[Frost] Bank lists and disk volume for g9b cooking

[Ken Livingston]

Hi Franz,
I don't remember making bos files with the pol info last time, only a 
dst. but looking at the cooking scripts it seems that is was done.
For making the polarization tables it would be good to have the pol_dst 
files on disk (from running dstmaker_pol). Last time we captured that 
stuff as it came out of the cooking and bbftp'd it over to Glasgow.  
Banks needed for the pol dsts are at least.:
"HEAD","RC26","STN0","STN1","STRE","TAGE","TAGR","EPIC","TESC","RFT "

Hope to see you next week?

Cheers,
Ken


On 09/29/2012 02:21 AM, Franz Klein wrote:
> Hi,
> for the upcoming pass1 cooking of all files of g9b I compiled the lists
> of banks copied into output files and made an estimate of the required
> disk volume.
> Please make your comments and suggestions!
> Franz
>
> (A) Disk space requirement for ca. 20,000 files (g9b runs):
> AnaHistFiles 11.6MB/file -> 230GB
> LOG-files, Trip-files ~90kB/file -> 1.9GB
> Helicity-checks  ~2.6MB/file -> 52GB (zipped -> 14GB)
> SKIMS DST_Kp 50-60MB/file -> 1.2TB
> DSTgpid 260-300MB/file ->6TB
> NT_piN 18-20MB/file->400GB
> ROOT DST 600-700MB/file ->14TB (will be copied to tape silo, not sure
> whether we can keep them on disk)
> BOS-files 4-5GB/file ->90TB (will only be kept on tape silo, not on disk)
>
>
> (B) output from cooking:
> (a) BOS output: cooked_xxxx.Axx.Bxx
> from raw data: HEAD, EPIC, TESC, HLS, TRGS, RC26, TGBI, RFT, EC1, EC,
> ECT, SC, SCT, STN0, STN1, TGTL, TGTR, TAGE (TGTL, TGTR, TAGE could be
> skipped for linearly polar. data),
> detector result banks: CL01, EC01, ECHB, SCRC, STRE, TAGR, TRKS, TBER,
> TDPL, DHCL, MVRT, VERT,
> particle id banks: PART TBID, GPID, HEVT, EVNT, DCPB, TRPB, ECPB, LCPB,
> SCPB, STPB, TGPB
>
> (b) BOS output: Pol_xxxx.Axx (only for linearly polar. data):
> HEAD, EPIC, TESC, TRGS, RC26, RFT, TAGE, TAGR, STN0, STN1, STRE, (?
> TGTL, TGTR ?)

>
> (c) ROOTbeer output: DST_xxxxx.Axx.Bxx.root
> from raw data: HEAD, EPIC, RC26, TGBI, RFT, EC1, EC, ECT, SC, SCT, STN0,
> STN1,
> result banks: CL01, EC01, ECHB, SCRC, STRE, TAGR, TBER, TDPL, MVRT,
> VERT, PART, TBID, GPID,
>        HEVT, EVNT, DCPB, TRPB, ECPB, LCPB, SCPB, STPB, TGPB
>
> (d) SKIMS Kplus: DST_Kp_xxxxx.Axx.Bxx.root
> same as ROOTbeer DST but cuts:
> at least 1 particle with Beta>bmin_K && Beta<bmax_K && Pmom>0.1 && Pmom<2.5
>    using EVNT (beta and Pmom) with
>    bmax_K= Pmom/sqrt(Pmom*Pmom+0.42*0.42)+0.05;
>    bmin_K = Pmom/sqrt(Pmom*Pmom+0.6*0.6)-0.05;
>
> (e) SKIMS: DSTgpid_xxxxx.Axx.Bxx.root
> banks: HEAD, EPIC, GPID, TBID, ECHB, SCRC, STRE, TAGR, MVRT, VERT
>
> (f) SKIMS: ROOTntuple NT_piN_xxxx_Axx.root
> using banks: HEAD, TGBI, EVNT, MVRT, DCPB, TAGR, SCPB, STPB
>    keeping a single pos. particle and up to 2 neutrals in a ROOTntuple
>
>
>
>


-- 
=======================================================
Ken Livingston

Dept. of Physics & Astronomy,        Tel: +44 141 330 6428
University of Glasgow,               Fax: +44 141 330 5889
Glasgow G12 8QQ.
Scotland. UK.
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