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Aerospace Science
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is a parameter.
,
,
or Dxf and Duf or fx
and fy.
)


represents a wavelength
traveling
in the positive x-direction with phase velocity c. This concept is to be distinguished
from signal velocity, group velocity, and the velocity of fluid parcels. See
velocity of propagation.

, centered around wavelength
,
per unit area of blackbody surface at temperature T; c1 and c2
are radiation constants. This
law was derived theoretically by M. Planck in 1901.

is the pressure gradient along the axis of the cylinder. The velocity profile
across the cylinder is seen to be parabolic, and this relation affords a convenient
experimental means of determining a fluid's viscosity. Also called Hagen-Poiseuille
flow. Compare Couette flow. 
, and
is the average density (or rate) with which the events occur. When
is large, the Poisson distribution approaches the normal distribution. The
binomial distribution approaches the Poisson when the number of events
n becomes large and the probability of success P becomes small
in such a way that
.

is the Laplacian
operator;
is a scalar function
of position; and F is a given function of the independent space variables.
For the special case F = 0, the Poisson equation reduces to the Laplace
equation. See relaxation method. 
which a line (radius vector) joining the given point and the origin makes with a fixed reference line, called the polar axis. The relations between rectangular Cartesian coordinates and polar coordinates are 

is the environmental lapse rate. The subscript 0 denotes values at the planet's
surface.
are related according to the formula 
is a constant and the subscript
0 denotes initial values of the variables. Therefore pressure and
temperature are similarly related: 
)
,
where F is the force;
is the del-operator;
and
is the potential. A force
which may be so expressed is said to be conservative, and the work done against
it in motion from one given equipotential surface to another is independent
of the path of the motion. See Gibbs function,
potential energy.
is most easily defined in relation to the potential temperature
as 
is the potential temperature; T is the Kelvin temperature; p is pressure, millibars; R is the gas constant for dry air; and cp is the specific heat or dry air at constant pressure. See equivalent potential temperature, adiabatic process.

and the
power spectrum of f(t) is
.
Here n take integral values and the spectrum is discrete. The total
energy of the periodic function is infinite, but the power, or energy per
unit period, is finite. 
. Geometrically, the probability integral equals the area under this density curve between -z and z , where z is an arbitrary positive number. Often denoted by the symbol erf z (read error function of z ) the probability integral is defined thus: 
.
)
p)