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Linshizhi
ffmpeg.wasm-core
Commits
d20902fd
Commit
d20902fd
authored
Feb 10, 2019
by
Reto Kromer
Committed by
Gyan Doshi
Feb 10, 2019
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doc/filters: fix typos
Signed-off-by:
Gyan Doshi
<
ffmpeg@gyani.pro
>
parent
9ec1f763
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doc/filters.texi
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d20902fd
...
...
@@ -431,7 +431,7 @@ Range is between 0 and 1.
@
end
table
@
section
acontrast
Simple
audio
dynamic
range
com
m
pression
/
expansion
filter
.
Simple
audio
dynamic
range
compression
/
expansion
filter
.
The
filter
accepts
the
following
options
:
...
...
@@ -605,8 +605,8 @@ The lower value, the more samples will be detected as impulsive noise.
@
item
b
Set
burst
fusion
,
in
percentage
of
window
size
.
Allowed
range
is
@
code
{
0
}
to
@
code
{
10
}.
Default
value
is
@
code
{
2
}.
If
any
two
samples
deteced
as
noise
are
spaced
less
than
this
value
then
any
sample
inbetween
those
two
samples
will
be
also
detected
as
noise
.
If
any
two
samples
detec
t
ed
as
noise
are
spaced
less
than
this
value
then
any
sample
in
between
those
two
samples
will
be
also
detected
as
noise
.
@
item
m
Set
overlap
method
.
...
...
@@ -1220,7 +1220,7 @@ Set max allowed Impulse Response filter duration in seconds. Default is 30 secon
Allowed
range
is
0.1
to
60
seconds
.
@
item
response
Show
IR
frequency
re
ponse
,
magnitude
(
magenta
)
and
phase
(
green
)
and
group
delay
(
yellow
)
in
additional
video
stream
.
Show
IR
frequency
re
sponse
,
magnitude
(
magenta
),
phase
(
green
)
and
group
delay
(
yellow
)
in
additional
video
stream
.
By
default
it
is
disabled
.
@
item
channel
...
...
@@ -1382,7 +1382,7 @@ Z-plane zeros/poles, polar degrees
@
item
r
Set
kind
of
processing
.
Can
be
@
code
{
d
}
-
direct
or
@
code
{
s
}
-
serial
cascading
.
Defaul
s
is
@
code
{
s
}.
Can
be
@
code
{
d
}
-
direct
or
@
code
{
s
}
-
serial
cascading
.
Defaul
t
is
@
code
{
s
}.
@
item
e
Set
filtering
precision
.
...
...
@@ -10534,7 +10534,7 @@ max value instead of calculating Minkowski distance.
@item sigma
The standard deviation of Gaussian blur to be applied on the scene. Must be
chosen in the range [0,1024.0] and default value = 1. floor( @var{sigma} * break_off_sigma(3) )
can'
t
be
e
uq
al
to
0
if
@
var
{
difford
}
is
greater
than
0.
can'
t
be
e
qu
al
to
0
if
@
var
{
difford
}
is
greater
than
0.
@
end
table
@
subsection
Examples
...
...
@@ -18858,7 +18858,7 @@ Default value for each plane is @code{0 0 0 0 1 0 0 0 0}.
@item 3rdiv
Set multiplier for calculated value for each plane.
If unset or 0, it will be sum of all matrix elements.
The option value must be a
n
float number greater or equal to @code{0.0}. Default value is @code{1.0}.
The option value must be a float number greater or equal to @code{0.0}. Default value is @code{1.0}.
@item 0bias
@item 1bias
...
...
@@ -18866,7 +18866,7 @@ The option value must be an float number greater or equal to @code{0.0}. Default
@item 3bias
Set bias for each plane. This value is added to the result of the multiplication.
Useful for making the overall image brighter or darker.
The option value must be a
n
float number greater or equal to @code{0.0}. Default value is @code{0.0}.
The option value must be a float number greater or equal to @code{0.0}. Default value is @code{0.0}.
@end table
...
...
@@ -19136,7 +19136,7 @@ the cpu version tonemap currently. A setting of 0.0 disables this option.
@item threshold
The tonemapping algorithm parameters is fine-tuned per each scene. And a threshold
is used to detect whether the scene has changed or not. If the distance beween
is used to detect whether the scene has changed or not. If the distance be
t
ween
the current frame average brightness and the current running average exceeds
a threshold value, we would re-calculate scene average and peak brightness.
The default value is 0.2.
...
...
@@ -19558,7 +19558,7 @@ Set outer coloring mode.
It shall assume one of following values:
@table @option
@item iteration_count
Set iteration coun
d
mode.
Set iteration coun
t
mode.
@item normalized_iteration_count
set normalized iteration count mode.
@end table
...
...
@@ -22479,7 +22479,7 @@ This filter is primarily created for reversing processed @ref{showspectrum}
filter
outputs
,
but
can
synthesize
sound
from
other
spectrograms
too
.
But
in
such
case
results
are
going
to
be
poor
if
the
phase
data
is
not
available
,
because
in
such
cases
phase
data
need
to
be
recreated
,
usually
its
just
recreated
from
random
noise
.
it
'
s just recreated from random noise.
For best results use gray only output (@code{channel} color mode in
@ref{showspectrum} filter) and @code{log} scale for magnitude video and
@code{lin} scale for phase video. To produce phase, for 2nd video, use
...
...
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