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Lesson Notes - For Teachers
Lesson Notes - For Teachers

... ither of the ways displayed will work for this activity. The point is that we will have the three angles of the triangle available to make the discovery. • Next, have students place the three angles on the second piece of blank paper that was distributed. • Have students line up the angles s ...
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Estimating Angle Measures - Nelson Math K-8

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... 2.) __________ A triangle that has all equal sides. 3.) __________ The name of the two congruent sides of an isosceles triangle. 4.) __________ A triangle that has sides that are all different lengths ...
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Unwrapped Standards: G.CO.10 - Prove theorems about triangles

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Geometry Chapter 4 Practice Test Name

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Standard 3 - Briar Cliff University

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Wilkes-Geometry-Unit 3-Parallel and Perpendicular Lines

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Chapter 4 Review HW KEY

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Angle Bisector Theorem (notes)

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Geometry UNIT 4

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Section 4.6

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Parallel lines, parallel planes, skew lines. Transversal, consecutive

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2006 Mississippi Math Framework

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Slide 15

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Wilkes-Geometry-Unit 3-Parallel and Perpendicular Lines

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McDougal Geometry chapter 6 notes

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Euler angles



The Euler angles are three angles introduced by Leonhard Euler to describe the orientation of a rigid body. To describe such an orientation in 3-dimensional Euclidean space three parameters are required. They can be given in several ways, Euler angles being one of them; see charts on SO(3) for others. Euler angles are also used to describe the orientation of a frame of reference (typically, a coordinate system or basis) relative to another. They are typically denoted as α, β, γ, or φ, θ, ψ.Euler angles represent a sequence of three elemental rotations, i.e. rotations about the axes of a coordinate system. For instance, a first rotation about z by an angle α, a second rotation about x by an angle β, and a last rotation again about z, by an angle γ. These rotations start from a known standard orientation. In physics, this standard initial orientation is typically represented by a motionless (fixed, global, or world) coordinate system; in linear algebra, by a standard basis.Any orientation can be achieved by composing three elemental rotations. The elemental rotations can either occur about the axes of the fixed coordinate system (extrinsic rotations) or about the axes of a rotating coordinate system, which is initially aligned with the fixed one, and modifies its orientation after each elemental rotation (intrinsic rotations). The rotating coordinate system may be imagined to be rigidly attached to a rigid body. In this case, it is sometimes called a local coordinate system. Without considering the possibility of using two different conventions for the definition of the rotation axes (intrinsic or extrinsic), there exist twelve possible sequences of rotation axes, divided in two groups: Proper Euler angles (z-x-z, x-y-x, y-z-y, z-y-z, x-z-x, y-x-y) Tait–Bryan angles (x-y-z, y-z-x, z-x-y, x-z-y, z-y-x, y-x-z). Tait–Bryan angles are also called Cardan angles; nautical angles; heading, elevation, and bank; or yaw, pitch, and roll. Sometimes, both kinds of sequences are called ""Euler angles"". In that case, the sequences of the first group are called proper or classic Euler angles.
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