STAR Correlations and Fluctuations PWG

[James Dunlop <dunlop AT bnl.gov>]

Hmm.  That's  interesting.   There's something wrong  with the magnetic field 
readout
for that run.  If I look at the runlog
https://online.star.bnl.gov/RunLogRun18/index.php?r=19158007
it says

STAR Magnet       100,000,000.0 Amps   

which would be pretty impressive if it were real :) 

this seems to last between runs 19158001-19158020
where 19158001-3 are  at -100  MAmps
and 19158006-20 are at +100 MAmps



> On Oct 21, 2022, at 6:54 PM, Eugenia Khyzhniak via Star-fcv-l 
> <star-fcv-l AT lists.bnl.gov> wrote:
> 
> Hi All,
> 
> I'm working with a 27GeV_production_2018 dataset. I found that this dataset 
> contains Full and Reverse Full Field data. However, according to the RunLog 
> page, we should not have data for the Full Field in this dataset at all. 
> Also the RunLog page states that these files must belong to the Reverse 
> Full Field. 
> Here is few examples:
> /home/starlib/home/starreco/reco/27GeV_production_2018/FullField/P19ib/2018/15/19158007/st_physics_19158007_raw_2000001.picoDst.root
> /home/starlib/home/starreco/reco/27GeV_production_2018/FullField/P19ib/2018/158/19158007/st_physics_19158007_raw_2500001.picoDst.root
> /home/starlib/home/starreco/reco/27GeV_production_2018/FullField/P19ib/2018/158/19158007/st_physics_19158007_raw_3000001.picoDst.root
> 
> I'm confused. Does anyone know what is happening here?
> 
> Thank you,
> Yevheniia (Eugenia) Khyzhniak
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