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/*****************************************************************************
* *
* BLACKMAN.SPL Copyright (C) 2004,2010 DSP Development Corporation *
* All Rights Reserved *
* *
* Author: Randy Race *
* *
* Synopsis: Multiplies a series with a Blackman Window *
* *
* Revisions: 19 Mar 2004 RRR Creation *
* 21 Jul 2010 RRR symmetry flag *
* *
*****************************************************************************/
#if @HELP_BLACKMAN
BLACKMAN
Purpose: Multiplies a series with a 3 Point Blackman window
Syntax: BLACKMAN(s, ampflag, "sym")
s - A series or array
ampflag - Optional, an integer, the correction factor.
0: do not correct amplitude (default)
1: correct amplitude
2: correct RMS
3: correct mean squared amplitude
"sym" - Optional. A string, the symmetry mode.
"symmetric" : Starting and ending points are equal
(default).
"periodic" : Periodically extended window. Conforms
to ISO standard.
Alternate Syntax:
BLACKMAN(N, ampflag, "sym")
N - An integer, the length of the window.
ampflag - Optional, an integer, the correction factor.
0: do not correct amplitude (default)
1: correct amplitude
2: correct RMS
3: correct mean squared amplitude
"sym" - Optional. A string, the symmetry mode.
"symmetric" : Starting and ending points are equal
(default).
"periodic" : Periodically extended window. Conforms
to ISO standard.
Returns: A series or array
Example:
W1: gsin(1000, .001, 45)
W2: spectrum(blackman(W1))
W3: spectrum(blackman(W1, 1))
The MAX of W2 == 0.539 and the MAX of W3 == 1.0. The amplitude
of the spectrum in W3 has been corrected to take into account
amplitude effects of the Hamming window.
Example:
blackman(1000, "periodic")
returns a 1000 point periodic blackman window.
Remarks:
If the input is an integer rather than a series, the N
point blackman window is returned.
If ampflag == 1, the correction factor is the mean of
the spectral window. This assures that the spectrum of a
sinusoid of amplitude 1.0 has a peak of 1.0.
If ampflag == 2, the correction is applied as follows:
w = blackman(s) * rms(s) / rms(blackman(s))
sqrt(area(psd(w))) == rms(s) approximately
If ampflag == 3, the correction is applied as follows:
w = blackman(s) / sqrt(win * win / length(win))
where win is the windowing function.
The "sym" flag controls the window symmetry as follows:
"Symmetric" sets the first and last points to be equal.
An N point symmetric window can be constructed by creating
an N-1 point periodic window and setting the Nth point to
the value of the first point.
"Periodic" or "iso" creates a periodic window function
useful in spectrum analysis applications. "Periodic" or
"iso" conforms to the ISO 18431-1 standard for windowing
functions.
See GBLACKMAN for more details on the Blackman window.
See Also:
Flattop
Gblackman
Hamming
Hanning
Kaiser
Winfunc
#endif
/* multiply a series with a blackman window */
SERIES blackman(s, ampflag, sym)
{
return(winfunc(5, s, ampflag, sym));
}