For the VCO, how about a reactance modulator. They were very popular for the 
sweeping local oscillator in many a panadapter. Or perhaps one of the voice 
coil based wobbulators?

John  WA4WDL


---- Bob Camp <[email protected]> wrote: 
> Hi
> 
> I believe that if you dig into it, the correlator is either running quite 
> fast (in serial mode) or is pretty large (parallel processing). 
> 
> Since you know neither the code nor the doppler (no almanac) you are sweeping 
> both the frequency and the code.
> 
> The VCO is a bit of a challenge (as mentioned earlier). Prior art was 
> basically a motor driven capacitor. Resolution / backlash / dead band are all 
> obvious issues. Not quite so obvious are dead spots in the capacitor it's 
> self and reversals in the tuning characteristic. It's the ratio of the tuning 
> range to the running accuracy that is the driver.
> 
> Bob
> 
> On Jun 24, 2013, at 8:40 PM, Jim Lux <[email protected]> wrote:
> 
> > On 6/24/13 3:01 PM, Bob Camp wrote:
> >> Hi
> >> 
> >> I'm not so sure that "slow" would work. With all the sat's moving various 
> >> directions all the time, I suspect you need to do a solution fairly 
> >> quickly. If you don't the stale data messes up the solution. Also you need 
> >> the correlators to work fast enough to lock on to an essentially unknown 
> >> code before the sat is out of view.
> >> 
> > The sliding correlator is pretty easy, and would lock up quite quickly. 
> > Basically, you need to have a vacuum tube PN generator to generate the 
> > correct Gold/Kasami code for the satellite in question (e.g. you need 32 of 
> > those generators). Each generator has a pair of 10 stage shift registers in 
> > it.  I haven't looked in my copy of Millman and Taub, but I think you could 
> > probably build the shift register with 2*N devices (maybe N tubes, if you 
> > use dual triodes/pentodes, what have you).  There might also be better 
> > choices for the tubes that have some form of latching behavior (thyratrons 
> > maybe..)
> > 
> > You slide the correlator until it locks, and then it automatically also 
> > tracks the doppler of that S/V.  I assume you'd use some sort of early/late 
> > tracker rather than a tau dither. I don't know what you'd use as the VCO, 
> > but there is probably some scheme (after all, FM transmitters existed 
> > before the invention of the Varactor solid state device)
> > 
> > You can track the raw observables (code phase and Doppler) without needing 
> > to do a nav solution at all. And those observables don't change all that 
> > quickly (after all, the Doppler only changes a few kHz during many hours as 
> > the satellite goes from horizon to horizon).
> > 
> > The trick is in how do you get the code phase into your nav algorithm. It's 
> > easy to get a pulse at 1 ms intervals when the code epoch comes by, but you 
> > really want to get a range estimate, and that means figuring out where you 
> > are in the bigger scheme of things. and, then getting that ingested into 
> > whatever computation scheme you're using.
> > 
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