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1 -== Some general stuff: ==
1 +* [[LINK to detailled infos from MSK~[~[image:url:http://hasfweb.desy.de/pub/TWiki/TWikiDocGraphics/external-link.gif~|~|width="13" height="12"~]~]>>url:http://mskwiki/index.php?title=BAM-DAQ_Channels||shape="rect"]]
2 2  
3 -* (% style="color: rgb(0,0,0);" %)There are several BAMs in FLASH. Essentially one in the accelerator section  (FL0.DBC2, Previously: 4DBC3) and one close to the respective undulator section (FL1.SFELC and FL2.SEED5).
4 -* (% style="color: rgb(0,0,0);" %)The BAM measures the arrival time for each single electron bun in the bunch train (for working principle see [[MSK SDiag Projects>>url:https://confluence.desy.de/display/SDiagPublic/MSK+SDiag+Projects||style="color: rgb(0,0,0);" shape="rect"]] or literature listed below) 
5 -* The data format of the BAM has been completely altered in the 2022 shutdown
6 -* (% style="color: rgb(0,51,102);" %)before 2022 BAMs were always saving the arrival time information for each 1µs bucked regardless if there were electrons in the accelerator or not. In addition the arrival times for  FL1 and FL2 were saved in the same parameter ...
7 -* (% style="color: rgb(0,51,102);" %)THIS is now different. There are new parameters saving only the arrival times for pulses that go to FL1 and to FL2 (in detail: first time slot of the accelerator and second)
8 -* (% style="color: rgb(0,51,102);" %)(typically) Bigger numbers indicate later arrival time of the electrons
9 -* (% style="color: rgb(0,51,102);" %)The arrival time should be within -20 ps and +20 ps - otherwise there might be a problem ...
10 -* (((
11 -(% style="color: rgb(0,51,102);" %)The actual time t0 = 0ps is an arbitrary offset which is only changed after setting up the system after, e.g., a maintenance time, and has no relevance.
12 -)))
13 -* (((
14 -(% style="color: rgb(0,51,102);" %)What one usually does, after defining/finding time zero in the experiment, is either observe the relative changes for a single bunch during the course of the measurement run compared to the starting point, or (in addition) observe the relative deviation across all bunches within the same bunch train.
15 -)))
16 -* (((
17 -(% style="color: rgb(0,51,102);" %)Those deviations and drifts happen usually only in the order of 50fs to 200fs; depending on the machine setup.
18 -)))
19 -* (((
20 -(% style="color: rgb(0,51,102);" %)The short-term timing jitter (over several 100 trains) for each individual bunch, i.e. the standard deviation from their mean value, is usually ~~ 20fs.
21 -)))
22 -* (((
23 -(% style="color: rgb(0,51,102);" %)The actual measurement resolution of a BAM can be - currently - as good as 3fs, for each bunch in the full train.
24 -)))
3 +\\
25 25  
26 -== Data structure ==
5 +* the relevant data is the Arrivaltime FLASH.SDIAG/BAM/4DBC3/LOW_CHARGE_ARRIVAL_TIME
27 27  
28 -* (% style="color: rgb(0,0,0);" %)The details about the functionality and the data structure can be found on the page: (%%)**[[ BAM Data Structure>>url:https://confluence.desy.de/display/SDiagPublic/BAM+Data+Structure||shape="rect"]]**
29 -* also see  [[doc:FLASHUSER.Data Acquisition and controls.Data Access at FLASH (DAQ, gpfs,\.\.\.).Offline data analysis (DAQ).The FLASH HDF5 structure.WebHome]]
7 +\\
30 30  
31 -{{info title="Correction of pump-probe delay"}}
32 -* (% style="color: rgb(255,0,0);" %)Here will be soon a link to a python notebook showing an example how to use the BAM data
33 -{{/info}}
9 +* There are now (since March 2017) LOW and HIGH charge channels. for now the LOW_CHARGE Channel is the relavant one.
34 34  
35 35  \\
36 36  
37 -= Publications related to BAM =
13 +* bigger numbers indicate later arrivaltime of the electrons
38 38  
39 -=== BAM principle ===
15 +\\
40 40  
41 -1. (% style="color: rgb(23,43,77);" %)A. Angelovski, et al.(%%)
42 -(% style="text-align: left;" %)//Evaluation of the cone-shaped pickup performance for low charge sub-10 fs arrival-time measurements at free electron laser facilities
43 -//(% style="color: rgb(23,43,77);" %)Phys. Rev. ST Accel. Beams (% style="text-align: left;" %)**18**(% style="color: rgb(23,43,77);" %), 012801 (2015)(%%)
44 -[[https:~~/~~/doi.org/10.1103/PhysRevSTAB.18.012801>>url:https://doi.org/10.1103/PhysRevSTAB.18.012801||style="text-align: left;" rel="nofollow" shape="rect"]]
17 +* the arrivaltime sould be within -20 ps and +20 ps . otherwise there might be a problem ...
45 45  
46 46  \\
47 47  
48 -=== Two publications showing how to use the BAM data to improve the time resolution: ===
21 +* There is a BAM status parameter: FLASH.SDIAG/BAM/4DBC3/BAM_STATUS.1 (the 1 indicates FLASH1)
22 +** bit 0 (value: 1) = data is valid,
23 +** bit 1 (value: 2) = at least 1 bunch is present,
24 +** bit 2 (value: 4) = calibration is on,
25 +** bit 3 (value: 8) = internal feedback is on,
26 +** bit 4 (value: 16) = tuning mode is on
49 49  
50 -1. Evgeny Savelyev, et al, 
51 -//Jitter-Correction for IR/UV-XUV Pump-Probe Experiments at the FLASH Free-Electron Laser//,
52 -New J. Phys. **19**, 043009 (2017), [[https:~~/~~/doi.org/10.1088/1367-2630/aa652d>>url:https://doi.org/10.1088/1367-2630/aa652d||shape="rect"]]
53 -1. (((
54 -Dennis Mayer, Fabiano Lever and Markus Gühr,
55 -//Data analysis procedures for time-resolved x-ray photoelectron spectroscopy at a SASE free-electron-laser//,
56 -J. Phys. B: At. Mol. Opt. Phys. **55**, 054002 (2022); [[https:~~/~~/doi.org/10.1088/1361-6455/ac3c91>>url:https://doi.org/10.1088/1361-6455/ac3c91||style="text-decoration: none;" shape="rect"]]
57 -)))
28 +\\
58 58  
59 -=== Publications showing the correlation between the values measured by the BAM and the XUV pulse arrival time ===
30 +* if DBC3 is not working then also 3DBC2 can be used. there is a linear correlation between BC2 and BC3
60 60  
61 -1. (% style="color: rgb(0,0,0);" %)//** Description of the FLASH synchronization system**//
62 -S. Schulz, et al.(%%)
63 -(% style="text-align: left;" %)//Femtosecond all-optical synchronization of an X-ray free-electron laser//(% style="color: rgb(0,0,0);" %),(%%)
64 -(% style="color: rgb(0,0,0);" %)Nature Communications (% style="text-align: left;" %)**6**(% style="color: rgb(0,0,0);" %), 5938 (2015); (%%)[[http:~~/~~/dx.doi.org/10.1038/ncomms6938>>url:http://dx.doi.org/10.1038/ncomms6938||style="text-decoration: none;text-align: left;" shape="rect"]]
32 +(from Marie: der groesste Drift-Beitrag kommt immer aus dem Injektor (also alles zw. Injektorlaser und ACC39) Einfluss von ACC23 ist deutlich kleiner. Im Mittel hat man einen linearen Zusammenhang zw. Ankunftszeit BC2 zu BC3.)
33 +
65 65  \\
66 -1. //**Showing a correlation of 11 fs rms between BAM and XUV arrival time
67 -**//R. Ivanov, et al to be published 2022  //**
68 -\\**//
69 -1. (((
70 -//**Showing a correlation of 20 fs rms between BAM and XUV arrival time**//
71 -R. Ivanov, J. Liu, G. Brenner, M. Brachmanski and S. Düsterer,
72 -//FLASH free-electron laser single-shot temporal diagnostic: terahertz-field-driven streaking//,
73 -Special Issue (PhotonDiag2017),
74 -J. Synchrotron Rad.** 25**, 26-31 (2018);[[ https:~~/~~/doi.org/10.1107/S160057751701253X>>url:https://doi.org/10.1107/S160057751701253X||style="text-decoration: none;" shape="rect"]]//**
75 -**//
76 -)))
77 -1. (((
78 -//**Study of arrival time fluctuations**//
79 -Ivette J. Bermúdez Macias, Stefan Düsterer, Rosen Ivanov, Jia Liu, Günter Brenner, Juliane Rönsch-Schulenburg, Marie K. Czwalinna, and Mikhail V. Yurkov,
80 -//Study of temporal, spectral, arrival time and energy fluctuations of SASE FEL pulses//,
81 -Optics Express 29, 10491-10508 (2021); [[https:~~/~~/doi.org/10.1364/OE.419977>>url:https://doi.org/10.1364/OE.419977||style="text-decoration: none;" shape="rect"]]
82 -)))
83 83  
84 84  \\
85 85  
38 +=== more Info: ===
39 +
86 86  \\
41 +
42 +* [[talk by Marie (2011)>>attach:FLASH-seminar-2011_BAM_study_results.pdf]]
43 +* contact: Marie Kristin Czwalinna
44 +
45 +\\
46 +
47 +== Streak camera info ==
48 +
49 +\\
50 +
51 +* the streak camera measures the delay between optical (amplified) laser and FEL (dipole radiation). - not in respect to the master clock !
52 +* streak camera ONLY delivers data which is averaged over seveal 10 seconds. there is NO shot to shot info.
53 +* a larger value of the streak camera delay indicates that the optical laser comes later than the FEL (or FEL earlier than the laser ...)
BAM-basics and outlook-2018_DESY-template_16-9Format.pdf
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