replacing the power supply.
Aaron Parsons
510-406-4322 (cell)
On Wed, Dec 27, 2023 at 8:55 AM Tommy Alford wrote:
> Hello, we have a ROACH that we use as a correlator. It has been working
> great for the last 8 years or so but randomly while running the other day
> it shut itself of
isit
> https://groups.google.com/a/lists.berkeley.edu/d/msgid/casper/af99003f-574f-4593-3a08-995a3dbdbff0%40kiranshila.com
> .
>
>
>
> --
> https://katfs.kat.ac.za/~marc/
>
> --
> You received this message because you are subscribed to the Google Groups "
> ca
> To view this discussion on the web visit
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> .
>
--
Aaron Parso
ists.berkeley.edu.
> To post to this group, send email to casper@lists.berkeley.edu.
>
--
Aaron Parsons
510-406-4322 (cell)
Campbell Hall 425, UCB
--
You received this message because you are subscribed to the Google Groups
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interested.
https://aprecruit.berkeley.edu/apply/JPF01223
Thanks,
Aaron
--
Aaron Parsons
510-406-4322 (cell)
Campbell Hall 425, UCB
The CASPER PFB uses a sample NTAPS times, using a sliding window that jumps
by NCHAN time samples.
On Mon, Dec 5, 2016 at 7:33 AM Jayanth Chennamangalam
wrote:
> Hi Richard,
>
> In the VEGAS LBW modes, a sliding window is implemented. As you've pointed
> out, the existence of a pre-filtering sta
e Spiegel <
davespie...@projectfla.com> with an email briefly describing your relevant
experience.
--
Aaron Parsons
510-406-4322 (cell)
Campbell Hall 523, UCB
> The reason I'm asking is that if you lose any
> >
> > On 05-Dec-14 01:36 PM, Jonathan Weintroub wrote:
> >> Hello CASPERites,
> >>
> >> Has anyone implemented an _inverse_ PFB? That is a block taking
> channelized PFB data and reproducing the original time series.
> >>
> >> If so, is the code/mdl/yellow block available?
> >>
> >> Thanks,
> >>
> >> Jonathan
> >>
> >>
> >>
> >
>
>
>
--
Aaron Parsons
510-406-4322 (cell)
Campbell Hall 523, UCB
Hi CASPERites,
UC Berkeley has finally given me approval to recruit a postdoc for next
year to work on PAPER and HERA. Please circulate to anyone you think might
be interested!
https://aprecruit.berkeley.edu/apply/JPF00544
--
Aaron Parsons
510-406-4322 (cell)
Campbell Hall 523, UCB
h Phd,
> Gauribidanur Radio Observatory
> Indian Institute of Astrophysics
>
>
--
Aaron Parsons
510-306-4322
Hearst Field Annex B54, UCB
27;m looking for documents or publications discussing the math behind
> combining the parallel FFT results for the in-place FFT. Aaron has a paper
> <http://ieeexplore.ieee.org/stamp/stamp.jsp?tp=&arnumber=4840623> on
> this, but I was hoping for one with more detail.
>
> Thanks!
> Stevo
>
--
Aaron Parsons
510-306-4322
Hearst Field Annex B54, UCB
of
> three
> (assuming you remove the corner turn in the FFT).
>
> you can also put more inputs in parallel, as i mentioned in my previous
> email, to cut latency down by factors of 2, 4, 8,...
>
> best wishes,
>
> dan
>
>
--
Aaron Parsons
510-306-4322
Hearst Field Annex B54, UCB
array"
>> .
>> I have a question: Where could post this work?
>>
>> I was thinking in this journal: Journal of Astronomical Instrumentation
http://www.worldscientific.com/page/jai/submission-guidelines
>>
>> someone posted here, could I submit your paper?
>> can guide me?
>>
>> Cheers
>>
>> Katty
>
>
--
Aaron Parsons
510-306-4322
Hearst Field Annex B54, UCB
ay dios mio
On Tue, Mar 12, 2013 at 6:40 PM, Ryan Monroe wrote:
> That makes two of us! Viva la revolution!
>
>
> On 03/12/2013 06:35 PM, Dan Werthimer wrote:
>
>>
>> it's pretty loud where i'm sitting.
>>
>
>
--
Aaron Parsons
510-306-4322
Hearst Field Annex B54, UCB
Aaron
>
> *correction on my last post: *When I said R4DC ("radix-4, Delay
> Commutator"), I should have said R4MDC ("radix-4, multi-delay commutator"),
> to distinguish it from streaming FFTs which only process FFT's worth of
> data at a time.
>
> -
> (which are ) in a different fashion, by re-casting
> them as a split-radix FFT (look it up). Doing this is computationally
> about the same, but saves resources and memory... and is simpler if the
> size of is greater than 2^2.
>
>
> I hope this helps, Luke (and everyone else)!
>
>
> --Ryan Monroe
>
--
Aaron Parsons
510-306-4322
Hearst Field Annex B54, UCB
is re-invented and implemented
> > casper's parameterized parallel FFT, (about a decade after we did):
> >
> > "Using the Parallel FFT for Multigigahertz FPGA Signal Processing"
> >
> http://issuu.com/xcelljournal/docs/xcell_journal_issue_82/51?mode=wi
ured as dual
> port memories,
> so you can get the PFB reverse and forward coefficients both at the same
> time,
> from the same memory, almost for free, without any memory size penalty
> over single port,
>
> dan
>
>
>
>
> On Mon, Jan 21, 2013 at 3:18 PM, Aaron
1024 (see attached model file),
>> and it looks pretty promising: errors are a max of about 2.5%.
>>
>> Coupling this with symmetric coefficients could cut coefficient storage
>> to 1/8th, at the cost of a few extra adders for the interpolation filter.
>> Thoughts?
>>
>> Cheers
>> Danny
>>
>
>
--
Aaron Parsons
510-306-4322
Hearst Field Annex B54, UCB
The decision to split the SKA between South Africa and Australia is official:
http://www.skatelescope.org/news/dual-site-agreed-square-kilometre-array-telescope/
Low frequency is expected to be sited primarily in Australia, and mid
will be primarily in South Africa.
--
Aaron Parsons
510-306
big, others quickly copy it. Then you do
> something else. The trick is to do something else."
>
>
> On Mon, 29 Nov 2010, John Ford wrote:
>
>> Hi all.
>>
>> Do any of you have any xilinx designs that implement SPEAD protocol
>> packets over 10 GbE?
>>
>> John
>>
>>
>>
>>
>
>
--
Aaron Parsons
510-406-4322 (cell)
Campbell Hall 523, UCB
AS = 0
> Set UNICODE = 0
> Set WX_CONFIG = "/opt/wx/bin/wx-config"
>
> $ python2.6 setup.py config
> $ python2.6 setup.py build
> $ sudo python2.6 setup.py install
> $ cd /usr/lib/python2.6/site-packages
> $ cp wx* /usr/lib64/python2.6/site-packages/
>
> Add the following line to /etc/ld.so.conf:
> /opt/wx/lib
> and then run ldconfig.
>
>
--
Aaron Parsons
510-406-4322 (cell)
Campbell Hall 523, UCB
and compact dewar utilizing a cryogen-free adiabatic demagnetization
> refrigerator (ADR) allows the camera to be deployed quickly at Naysmith or
> Coude foci at a variety of telescopes. A highly expandable software defined
> radio (SDR) readout that can scale up to much larger arrays has been
verrides the built-in "size" function.
Have the guys at Mathworks never heard of namespaces? This is getting
ridiculous.
--
Aaron Parsons
510-406-4322 (cell)
Campbell Hall 523, UCB
on is different from the
command line (I think I'm sending the same iterrupt signal), but
something's definitely disagreeing with bkexecd.
2) Can bkexecd be restarted without rebooting the entire system? If
so, how? There's nothing in /etc/init.d/ to this effect.
--
Aaron Parsons
510
bit words transferred per second as around 3.5 million. I don't know the
>> frequency at which the bus runs, but I suspect it is far greater than 3.5
>> MHz hence my comment about room for improvement.
>>
>> Dave
>>
>> P.S. I don't know how conventional or official it is, but I use lowercase
>> 'b' for "bit" and uppercase 'B' for "byte".
>>
>>
>>
>
>
>
>
>
>
--
Aaron Parsons
510-406-4322 (cell)
Campbell Hall 523, UCB
o others don't have to bump into it ?
>
> Mel.
>
> On 4/28/10, Aaron Parsons wrote:
>> So commenting out all the lines in /etc/syslog.conf and then rebooting
>> seems to have done the trick. I now see ~7.8MB/s read times. Yay!
>>
>> Muchas gracias!
>>
&
; by reading small quantities of data from different BRAMs etc.
>
> If you try to dump the whole DRAM using tcpborphserver's "bulkread" command,
> you should achieve something close to 3.5MB/s across the network using the
> Python KATCP and the wrapper in corr.
>
> Jas
ven't found anything
with lsof that indicates what may be writing to /proc/kmsg. I'm left
thinking that maybe this logging is compiled into the kernel.
Does anyone know what is cause such lousy file I/O performance on the
ROACH? If it is indeed a problem with excessive logging, how do
with utilization if you use a lot of software registers
> (eg the packetized correlator).
> These changes apply from svn revision 2945.
> Cheers,
> David
> --
> David George
> Karoo Array Telescope
> Tel: +27 21 531-7282
> Email: david.geo...@ska.ac.za
>
--
Aaron Parsons
510-406-4322 (cell)
Campbell Hall 523, UCB
ulated it. I've never used
> Glenn's so can't comment on that one.
>
> Jason
>
> On 07 Apr 2010, at 10:19, Suraj Gowda wrote:
>
>> Xilinx style fix: Use Glenn's vector accumulator from the GAVRT library.
>>
>> On Apr 7, 2010, at 7:32 AM, Aaron
2010, at 7:32 AM, Aaron Parsons wrote:
>
>> It looks like this block is not correctly configured in the library.
>> Volunteers to fix/test?
>>
>> --
>> Aaron Parsons
>>
>> 510-406-4322 (cell)
>> Campbell Hall 523, UCB
>>
>
>
--
Aaron Parsons
510-406-4322 (cell)
Campbell Hall 523, UCB
It looks like this block is not correctly configured in the library.
Volunteers to fix/test?
--
Aaron Parsons
510-406-4322 (cell)
Campbell Hall 523, UCB
set up like this? (I'm using the 10.1 tools on
> otto.eecs.berkeley.edu, in case it helps)
>
> Thanks,
> Jonathan Landon
>
>
>
--
Aaron Parsons
510-406-4322 (cell)
Campbell Hall 523, UCB
Another thing to think about is that for signals that are strong relative to
the number of bits you are using to represent them, you can see the effects
of the asymmetric distribution of values around zero for two's complement
numbers. For example, in the CASPER correlators, where we use four bits
output from X engines. This involves
doing away with parallel polarizations (they should just be treated as
separate antennas), and having real/imag samples multiplexed onto the
same bus. This should reduce to some extent the logic used in
handling and re-multiplexing these wide busses. Any objections?
--
Aaron Parsons
510-406-4322 (cell)
Campbell Hall 523, UCB
g list. I put up everything I have on the subject at
> http://casper.berkeley.edu/wiki/Logos
>
> Any improvements are welcome (especially ones that incorporate the new
> 'Collaboration' language)!
>
> Regards,
>
> Andrew
>
>
>
>
--
Aaron Parsons
510-406-4322 (cell)
Campbell Hall 523, UCB
<>
If preloading the library fixes the problem, then the less hackish way
of getting it to automatically preload is to add it to the startup.m
script in the directory that you launch matlab from.
On Sep 14, 2009, at 10:28 PM, Suraj Gowda
wrote:
Hi Ron,
The 'dspsigops' library is not loade
u try setting your SGCORECACHE environment variable to some temp
> directory where you know you have read/write permissions?
>
> Thanks,
> Henry
>
>
> Aaron Parsons wrote:
>
>> Maybe I'm flummoxed because I'm a windows noob, but I'm trying to compile
>>
a part of the SgGenerateCores.pm script that seems to be looking
for cached results to copy around for cores, so it seems like the file
existing should be an error.
Any ideas?
On Tue, Sep 8, 2009 at 11:53 AM, Aaron Parsons wrote:
> Maybe I'm flummoxed because I'm a windows noob, but
C:\WINDOWS\TEMP/binary_counter_virtex2p_7_0_78a3dd824f4df0df: File exists at
C:/Xilinx/10.1/DSP_Tools/sysgen/scripts/SgGenerateCores.pm line 551
but C:\WINDOWS\TEMP is inaccessible to me, and other designs compile without
access to it. What am I missing here?
--
Aaron Parsons
510-406-4322 (cell)
Campbell Hall 523, UCB
it is currently implemented, it does not seem to work. I am
> using the green 7.1 blocks. Has anyone successfully used this feature (i.e.
> made a single input biplex FFT of length greater than MaxCoeffNum, 2^11 by
> default)?
> Thanks,
> Glenn
>
--
Aaron Parsons
510-406-4322 (cell)
787-878-2612 x329 (arecibo office)
787-721-3991 (home)
I wanted to share what I've done
>> so far. It is not yet tested. The code is here:
>> http://casper.berkeley.edu/svn/trunk/caltech/lib10.1/map_init.m
>>
>> Glenn
>
>
--
Aaron Parsons
510-406-4322 (cell)
787-878-2612 x329 (arecibo office)
787-721-3991 (home)
inputs down to 1 complex output.
> Please let me know if you've seen a problem like this and have an idea as to
> where to start looking to fix it. I seached the map output to see if
> anything obvious was being optimized out but didn't find anything.
>
> Hope this helps someo
>>> Thanks for clarifying Aaron, I will go through the block carefully
>>> tonight and see if I can trace down the "cross-coupling."
>>> Glenn
>>>
>>> On Thu, Sep 18, 2008 at 6:12 PM, Aaron Parsons
>>> wrote:
>>>>
>>
unctionality of the block since a biplex
> pfb_fir block should be equivalent two single input pfb_fir blocks.
> Can someone more clearly explain the functionality of the FFT block?
> Thank you,
> Glenn
>
--
Aaron Parsons
510-406-4322 (cell)
787-878-2612 x329 (arecibo office)
787-721-3991 (home)
; testing if the bits are all '1' or '0' respectively?
>
> There is probably a clever answer to this or I have misunderstood something
> somewhere. Could someone have a look at this and let me know what they
> think.
>
> Thanks
> Andrew
>
--
Aaron Parsons
510-406-4322 (cell)
787-878-2612 x329 (arecibo office)
787-721-3991 (home)
> > >>
> > >> --
> > >> Oren Milgrome
> > >> University of California - Berkeley
> > >> Radio Astronomy Lab 601 Campbell Hall
> > >> Berkeley, CA 94720-3411
> > >> mobile: 510 368 6857 office: 510 642 5509
> > >> lab: 510 642 0381 fax: 510 642 3411
> > >> email: o...@berkeley.edu
> > >>
> > >>
> > >
> >
> >
> > --
> > Oren Milgrome
> > University of California - Berkeley
> > Radio Astronomy Lab 601 Campbell Hall
> > Berkeley, CA 94720-3411
> > mobile: 510 368 6857 office: 510 642 5509
> > lab: 510 642 0381 fax: 510 642 3411
> > email: o...@berkeley.edu
> >
> >
>
--
Aaron Parsons
510-406-4322 (cell)
787-878-2612 x329 (arecibo office)
787-721-3991 (home)
using some of Aaron's python from the corr
> python module.
>
> Thanks.
>
> John
>
>
>
>
--
Aaron Parsons
510-406-4322 (cell)
787-878-2612 x329 (arecibo office)
787-721-3991 (home)
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