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PlanetPhysics/Gradient

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The gradient is the vector sum of the resultant rate of increase of a scalar funcion V and is denoted βˆ‡V. It represents a directed rate of change of V. A directed derivative or vector derivative of V, so to speak. In cartesian coordinates

βˆ‡V=βˆ‚Vβˆ‚x𝐒̂+βˆ‚Vβˆ‚y𝐣̂+βˆ‚Vβˆ‚z𝐀̂

It is common to regard βˆ‡ as the gradient operator which obtains a vector βˆ‡V from a scalar function V of position in space.

βˆ‡V=(βˆ‚βˆ‚x𝐒̂+βˆ‚βˆ‚y𝐣̂+βˆ‚βˆ‚z𝐒𝐀̂)V

Thus it is easy to work with just the gradient operator

βˆ‡=βˆ‚βˆ‚x𝐒̂+βˆ‚βˆ‚y𝐣̂+βˆ‚βˆ‚z𝐀̂

This symbolic operator βˆ‡ was introduced by Sir W. R. Hamilton. It has been found by experience that the monosyllable del is so short and easy to pronounce that even in complicated formulas in which βˆ‡ occurs a number of times no inconvenience to the speaker or hearer arises from the repetition. βˆ‡V is read simply as "del V."

Coordinate System Independence

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Although this operator βˆ‡ has been defined as

βˆ‡V=βˆ‚βˆ‚x𝐒̂+βˆ‚βˆ‚y𝐣̂+βˆ‚βˆ‚z𝐀̂

so that it appears to depend upon the choice of the axes, it is in reality independent of them. This would be surmised from the interpretation of βˆ‡ as the magnitude and direction of the most rapid increase of V. To demonstrate the independence take another set of axes, 𝐒̂, 𝐣̂, 𝐀̂ and a new set of variables x, y, z referred to them. Then βˆ‡ referred to this system is

βˆ‡=βˆ‚βˆ‚x𝐒̂+βˆ‚βˆ‚y𝐣̂+βˆ‚βˆ‚z𝐀̂

(Please Insert PROOF here...)

Leaving behind the proof of coordinate system independence, here is the gradient opertor in the most common coordinate systems.

Cartesian Coordinates

βˆ‡V=βˆ‚Vβˆ‚x𝐒̂+βˆ‚Vβˆ‚y𝐣̂+βˆ‚Vβˆ‚z𝐀̂

Cylindrical Coordinates

βˆ‡V=βˆ‚Vβˆ‚r𝐫̂+1rβˆ‚Vβˆ‚ΞΈπœ½Μ‚+βˆ‚Vβˆ‚z𝐳̂

Spherical Coordinates

βˆ‡V=βˆ‚Vβˆ‚r𝐫̂+1rβˆ‚Vβˆ‚Ο•π“Μ‚+1rsinΟ•βˆ‚Vβˆ‚ΞΈπœ½Μ‚

References

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[1] Wilson, E. "Vector Analysis." Yale University Press, New Haven, 1913.

This entry is a derivative of the Public domain work [1].