As soon as we are online in the southern hemisphere we will have more work
than we can handle.
If they were truly worried about not having enough WU's to go around they
would not have disconnected from Arecibo.
http://setiathome.ssl.berkeley.edu/sstatus.html
Terry
"Alan Kubiak" <theku...@worldnet.att.net> wrote in message
news:EBhB7.137469$3d2.4...@bgtnsc06-news.ops.worldnet.att.net...
Seti have tried to balance a lot of things. The greater than expected number
of volunteers has allowed the same amount of data to be processed at least
twice (as in any worthy scientific experiment) and allowed the search to be
widened. Since we don't know where to look, looking in more places because
there are more volunteers with better CPUs can only be good.
At the end of the day you are a volunteer, so you have to make up your own
mind.
Regards,
Roy Bamford
--
There are two classes of computer users,
those who do backups and
those who have never had a hard drive fail.
"Alan Kubiak" <theku...@worldnet.att.net> wrote in message
news:EBhB7.137469$3d2.4...@bgtnsc06-news.ops.worldnet.att.net...
Not using a personal computer for a noble scientific cause is wasting
electrons.
--
Jonathan
Co-Webmaster and Designer of:
www.windows-eXPerience.co.uk
"red" <r...@xmission.com> wrote in message
news:3BD60D44...@xmission.com...
Now that I'm aware that I can talk about it, I suppose I could fill everyone
in on the current direction things are going (colored a bit with the direction
I'd like them to go).
The first big thing is that observing at Parkes will be different than at
Arecibo. We'll be tagging along on the primary receivers, so we won't be
slewing across the sky like we do at Arecibo. Gaussian fitting goes away
in this observing mode. On the other hand we're on the same spot of sky
for longer, so we can bump up max FFT length to 256k and look at even
narrower bandwidths.
The current plan is for a workunit to still be 1M samples, but to frequency
step across the workunit. The first 256K samples will be at in one frequency
band. The next 256K samples will be in a band 2.5 MHz higher. So in essence
each workunit will cover about 40 kHz rather than the current 10 kHz. Going
to 256K will increase processing time an as yet undetermined amount.
I'm pushing for the new client to be capable of processing Arecibo work
units, so I'm hoping that we'll still keep looking in the north without needing
some people to keep running the old version of the client.
We're still nailing down the details. And we haven't even started client
development at this point. (We're pretty strapped for cash right now, too.
A lot of our funding sources are feeling the economic pinch and some
donations that were to be matched by the university haven't (yet) come
through. So if anyone has some loose change...)
Of course, we send our thanks to those who have given cpu time, advice,
money, equipment, etc.
Eric
--
Eric Korpela | An object at rest can never be
kor...@ssl.berkeley.edu | stopped.
<a href="http://setiathome.ssl.berkeley.edu/~korpela">Click for home page.</a>
Eric, can you give us a rough idea when we may see some of this
coming down the pike - the new software, the new workunits,
etc... Thanks.