PSN-L Email List Message
Subject: Re: Vertical vs. Horz.
From: ChrisAtUpw@.......
Date: Tue, 22 Dec 2009 21:32:59 EST
In a message dated 22/12/2009, brett3nt@............. writes:
>1 I know this is an over simplification, but does the P arrives at an
>angle (bottom to top) and this influences the spring?
What you suggest I believe is true, that P waves may have some vertical
component, though there might possibly be another contribution related to
something that Randall mentioned. We frequently see P waves on the
verticals, sometimes quite strongly, which might in part relate to the
fact
that when something gets squeezed in one direction, it will expand
somewhat
to the sides.
Hi Brett,
It may have even more to deal with the curved paths that the rays
travel inside the spherical earth!
This ratio of the sideways expansion to the original amount
of compression is called Poisson's Ratio, which for many materials is
about
1/3. As a horizontal P wave expands and compresses the earth, it may
possibly be causing additional vertical motion due to that effect, which
you should see on the vertical (though I don't know what Poisson's ratio
might be for dirt).
It is rock that you need to check.
>The obvious advantage of a vertical is they see many earthquakes, the
>disadvantage they are limited and also see a lot of other things which
are
>not earthquakes. All of my verticals have been 1 to 2.5 seconds.
> A typical vertical sensor recording will have a trace of 20
>mins vs. a 3 hours trace on the Lehman.
This must be an observational error. The noise on an uncased,
uncompensated vertical may be over 20x that on a horizontal. The noise on verticals
is only less at longer periods since atmospheric noise is excluded in
contemporary seismometers by the hermetically sealed case.
From what I have seen, much of the surface-wave energy of large teleseisms
is in the region of 18 to 20 seconds, and sometimes longer. 20 seconds
will see a lot, while 40 or 50 seconds can often see somewhat more.
You definitely need the sensor response flat out to 20 seconds. A
Lehman with this range will see 40 second waves at 1/4 their true amplitude.
The roll-off in a vertical may be more rapid, depending on the type /
feedback.
One problem is that there is so much microseism noise in the six-second
region and also around 12 seconds. I generally use a 0.08Hz (12.5 second)
4 or 6 pole low pass filter to cut out most of that noise, while allowing
through much of the big-quake frequencies. An instrument that can only go
down to 6 seconds will unfortunately be quite good at displaying the noise
while missing most teleseism surface waves.
Yup! I only see 10 second noise on a few days each month in the UK.
The six second noise batters us all the time!
> One's location has an influence on which sensor type works for them
The only problem is that the movement of a seismometer in response to an
error force, such as from small temperature changes, etc. increases as
1/Frequency^2
Even more critical are air density changes effecting a vertical sensor
and also wind noise. Temperatures should change quite slowly inside an
insulating case, assuming that the sun does not shine on it!
It is way harder to make a stable instrument for 50
seconds than for 10 or 20 or 6. Long period verticals almost certainly
need to use a feedback design if they are going to be sensitive enough to
see distant quakes while at the same time, insensitive enough to
temperature and other variations to not wander off to maximum output.
Uh, Uh! Now define what you are calling long period?
The Roberts' period compensating amplifier circuit is probably the
easiest technique for amateurs to use. It has constant gain from the LP filter
down to ~ the resonant frequency rf of the vertical sensor, at say 1/2 Hz.
See _http://jclahr.com/science/psn/roberts/index.html_
(http://jclahr.com/science/psn/roberts/index.html) It was first used on geophones.
Below this to about rf / 10, (= 1/20 Hz) the gain increases as 1 / f^2, so
compensating the f^2 falling output to give a flat characteristic. So you
can extend a 2 second period vertical sensor out to about 20 seconds quite
easily. Extending the period much beyond x10 quickly runs into noise
problems with a coil + magnet velocity detector. You need two of these stages
with maximum gains of x10 (total x100 at 20 seconds) linked by a 2 pole high
pass filter at ~ 1/30 Hz. Lennartz use a system like this. So do I and it
works fine.
Direct digital period compensation probably works best with 24 bit
ADCs. The French use it on their schools system. 16 bit ADCs may only show a
few counts (1/100 the rest of the signal) at x10 period, unless the gain is
quite high and it may be partly masked by electronic noise.
Regards,
Chris Chapman
In a message dated 22/12/2009, brett3nt@............. writes:
>1 I know this is an over simplification, but does=
=20
the P arrives at an
>angle (bottom to top) and this influen=
ces=20
the spring?
What you suggest I believe is true, that P=
waves=20
may have some vertical
component, though there might possibly be ano=
ther=20
contribution related to
something that Randall mentioned. We=
=20
frequently see P waves on the
verticals, sometimes quite strongly,=
which=20
might in part relate to the fact
that when something gets squeezed=
in one=20
direction, it will expand somewhat
to the sides.
Hi Brett,
It may have even more to deal with the curved=
paths=20
that the rays travel inside the spherical earth!
This=20
ratio of the sideways expansion to the original amount
of compressio=
n is=20
called Poisson's Ratio, which for many materials is about
1/3. =
As a=20
horizontal P wave expands and compresses the earth, it may
possibly=
be=20
causing additional vertical motion due to that effect, which
you sho=
uld=20
see on the vertical (though I don't know what Poisson's ratio
might=
be for=20
dirt).
It is rock that you need to check.<=
/DIV>
>The=20
obvious advantage of a vertical is they see many earthquakes, the=20
>disadvantage they are limited and also see a lot of other things=
which=20
are
>not earthquakes. All of my verticals have been 1 to 2.=
5=20
seconds.
> A typical vertical sensor recording will have a=
trace=20
of 20
>mins vs. a 3 hours trace on the Lehman.
This must be an observational error. The nois=
e on=20
an uncased, uncompensated vertical may be over 20x that on a horizontal.=
The=20
noise on verticals is only less at longer periods since atmospheric=
noise=20
is excluded in contemporary seismometers by the hermetically sealed case.=
=20
From=20
what I have seen, much of the surface-wave energy of large teleseisms is=20
in the region of 18 to 20 seconds, and sometimes longer. 20 second=
s=20
will see a lot, while 40 or 50 seconds can often see somewhat=20
more.
You definitely need the sensor response =
flat=20
out to 20 seconds. A Lehman with this range will see 40 second waves at 1/=
4=20
their true amplitude. The roll-off in a vertical may be more rapid, depend=
ing on=20
the type / feedback.
One=20
problem is that there is so much microseism noise in the six-second
=
region=20
and also around 12 seconds. I generally use a 0.08Hz (12.5 second)=
4=20
or 6 pole low pass filter to cut out most of that noise, while allowing=
=20
through much of the big-quake frequencies. An instrument that=
can=20
only go
down to 6 seconds will unfortunately be quite good at displa=
ying=20
the noise
while missing most teleseism surface waves.
Yup! I only see 10 second noise&n=
bsp;on=20
a few days each month in the UK. The six second noise batters us all the=
=20
time!
> One's location has an influence on which sensor=
type=20
works for them
The only problem is that the movement of a seismom=
eter=20
in response to an
error force, such as from small temperature change=
s,=20
etc. increases as
1/Frequency^2
Even more critical are air density changes=20
effecting a vertical sensor and also wind noise. Temperatures should chang=
e=20
quite slowly inside an insulating case, assuming that the sun does no=
t=20
shine on it!
It is=20
way harder to make a stable instrument for 50
seconds than for 10 or=
20 or=20
6. Long period verticals almost certainly
need to use a feedba=
ck=20
design if they are going to be sensitive enough to
see distant quake=
s=20
while at the same time, insensitive enough to
temperature and other=
=20
variations to not wander off to maximum output.
Uh, Uh! Now define what you are calling long=
=20
period?
The Roberts' period compensating amplifier ci=
rcuit=20
is probably the easiest technique for amateurs to use. It has constant gai=
n from=20
the LP filter down to ~ the resonant frequency rf of the vertical sen=
sor,=20
at say 1/2 Hz. See
http://jclahr.co=
m/science/psn/roberts/index.html =20
It was first used on geophones.=20
Below this to about rf / 10, (=3D 1/20 Hz) th=
e gain=20
increases as 1 / f^2, so compensating the f^2 falling output to give a fla=
t=20
characteristic. So you can extend a 2 second period vertical sensor out to=
about=20
20 seconds quite easily. Extending the period much beyond x10 quickly runs=
into=20
noise problems with a coil + magnet velocity detector. You need two=
of=20
these stages with maximum gains of x10 (total x100 at 20=20
seconds) linked by a 2 pole high pass filter at ~ 1/30 Hz. Lennartz=
use a=20
system like this. So do I and it works fine.
Direct digital period compensation probably=
works=20
best with 24 bit ADCs. The French use it on their schools system. 16 bit=
ADCs=20
may only show a few counts (1/100 the rest of the signal) at x10 period,=
unless=20
the gain is quite high and it may be partly masked by electronic=20
noise.
Regards,
Chris Chapman
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