Brooke

Yes but the accuracy would suffer due to observer related effects.
However when used with a CCD camera or equivalent the accuracy should improve 
somewhat much as adding a TV camera to a transit circle improved its accuracy. 
I had a personal tour of the USNO setup on Black- Birch/Altimarloch during 
their southern hemisphere campaign during the 1980's. 

Bruce
> On 27 March 2019 at 20:39 Brooke Clarke <[email protected]> wrote:
> 
> 
> Hi Bruce:
> 
> Would the David White 60 Degree Pendulum Astrolabe also work?
> https://prc68.com/I/PendulumAstrolabe.shtml
> 
> -- 
> Have Fun,
> 
> Brooke Clarke
> https://www.PRC68.com
> http://www.end2partygovernment.com/2012Issues.html
> axioms:
> 1. The extent to which you can fix or improve something will be limited by 
> how well you understand how it works.
> 2. Everybody, with no exceptions, holds false beliefs.
> 
> -------- Original Message --------
> > The Danjon impersonal astrolabe is perhaps better suited to accurate 
> > measurements:
> > https://www.nzmuseums.co.nz/collections/3267/objects/3380/astrolabe
> >
> > Bruce
> >> On 27 March 2019 at 15:48 Tom Van Baak <[email protected]> wrote:
> >>
> >>
> >> BobH wrote:
> >>>> This would be an excellent project for time-nuts to verify.  First, a
> >>>> better explanation of John Harrison’s method is in order.  A vertical
> >>>> window edge is not sufficient - a second vertical reference at a
> >>>> distance is required - Harrison used a chimney on a neighbor's house.
> >> Agreed! The project is the perfect intersection of amateur astronomy and 
> >> amateur timekeeping. Surely, a couple of people on the list could 1) 
> >> attempt to verify the Harrison method, and 2) determine what the limits of 
> >> its accuracy are, say, with little effort vs. with hard work vs. with 
> >> extreme dedication.
> >>
> >> JimL wrote:
> >>> To get 1 second accuracy, you need 360/86400 = 0.004 degree
> >>> measurements. That's 0.073 milliradian - 1 cm  at 140 meter distance.
> >>>
> >>> I'm not sure an "edge" is sharp enough (diffraction, etc.), although
> >>> your eye is pretty good at "deconvolving" the linear equivalent of an
> >>> Airy disk/rings.
> >> Keep in mind too that one can take more than one star reading per night. 
> >> Any identifiable star that crosses your edge is a recordable timing event 
> >> that evening. So, in theory, if you measure N stars you get sqrt(N) 
> >> improvement in accuracy per day.
> >>
> >> I want to encourage anyone to study the problem and help solve the riddle, 
> >> either by uncovering existing professional or amateur literature or by 
> >> actually trying this at home. It boils down to how accurately can you 
> >> measure earth rotation using the Harrison method.
> >>
> >> To put this in time nuts context, precision timekeeping prior to the 
> >> middle of the 20th century was always a form of "Earth Disciplined 
> >> Oscillator". Not unlike a GPSDO, your observatory's pendulum clock kept 
> >> accurate time short-term and star tracking (earth rotation) kept accurate 
> >> time long-term. The ADEV's crossed just like a GPSDO.
> >>
> >> The short-term ADEV of a really good pendulum clock is here:
> >>
> >> http://leapsecond.com/pend/shortt/
> >>
> >> The long-term ADEV of earth rotation is here:
> >>
> >> http://leapsecond.com/museum/earth/
> >>
> >> So the performance of a DIY earth disciplined oscillator would be a 
> >> combination of the two.
> >>
> >> /tvb
> >>
> >>
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>

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