PSN-L Email List Message

Subject: Re: nonlinearities
From: "Dave Nelson" davefnelson@.......
Date: Thu, 18 Aug 2011 13:59:44 -0000





From: Christopher Chapman=20
Sent: Thursday, August 18, 2011 11:38 AM
To: psnlist@.................
Subject: Re: nonlinearities


From: Dave Nelson davefnelson@.......
Subject: Re: nonlinearities


All,

The simple fact remains -- Feedback seismometers are the world standard. =
 No other technology can come anywhere near their performance and =
operational flexibility.
Their noise levels and bandwidth of the typical off the shelf instrument =
from several sources are such that the only area where significant =
improvement is desired relates to extremely long period performance for =
the study of whole earth modes at 1000 seconds and longer.
Most of the development activity is related to making smaller and less =
expensive instruments and greater flexibility in installation. One =
significant exception is Metrozet where a new instrument to replace the =
STS-1 is under development.
$$$$ Is that the only area where significant improvements are desired ? =
WHO sell these LESS expensive instruments, please ? And less expensive =
than what ? A new car maybe ?

The lowest cost  professional quality 3 axis force balance broadband =
costs about $8000 ( Nanometrics Trillium Compact).  My vertical force =
balance vertical can be built by a skilled amateur for a few hundred =
dollars. It is very low noise and has a flat frequency response from 30 =
Hz to 50 seconds and will operate over a ~50 Kelvin temperature range =
without re-centering.  It does require a very good site and proper =
installation in order to realize its low noise potential.  This is true =
for all low noise instruments.

The scientific community seems to choose the most expensive instruments =
when a lower cost instrument might do the job. It seems the higher the =
cost of your equipment the greater the credibility of your work.  Human =
nature I guess.  However ,for  research into the structure of the earth =
,excellent very long period performance is essential .  Clearly lower =
cost should be a goal. However, for the professional installation the =
instrument is not  usually the major cost item.=20

Non feedback instruments are a relic of the past or short period =
geophone or geophone-like instruments which have their niche in local =
event monitoring and the amateur community.
$$$$ The UK is covered by an official network of Willmore vertical =
seismometers. The sensor band is either variable 1 to 3 seconds or =
sometimes 20 seconds to 20 Hz, depending on the Model. But we have over =
400 horizontal school seismometers sensing from 5 Hz to 25 seconds =
producing signals comparable to the "professional" seismometers. You =
simply require reasonably good design and construction. See =
http://www.mindsetsonline.co.uk/images/Seismometer.pdf  Long period =
vertical seismometers are more difficult to make.

You make my point.   =20

 The optical open loop instrument is unlikely to have any success (in my =
opinion) simply because it will never be stable.  When I first read the =
paper I concluded the project had no chance of becoming an operational =
instrument but it was an interesting a academic exercise. Others with =
the best credentials in the business have shared that sentiment.
$$$$ If you add "in it's present form", I would agree with you. But go =
back a few centuries and "Others with the best credentials in the =
business" said that the world was flat !

Yes --  In its present form. However, I still have serious reservations' =
regarding the fundamental concept .The objective of zero power =
dissipation in the instrument case  can probably be met with a feedback =
design with much lower complexity and vastly greater stability.  The =
optical readout of the mass position is extremely complex. It requires =
measuring the instantaneous phase  of the optical signal to 1 degree or =
better.

Regarding creep effects --   When a spring is first installed in an =
instrument there will be  "pops" related to what is probably dislocation =
effects in the spring material . Their frequency will gradually reduce =
in time. The solution is too bake the assembly, with the spring at its =
operational stress, at ~ 160 C for several hours. This will essentially =
eliminate the effect.
$$$$ I wish it were that simple. Heat treating the spring under tension =
does greatly reduce the noise, but it doesn't eliminate it. You also =
have noise from the feedback circuit. Differentiating a signal is a =
noisy process. It could be a distinct advantage to combine active =
damping with passive damping, which is quieter.

Brett's analytical work and the actual performance of the instruments =
say  otherwise.    Passive damping will increase noise Not reduce noise. =
  I try to minimize passive damping and keep the open loop Q as high as =
possible. The ONLY SIGNIFICANT source of spring related noise is due to =
the temperature coefficient of  Young's modulus.  It  results in a =
signal proportional to the rate of change of temperature. =20

I will let Brett comment further.

My Best Regards to you Chris --It is good to hear from you.

Dave Nelson=20
Rolling Hills Estates , California=20










 

From: Christopher Chapman
Sent: Thursday, August 18, 2011 11:38 AM
To: psnlist@..............
Subject: Re: nonlinearities

From: Dave Nelson davefnelson@.......
Subject: Re:=20 nonlinearities

All,
 
The simple fact remains -- Feedback = seismometers=20 are the world standard.  No other technology can come anywhere near = their=20 performance and operational flexibility.
Their noise levels and = bandwidth of the=20 typical off the shelf instrument from several sources are such that = the=20 only area where significant improvement is desired relates to = extremely=20 long period performance for the study of whole earth modes at = 1000 seconds and longer.
Most of the development activity is = related to=20 making smaller and less expensive instruments and greater flexibility in = installation. One significant exception is Metrozet where a new = instrument to=20 replace the STS-1 is under development.
$$$$ Is that the only area where = significant=20 improvements are desired ? WHO sell these LESS expensive instruments, = please ?=20 And less expensive than what ? A new car maybe ?
 
The lowest cost  professional = quality 3 axis=20 force balance broadband costs about $8000 ( Nanometrics Trillium = Compact). =20 My vertical force balance vertical can be built by a skilled amateur for = a few=20 hundred dollars. It is very low noise and has a flat frequency response = from 30=20 Hz to 50 seconds and will operate over a ~50 Kelvin temperature range = without=20 re-centering.  It does require a very good site and proper = installation in=20 order to realize its low noise potential.  This is true for all low = noise=20 instruments.
 
The scientific community seems to = choose the=20 most expensive instruments when a lower cost instrument might do the = job. It=20 seems the higher the cost of your equipment the greater the credibility = of your=20 work.  Human nature I guess.  However ,for  = research=20 into the structure of the earth ,excellent very long period performance = is=20 essential .  Clearly lower cost should be a goal. However, for = the=20 professional installation the instrument is not  usually the major = cost=20 item.
 
Non feedback = instruments are a relic=20 of the past or short period geophone or geophone-like instruments = which have=20 their niche in local event monitoring and the amateur=20 community.
$$$$ The UK is covered by an=20 official network of Willmore vertical seismometers. The sensor band = is=20 either variable 1 to 3 seconds or sometimes 20 seconds to 20 Hz, = depending=20 on the Model. But we have over 400 horizontal school = seismometers sensing=20 from 5 Hz to 25 seconds producing signals comparable to=20 the "professional" seismometers. You simply require reasonably = good=20 design and construction. See http://www.mindsetsonline.co.uk/images/Seismometer.pdf  Long period vertical seismometers are more difficult to=20 make.
 
You make my point.   =20
 
 The optical open loop instrument = is unlikely=20 to have any success (in my opinion) simply because it will never be=20 stable.  When I first read the paper I concluded the project had no = chance=20 of becoming an operational instrument but it was an interesting a = academic=20 exercise. Others with the best credentials in the business have shared = that=20 sentiment.
$$$$ If you add "in it's present = form", I=20 would agree with you. But go back a few centuries and "Others with the = best=20 credentials in the business" said that the world was flat = !
 
Yes --  In its present form. = However, I still=20 have serious reservations' regarding the fundamental concept .The = objective of=20 zero power dissipation in the instrument case  can probably be met = with a=20 feedback design with much lower complexity and vastly greater = stability. =20 The optical readout of the mass position is extremely complex. It = requires=20 measuring the instantaneous phase  of the optical signal to 1 = degree=20 or better.
 
Regarding creep effects --   = When a=20 spring is first installed in an instrument there will be  "pops" = related to=20 what is probably dislocation effects in the spring material . Their = frequency will gradually reduce in time. The solution is too bake = the=20 assembly, with the spring at its operational stress, at ~ 160 C for = several=20 hours. This will essentially eliminate the effect.
$$$$ I = wish it were=20 that simple. Heat treating the spring under tension does greatly = reduce the=20 noise, but it doesn't eliminate it. You also have noise from the = feedback=20 circuit. Differentiating a signal is a noisy process. It could be a = distinct advantage to combine active damping with passive damping, which = is=20 quieter.
 
Brett's analytical work and the actual = performance=20 of the instruments say  otherwise.    Passive = damping=20 will increase noise Not reduce noise.   I try to minimize = passive=20 damping and keep the open loop Q as high as possible. The ONLY = SIGNIFICANT=20 source of spring related noise is due to the temperature coefficient = of =20 Young's modulus.  It  results in a signal proportional to = the=20 rate of change of temperature. 
 
I will let Brett comment=20 further.
 
My Best Regards to you Chris --It is = good to hear=20 from you.
 
Dave Nelson
Rolling Hills Estates , California=20
 
 
 
 
 
 
<= /DIV>

[ Top ] [ Back ] [ Home Page ]