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Re: [time-nuts] True Position GPSDP + Rb X72

K
KA2WEU@aol.com
Sun, Sep 24, 2017 12:50 PM

Meaning home=home ?  just kidding. ,long staying constant

73 de Ulrich

In a message dated 9/24/2017 8:45:35 A.M. Eastern Daylight Time,
magnus@rubidium.dyndns.org writes:

Hi,

On 09/24/2017 02:30 PM, Bob kb8tq wrote:

Hi

On Sep 23, 2017, at 9:39 PM, Hal Murray  hmurray@megapathdsl.net wrote:

kb8tq@n1k.org said:

If the main use is feeding test gear (and  not direct synthesis) an Rb

may do

pretty well. Most  instruments assume a dirty reference signal and

clean it

up  internally.

What's the bandwidth on the typical  cleanup PLL?  How well does that

match

the noise from a  Rb?

It’s like any other PLL with noise involved. You look at  the noise of

the Rb, the

noise of the particular cleanup oscillator,  and your system

requirements. In some

cases that comes out to a few  seconds. For Time Nut grade with a really

good

OCXO you are at some  pretty long numbers.

If the Rb starts at 2x10^-11 at 1 second  and goes down by square root

tau: At

100 seconds you are at 2x10^12.  Still not as good as a really good OCXO.

At

10,000 seconds you might  get to 2x10^-13 (but probably will not). Your

OCXO

likely will climb  out of the “parts in 10^-13” range before 10,000

seconds.

Lots of fun.

Once up on a time, you could order the OSA cesiums width  different
oscillators, essentially to buy into different balances between
oscillator cost and performance. The time constant is adapter with
regards to oscillator type, as the trade off shifts.

I can't recall  any other cesium or rubidium that did this, but HP
upgraded oscillators at  one point for this reason  too.

Cheers,
Magnus


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Meaning home=home ? just kidding. ,long staying constant 73 de Ulrich In a message dated 9/24/2017 8:45:35 A.M. Eastern Daylight Time, magnus@rubidium.dyndns.org writes: Hi, On 09/24/2017 02:30 PM, Bob kb8tq wrote: > Hi > > >> On Sep 23, 2017, at 9:39 PM, Hal Murray <hmurray@megapathdsl.net> wrote: >> >> >> kb8tq@n1k.org said: >>> If the main use is feeding test gear (and not direct synthesis) an Rb may do >>> pretty well. Most instruments assume a dirty reference signal and clean it >>> up internally. >> >> What's the bandwidth on the typical cleanup PLL? How well does that match >> the noise from a Rb? > > It’s like any other PLL with noise involved. You look at the noise of the Rb, the > noise of the particular cleanup oscillator, and your system requirements. In some > cases that comes out to a few seconds. For Time Nut grade with a really good > OCXO you are at some pretty long numbers. > > If the Rb starts at 2x10^-11 at 1 second and goes down by square root tau: At > 100 seconds you are at 2x10^12. Still not as good as a really good OCXO. At > 10,000 seconds you might get to 2x10^-13 (but probably will not). Your OCXO > likely will climb out of the “parts in 10^-13” range before 10,000 seconds. > > Lots of fun. Once up on a time, you could order the OSA cesiums width different oscillators, essentially to buy into different balances between oscillator cost and performance. The time constant is adapter with regards to oscillator type, as the trade off shifts. I can't recall any other cesium or rubidium that did this, but HP upgraded oscillators at one point for this reason too. Cheers, Magnus _______________________________________________ time-nuts mailing list -- time-nuts@febo.com To unsubscribe, go to https://www.febo.com/cgi-bin/mailman/listinfo/time-nuts and follow the instructions there.