointEquals( new Point( 14, -16 ), z.apply( new Point( -7, 8 )) );
  }

View Full Code Here

Examples of purrpackagedemo.Transformation.Rotation

  }
  
  @Test
  public void testAccidentally() {
    Point p = new Point( 0, -1 );
    Rotation r = new Rotation( Math.PI / 2);
    System.out.println( r.apply( p ));
    


  }

View Full Code Here

0 1 2 3 4 5

TOP

All source code are property of their respective owners. Java is a trademark of Sun Microsystems, Inc and owned by ORACLE Inc. Contact coftware#gmail.com.