Examples of using Cartesian coordinates in English and their translations into Turkish
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What? What? Cartesian coordinates.
Cartesian coordinates. what? what?
What? What? Cartesian coordinates.
Cartesian coordinates. of course. coded cartesian. .
And it's the standard basis for two-dimensional Cartesian coordinates.
Coded Cartesian coordinates.
He was measuring the stars' radial velocity,the distance in parsecs, And the cartesian coordinates.
Coded Cartesian coordinates.
And they do it intentionally in physics books,because you don't have to do it using Cartesian coordinates, using x's and y's.
Coded cartesian coordinates. Cartesian coordinates. .
The analytic geometry developedby René Descartes(1596-1650) allowed those orbits to be plotted on a graph, in Cartesian coordinates.
All right, now they want to convert from polar to Cartesian coordinates, and so they give us the polar function r is equal to 4 sine of theta.
Cartesian coordinates-- and actually, they can apply to more than just 2 dimensions.
These coordinates may be derived from a set of Cartesian coordinates by using a transformation that is locally invertible(a one-to-one map) at each point.
I have enhanced the viewing matrix… the yaw, pitch and roll… to give us the exact position and orientation of our baby. Yeah.to track both the Cartesian coordinates and three altitude angles.
Of course, coded cartesian coordinates. Cartesian coordinates.
In calculus and related areas of mathematics, a linear function from the real numbers to thereal numbers is a function whose graph(in Cartesian coordinates with uniform scales) is a line in the plane.
The viewing matrix to track both the Cartesian coordinates the exact position and orientation of our baby.- Yeah. I have enhanced and three altitude angles, the yaw, pitch and roll to give us.
The ephemerides are updated every 30 minutes using data from the Ground Control segment;they use Earth Centred Earth Fixed(ECEF) Cartesian coordinates in position and velocity, and include lunisolar acceleration parameters.
If Cartesian coordinates in SI units are used, then the components of the position four-vector are given by: x0 t, x1 x, x2 y, and x3 z, where t is time in seconds, and x, y, and z are distances in meters.
Each element is created and manipulated numerically;essentially using Cartesian coordinates for the placement of key points, and then a mathematical algorithm to connect the dots and define the colors.
Here we will suppose these coordinates can be related to a Cartesian coordinate system by a set of functions: x j x j( x, y, z,…), j 1,…, n,{\displaystyle x^{ j}= x^{ j}( x,\ y,\ z,\\dots),\quad j=1,\\dots,\ n,} where x, y, z, etc. are the n Cartesian coordinates of the point.
Generalized coordinates and constraints In Newtonian mechanics, one customarily uses all three Cartesian coordinates, or other 3D coordinate system, to refer to a body's position during its motion.
This article provides a few of the easier ones to follow in the context of special relativity, for the simplest case of a Lorentz boost in standard configuration, i.e. two inertial frames moving relative to each other at constant(uniform) relative velocity less than the speed of light,and using Cartesian coordinates so that the x and x′ axes are collinear.
For example, in 3-D Euclidean space and using Cartesian coordinates; the coordinate vector A(A1, A2, A3)(Ax, Ay, Az) shows a direct correspondence between the subscripts 1, 2, 3 and the labels x, y, z.
In flat spacetime and using Cartesian coordinates, if one combines this with the symmetry of the stress-energy tensor, one can show that angular momentum is also conserved: 0( x α T μ ν- x μ T α ν), ν.{\displaystyle 0=(x^{\alpha}T^{\mu\nu}-x^{\mu}T^{\alpha\nu})_{,\nu}.\!} When gravity is non-negligible or when using arbitrary coordinate systems, the divergence of the stress-energy still vanishes.
We could associate an algebra to our geometry using a Cartesian coordinate system made of two lines, and represent points of our plane by vectors.
In general, in a Cartesian coordinate system xi on a Euclidean space, the partial derivatives∂/∂xi are orthonormal with respect to the Euclidean metric.