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Re: [10GBASE-CX4] comments on latest CX4 revision



Mike,
    I've added a comment to Steve's about the jitter.  See below between the <HAB>s.

Howard
 

"Dreyer, Steve" wrote:

   Part 1.1    Type: Plain Text (text/plain)
           Encoding: quoted-printable
Mike,
 
My answers to your comments below in blue.
 
Steve

-----Original Message-----
From: Mike Jenkins [mailto:jenkins@lsil.com] 
Sent: Friday, February 28, 2003 4:56 PM
To: DOVE,DANIEL J (HP-Roseville,ex1)
Cc: 'clarkf@mxim.com'; 'stds-802-3-10GBCX4@ieee.org'
Subject: Re: [10GBASE-CX4] comments on latest CX4 revision


Dan, 

I share Clark's concerns.  The only related presentation I found for
February (cx4_electrical_specs_02_18_03_Raleigh.pdf) showed simulations,
not hardware. 


*       These simulations used up all the space in the template, passing
only when the pre-emphasis was adjusted a couple percent (which is easy
to do in simulations, but tough, slow and expensive in silicon).  

          The original template was based on simulations from myself and
Howard Baumer, and there was plenty of margin
          against these simulations. . Zeev Roth from Mysticom then
contributed the more detailed simulations for the 
          presenatation.  Zeev's simulations were deemed to be close to
worst case, so we tentatively decided to keep 
          the template limits that barely encompased Zeev's results.
The template can be adjusted further, but the
          group needs to see sim results to be able to do that, if you
have some specific results which show problems,
          please submit to the group so those can be factored in.  
          
          As far as pre-emphasis tolerance goes, there is some
allowance.  In case there is any confusion, a 
         waveform is first normalized in amplitude so that the flat
pre-emphasis section is sitting on 50% point.
         So, the actual pre-emphasis value is that 50% point relative to
the peak in the template.  The peak amplitude
         template varies from 0.875 to 1.175.  Calculating this out
shows that the pre-emphasis can be between
         42.5-57.5 percent and meet the template.  The group thought
this was reasonable from an implementation
         standpoint.  Of course, these numbers can be  adjusted if
somneone has  data/results to indicate a problem. 

*       The need to change the pre-emphasis was due to modelling 2
inches of PCB.  What if it's 3 inches instead?  or a different
dielectric?  or a different package?  

      The group spent a lot of time debating how much "system" tolerance
to build in to the spec.  It was decided that
      2" of FR4 was a reasonable goal.  This doesn't preclude anyone
from building an IC that accomodates
     longer lengths and different materials, as long as the spec is met
at TP2 anything can be done.

*       Assumptions in this simulation included perfect impedance
matching and no reflections.  I very much doubt that a GigaCN-to-SMA
adapter board would meet those assumptions.  

     Agree.  No one had any reflection data to present.  It was
discussed, and most felt that reflections might require
     an opening up of the template along the flat pre-emphasis section.
But it was decided to leave as is pending 
     sim results showing a problem and solution. 

*       No tolerance is allowed for jitter or amplitude noise. 

      The DJ spec of 0.18UI was factored in the template.  The RJ=0.17UI
part was was kept as a separate spec.
      See working paper draft 3.1.


<HAB>
    The Rj is assumed to be taken out of the measurement via averaging of the measured waveform.  This is a very common practice that most high BW digital sampling scopes can do.  Because of this the template does not need to contain Rj. As Steve stated above we have a limit on Rj that will need to be measure seperately.
<HAB>


*       Margin for amplitude noise is 10% max, including ringing &
reflections.  

      This was addressed by allowing a lot of room on the top of the
template on the short pulse section.
      The amplitude limits go from 0.875 to 1.175, which everyone
thought was adequate to address ringing and
      refrlections.  If someone brings in more data to show a problem,
the template can be adjusted accordingly.

*       Depending on how you model it, slow risetimes (0.41 UI) either
just make it or just miss with everything else perfect. 

     Agreed.  At last meeting, the  group decided to add an additional
separate rise and fall time spec of 
    60-130ps (same as XAUI), this was added to working paper 3.1.
  
Apologies if I've missed a presentation with actual hardware compared to
this template.  But if we're proceeding without any hardware experience,
I am frankly concerned that this approach will be a measurement
nigntmare.  
 
As far as measurement goes, it is true that doing any measurement
degrades the signal being observed, but 
commonly the effects of the measuring equipment are subtracted from the
result to determine what the observed
signal actually is.   This is true of XAUI measuremnets today where
everyone routinely subtracts the effects
 of SMA connectors, loss of scope cables, degradation due to FR4, etc.
 
 Regards, 
Mike 

"DOVE,DANIEL J (HP-Roseville,ex1)" wrote: 


Hi Clark, 

I believe a lot of your questions would have been addressed 
at our meetings. We have had numerous presentations with 
measurements of cable assemblies and devices where the first 
thing that is done, is determine the impact of the connectors 
and PC board, and other impairments on the measurement. 


Nobody is claiming this is easy, that is not required. It is 
necessary to ensure compliance that we have a transmitter that 
meets an objective template, and a channel that meets a set of 
objective specs, and a receiver that works when connected to 
the two former items. Verification is required, but those of 
us who have been working on this have spent a substantial 
amount of time doing just that. 


The reason we spec'ed TP2 at the back side of the mated 
interface was specifically so that we could get a physical 
point as a reference plane. 


Regards, 


Dan 


-----Original Message----- 
From: Clark Foley [mailto:clarkf@mxim.com] 
Sent: Thursday, February 27, 2003 10:30 AM 
To: 'ddprocurve@antelecom.net'; 'stds-802-3-10GBCX4@ieee.org' 
Subject: RE: [10GBASE-CX4] comments on latest CX4 revision 


Dan, 


Has such a correction for impairments been demonstrated at 3.125Gb/s? 


Clark 


On Wednesday, February 26, 2003 10:11 PM, ddprocurve@antelecom.net 
[SMTP:ddprocurve@antelecom.net] wrote: 
> 
> Hi Clark, 
> 
> We discussed this and the conclusion was that there will be some 
impairment 
> caused by the fixturing (loss, etc) but that must be calibrated out by
the 
> user. We did not want to get into mandating how much loss, what kind
of 
> SMAs, etc. Rather, we spec the signal at the interface and rely upon
the 
> user to be able to make that measurement. 
> 
> This is consistent with 1000BASE-T and other 802.3 technologies where
the 
> measurement requires some calibration by the user to compensate for
probe 
> effects. 
> 
> Dan 
> > 
> > 
> >54.7.3.6 Differential Output Template and Figure 54-3 
> >The interconnect from the MDI to the scope for measuring against this

> >template has not been adequately described.  I could not find any 
> >information on the plumbing.  A tight template like this one must be 
> spec'd 
> >along with the interconnect hardware. 
> > 
> >Please consider readily available adapters and cables for this.  I 
suggest 
> 
> >that the test interface be comprised of a 1m, 24AWG cable to connect 
> >between the MDI and a GigaCN-to-SMA adapter board.  If you don't have
one 


> >of these boards yet, you will soon!  From the SMA to the scope, we
can 
use 
> 
> >short, high quality cable.  This is easy and convenient. 
> > 
> > 
> >Regards, 
> >Clark Foley 
> >Maxim Integrated Products 
> >(503) 547-2018 
> > 
> >

-- 

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