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Detector Characterisation (Spectral lines)
fiori - 11:01 Wednesday 02 August 2017 (38996) Print this report
moving peaks

It is always rewarding to browse through the Hrec spectrogram plot using Didier's "magic command" (here the command used for the plots attached below):

$ROOTROOT/$UNAME/bin/root.exe -l /opt/w3/vim/spectro/spectro_auto.C\(\"Hrec_hoft_20000Hz\",1185277224,400000,0.1,0,500,0,0,0\)

(note, you also need to create in your home dir one file named ".rootrc" containing the following text.

Unix.*.Root.DynamicPath:    .:$(ROOTSYS)/$(UNAME):$(ROOTSYS)/lib:$(FRROOT)/$(UNAME)
Unix.*.Root.MacroPath:      .:$(ROOTSYS)/macros:$(FRROOT)/root
Rint.Logon:              $(FRVROOT)/root/FrvLogon.C
Rint.History:            $(HOME)/.root_hist

)

There are peaks that move in frequency (some more, some less). It is interesting to investigate them more deeply, for example by looking for correlations with temperature sensors, alignment signals, beams power (to start with...). Here a tentative list of commonly moving peaks:

  • 442 Hz, 409 Hz, 373 Hz (Figures 1,2,3) move significantly in frequency (already noticed in 38677)
  • family of lines around 270 Hz (figures 4 and 5)
  • 193 Hz, 156 Hz move slightly in frequency (note: these peaks are "certified" to belong to SDB1, since they clearly rised when the bench was shaked with white noise) also 126 Hz moves coherently (Figures 6, 7,8)... do they correlate with temperature changes inside SDB1?
  • 367 Hz (a group of three lines) in Figure 9
  • 255 Hz, in Figure 10
  • wandering lines: around 450Hz and around 90Hz: Figures 11 and 12

Good also to check if these peaks are tracked by Noemi....

Images attached to this report
Comments to this report:
bejger - 20:12 Thursday 03 August 2017 (39026) Print this report
Followup of wandering lines near 90Hz and 450Hz. I was too optimistic on the daily DetChar meeting: both sets of lines didn't disappear, but moved to lower frequencies. Their frequency evolution is similar (Fig1 for 65-100Hz range, Fig2 for 330-500Hz range). The structure from 30 July was also visible at higher frequencies (Fig3, above 500Hz), and much weaker near 230Hz and 920Hz.

These lines are very well visible in LSC_PRCL (Figs 4, 5).

Unfortunately, didn't yet find anything interesting in ENV channels.
Images attached to this comment
bejger - 15:01 Friday 04 August 2017 (39037) Print this report
Followup on group of lines now at below 80Hz (previously near 95Hz). Noemi doesn't track these lines.
Spectrograms of several channels at B2 and PR:

ASC_B2_QD2_V_8MHz_I LSC_B2_8MHz_I SIB2_B2_PD2_8MHz_I
ASC_PR_TX_IN

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