colatitude's Usage Examples:

In a spherical coordinate system, a colatitude is the complementary angle of a given latitude, i.

as usual by the longitude (angle φ {\displaystyle \varphi } ) and the colatitude (angle θ {\displaystyle \theta } ) then φ = c θ , c > 0 {\displaystyle.

if in absolute value the declination is more than the colatitude, in the corresponding hemisphere) The object is below the horizon even.

temperature T eff {\displaystyle T_{\text{eff}}} can then be found at a given colatitude θ {\displaystyle \theta } from the local effective gravity: T eff ( θ.

The polar angle may be called colatitude, zenith angle, normal angle, or inclination angle.

can be broken down into the product of three functions of the radius, colatitude (or polar) angle, and azimuth: ψ ( r , θ , ϕ ) = R ( r ) P ( θ ) F ( ϕ.

They are the same as the colatitudes measured in turns times 16.

for R E {\displaystyle R_{E}} ), and θ {\displaystyle \theta } is the colatitude measured from the north magnetic pole (or geomagnetic pole).

r^{\prime }} is the radius, θ ′ {\displaystyle \theta ^{\prime }} is the colatitude and ϕ ′ {\displaystyle \phi ^{\prime }} is the azimuthal angle.

}}{\overline {G_{o}\otimes _{o}S}},} where θ {\displaystyle \theta } is colatitude and λ {\displaystyle \lambda } is longitude, t {\displaystyle t} is time.

Similar to Korn and Korn (1961), but uses colatitude θ = 90° - ν instead of latitude ν.

rotating with angular speed Ω that depends on both the radius r and the colatitude θ Ω = − g t ϕ g ϕ ϕ = r s α r c ρ 2 ( r 2 + α 2 ) + r s α 2 r sin 2 ⁡.

λ is the magnetic latitude (equal to 90° − θ) where θ is the magnetic colatitude, measured in radians or degrees from the dipole axis m is the dipole moment.

the tube design and detector mounting, adding azimuth in addition to colatitude.

Like Korn and Korn (1961), but uses colatitude θ = 90° - ν instead of latitude ν.

{\displaystyle \phi } is East longitude, θ {\displaystyle \theta } is colatitude (the polar angle), a {\displaystyle a} is the Earth's radius, g ℓ m {\displaystyle.

normalization constant, and θ and φ represent colatitude and longitude, respectively.

In particular, the colatitude θ, or polar angle, ranges from 0 at the.

When the longitude and colatitude of a point P on a sphere are denoted by q and ƒ and if P moves so that.

declinations or polar distances, it was necessary to determine the observatory's colatitude, or distance of the celestial pole from the zenith, by observing the upper.