10. Managing the beamline#

In this section, some recipes are provided for managing the beamline and meeting the needs and expectations of different experiments.

10.1. Starting and ending an experiment#

When a new experiment begins, run the command:

BMMuser.start_experiment(name='Betty Cooper', date='2019-02-29', gup=123456, saf=654321)

This will create that data folder and populate it with an experimental log (Section 9), write a template for a macro file (Section 7.6), configure the logger to write a user log file (Section 9.1) for this experiment, set the GUP and SAF numbers as metadata for output files, set up snapshot (Section 9.2) and dossier (Section 9.4) folders, and perform other experiment start-up chores.

Note

In the near future, the start_experiment() command will grab metadata from PASS (or UPS, or whatever) and set access permissions on data. When that happens, the only argument needed will be the SAF number.

The name should be the PI’s full name, preferably transliterated into normal ASCII. The date should be the starting day of the experiment in the YYYY-MM-DD format. The `GUP and SAF numbers can be found on the posted safety approval form.

Once the experiment is finished, run this command:

BMMuser.end_experiment()

This will reset the logger and the DATA variable and unset the GUP and SAF numbers.

10.2. Change energy#

Changing energy is simple. Usually, it is as simple as doing

RE(change_edge('Fe'))

replacing the two-letter element symbol with the element you actually want to measure. This command will move the monochromator, put the photon delivery system in the correct mode, move the M2 bender to approximately the correct setting, run a rocking curve scan, optimize the slit height, move the reference foil holder to the correct position (if configured), and select the correct ROI channel (if configured).

If you want to reproduce this by hand, here is the command sequence:

  1. First move the DCM to the new energy position. It is usually a good idea to move a bit above the target edge energy. Here’s an example for moving 50 eV above the iron K edge energy:

    RE(mv(dcm.energy, 7112+50))
    
  2. Put the beamline in the correct photon delivery system mode. (See the table just above.) Continuing with the example of the iron K edge, for unfocused beam:

    RE(change_mode('E'))
    

    If the new edge energy is in the same energy range according to the table above, you can skip this step. For example, Mn and Fe are both in mode E (or mode C). The change_mode() command does not need to be run to move between those edges.

  3. Measure a rocking curve scan (Sec 6.2) to verify that the second crystal of the rocking curve is parallel to the first crystal. This is more important for large energy changes. You may find that you can skip this step if you are changing between nearby edges.

    RE(rocking_curve())
    

    At the end of the scan, the mono pitch will be moved to the top of the rocking curve.

  4. If using focused beam, make sure that the mirror bender is in the correct position. For focusing at the XAS table, m2_bender should be at about 212000 counts. For focusing at the position of the goniometer, m2_bender should be about 112000 counts.

    RE(mv(m2_bender, 212000))
    
  5. Next, verify that the height of the hutch slits (Sec 6.2) is optimized for the beam height. In principle, this should be correct after changing photon delivery system mode. But it doesn’t hurt to verify.

    RE(slit_height())
    

    At the end of the scan, you will need to pluck the correct position from the plot.

  6. Next, if you are using a reference foil, you should move the reference foil holder to the slot containing the correct foil. The command is something like:

    RE(reference('Fe'))
    

    choosing the correct element for your measurement.

  7. Finally, select the correct ROI channel:

    BMMuser.verify_roi(xs, 'Fe', 'K')
    

As a reminder, here is the table of operating modes.

Table 10.1 Photon delivery modes#

Mode

focused

energy range

A

above 8 keV

B

below 6 keV

C

6 keV – 8 keV

D

above 8 keV

E

6 keV – 8 keV

F

below 6 keV

XRD

above 8 keV

10.3. Change crystals#

Suppose you wanted to change from the Pt L3 edge (11564 eV) on the Si(111) crystal to the same energy on the Si(311) crystal.

RE(change_xtal('311'))

This will move the lateral motor of the DCM and optimize the roll and pitch of the second crystal. It will then move the DCM to the energy that you started at with the other crystal set and run a rocking curve scan.

Note that some of these motions can be a bit surprising in the sense that the monochromator will end up outside the normal operating range of the beamline. They will, however, eventually return to sensible places.

10.4. Change XAS ↔ XRD#

Begin this transition by leaving the I0 chamber in place to monitor the incidence flux. In most cases, this should do the trick:

RE(change_edge('Ni', xrd=True, energy=8600))

The element symbol in the first argument is not actually used in any way when xrd=True is used, however the funtion requires something as its first argument. Setting xrd=True forces the focus=True and target=0 arguments to the change_edge() command to be set. This will move to the specified energy, place the photon delivery mode in XRD mode, optimize the second crystal and the slit height, and move to an approximately M2 bender position.

To do all of that by hand, you would do the follow commands:

RE(change_mode('XRD'))
RE(mv(dcm.energy, 8600))
RE(rocking_curve())
RE(slit_height())

This change of mode should have the beam in good focus at the position of the goniometer. 8000 eV is the nominal operating energy for the goniometer. If a higher energy is required, substitute the correct energy for 8600 in the second line.

Todo

Determine look-up table for lower energy operations using both M2 and M3. This will require a new XAFS table and adjustments to the limit switches on m3_ydo and m3_ydi.

Once the photon delivery system is set, remove the ion chambers and insert the XRD flight path into its place.

10.5. XAFS with Si(333)#

Using the Si(111) monochromator, it is possible to use the third harmonic – the Si(333) reflection – to measure XAS with slightly higher energy resolution. In this section, we explain how to set up the beamline to measure the Ge K edge at 11103 eV using the Si(333).

You cannot use the change_edge() command to do this. Use of the Si(111) (or Si(311)) is hard-wired into that plan. You have to set up the beamline by hand.

First, put the photon delivery system in mode D (or mode A if using the focusing mirror):

RE(change_mode('D'))

Next, move the monochromator to a few 10s of eV above the absorption edge, as measured with the third harmonic. The Ge K edge is at 11103 eV, so we need to move the monochromator to 11103/3 = 3701 eV.

RE(mv(dcm.energy, (11103+27)/3))

or simply

RE(mv(dcm.energy, 3701+9))

This will put the third harmonic energy 27 eV above the Ge K edge.

Now, run a rocking curve scan:

RE(rocking_curve())

This will produce a plot that looks something like this:

_images/rocking_curve_333_E%3D3716.png

Fig. 10.1 A rocking curve scan with the photon delivery system in mode D and the mono at 3716 eV.#

The broad base of this curve is the Si(111) rocking curve with photons at 3710 eV. The sharp spike in the middle is the Si(333) rocking curve with photons at 11130 eV.

Optimize the slit_height:

RE(slit_height())

You are ready to measure XAS with the Si(333) reflection!

Here’s an example scan.ini file for XANES of elemental Ge:

[scan]
experimenters = Bruce Ravel

filename      = Ge
sample        = elemental Ge, crystalline
prep          = standard sample
comment       = measured with Si(333) reflection, 25um Al foil in beam path before I0

ththth        = True
e0            = 11103
element       = Ge
edge          = K

nscans        = 1
start         = next

## mode is one of transmission, fluorescence, both, or reference
mode       = transmission

## Ge Si(333)
bounds     = -45    -18     -9      36    150
steps      =      9     0.9     0.3    0.9
times      =      0.5    0.5    0.5    0.5

Several things to note:

  1. Note that the actual value for E0 is specified, not the divided-by-3 value.

  2. Actual energy bounds and steps are specified, the xafs scan plan will convert them to appropriately sized steps for the Si(111).

  3. By setting the 333 flag to True, the correct thing will happen, including writing the correct energy axis to the output data file.

  4. The on-screen plot will show the fundamental – Si(111) – energy, however.

  5. Also, you still need to set up the photon delivery system up by hand.

10.6. Motor controller kill switches#

The MCS8 motor controllers supplied by FMBO have a kill switch for power cycling the Phytron amplifier cards. This is implemented by the vendor as connector plugged into the back of the chassis which shorts the two leads of the receptacle. To kill the amplifiers, this plug is removed and reinserted.

That’s fine, but the motor controllers are on top of the FOE – not a convenient location.

The new kill switch system uses DIODE to close the kill switch circuit. Two-conductor cable is run from each motor controller to a remote DIODE box mounted on the inboard wall of the end station.

The Bluesky interface is defined here

From the docstring of the class:

A simple interface to the DIODE kill switches for the Phytron
amplifiers on the FMBO Delta Tau motor controllers.

In the BMM DIODE box, these are implemented on channels 0 to 4 of
slot 4.

attributes
----------
dcm
  kill switch for MC02, monochromator
slits2
  kill switch for MC03, DM2 slits
m2
  kill switch for MC04, focusing mirror
m3
  kill switch for MC05, harmonic rejection mirror
dm3
  kill switch for MC06, hutch slits and diagnostics

methods
-------
kill(mc)
  disable Phytron
enable(mc)
  activate Phytron
cycle(mc)
  disable, wait 5 seconds, reactivate, then re-enable all motors

Specify the motor controller as a string, i.e. 'dcm', 'slits2', 'm2', 'm3', 'dm3'

Here is a common problem which is resolved using a kill switch.

   BMM E.111 [36] ▶ RE(mvr(m2.pitch, 0.05))
   INFO:BMM_logger:    Moving m2_pitch to 2.550

   Moving m2_pitch to 2.550
   ERROR:ophyd.objects:Motion failed: m2_yu is in an alarm state status=AlarmStatus.STATE severity=AlarmSeverity.MAJOR
   ERROR:ophyd.objects:Motion failed: m2_yu is in an alarm state status=AlarmStatus.STATE severity=AlarmSeverity.MAJOR
   ERROR:ophyd.objects:Motion failed: m2_ydi is in an alarm state status=AlarmStatus.STATE severity=AlarmSeverity.MAJOR
   ERROR:ophyd.objects:Motion failed: m2_ydi is in an alarm state status=AlarmStatus.STATE severity=AlarmSeverity.MAJOR
   Out[36]: ()

This is telling you that the amplifiers for two of the M2 jacks
went into an alarm state. In the vast majority of cases, this
simply requires killing and reactivating those amplifiers.

The solution to this one is:

   BMM E.111 [1] ▶ ks.cycle('m2')
   Cycling amplifiers on m2 motor controller
   killing amplifiers
   reactivating amplifiers
   enabling motors

10.6.1. Old kill switch system#

There is a row of switches on rack D, the rack next to the control station, that are used to disable the amplifiers for the MCS8 motor controllers. The cabling for this system still exists, but is not plugged into the controllers. Should the DIODE system somehow fail, this can be redeployed easily.

_images/Kill_switches.jpg

Fig. 10.2 The manual kill switch system#

When you suspect that a motor has an amplifier fault, toggle the appropriate switch to the off position. Wait 10 seconds (to be very safe…). Then toggle the switch back to the on position. The motor should be ready to go. These switches replace the shorted plugs that came attached to the “disable” port on the back side of the MCS8s.

MCS8

RGA label

RGD label

motors

MC02

6BM-100149-RG:A1-PT1B3-A

6BM-100149-RG:A1-PT1B3-B

DCM

MC03

6BM-100150-RG:A1-PT1B3-A

6BM-100150-RG:A1-PT1B3-B

slits2

MC04

6BM-100151-RG:A1-PT1B3-A

6BM-100151-RG:A1-PT1B3-B

M2 + DM2 FS

MC05

6BM-100152-RG:A1-PT1B3-A

6BM-100152-RG:A1-PT1B3-B

M3 + Filters

MC06

<installed, not yet labeled>

DM3 (bct,bpm,fs,foils)+ Slits3

In the situation where toggling the switch does not clear the amplifier fault, the next troubleshooting step is to power cycle the MCS8. This is done by toggling the red, illuminated switch on the front of the MCS8. Wait for the red amplifier lights to stop flickering after turning off the MCS8, then turn the MCS8 back on.

After power cycling the MCS8, it is necessary to re-home all the motors controlled by the MCS8.

10.6.2. MCS8 Connector#

The disable plug on the back of the MCS8 controllers is a Binder RS connector, part number 468-885. Here’s an example.

And here is the wiring diagram. Short the prongs on the side opposite to the alignment groove.

_images/Kill_switch_connector.png

Tutorial for how to put together the Binder connectors: PDF

10.7. Windows VM and BioLogic#

We use the BioLogic EC_lab software to run the VSP-300 potentiostat. Since there is not a dedicated Windows machine at BMM, EC-Lab is run on a virtual machine that is spun up when needed. Here are the instructions for starting and interacting with the the VM.

10.7.1. Starting the virtual machine#

  • At a command line, do rdesktop xf06bm-srv2

  • This will open a new window and display a Windows login screen. Normal credentials do not work. Log in as xf06bm using the password provided by beamline staff.

  • The Windows desktop will start with a full-screen management application that looks like the figure below. You can close or minimize that window.

  • Double-click on the EC-lab icon.

  • Start doing electrochemistry.

  • Save your data to the Echem folder on the Windows desktop. In that folder you will find a folder with the name of the PI for the experiment. In that, you will find a folder with the start dat of the experiment. Save your data in that folder.

_images/Winvm_startup.png

Fig. 10.3 VM management window. You can minimize or close this.#

10.7.2. Transferring echem data#

The VM is on the INST network, thus data must be transferred to a machine on the INST network. This means an IOC server needs to be used for data transfer. Here is how this can be done using the bravel account.

  • Open a CMD window on the VM

  • cd to the location of the current user’s Echem data

  • do something like scp * bravel@10.68.42.26:/nsls2/users/bravel/temp_folder

  • on IOC2, zip up the temp_folder and transfer the file to the xf06bm user via the /tmp/ folder.

Obviously, this needs streamlining.

10.8. Calibrate the mono#

The typical calibration procedure involves measuring the angular position of the Bragg axis for the edge energies of 10 metals: Fe, Co, Ni, Cu, Zn, Pt, Au, Pb, Nb, and Mo.

The tabulated values of edge energies from Table 1 in Kraft, et al. are used in the calibration.

  1. Be sure that all 10 of these elements are actually mounted on the reference wheel and configured in the xafs_ref.mapping dict. (They should be. It would be very unusual for any of these foils to have been removed from the reference wheel.)

  2. Run the command

    RE(calibrate(mono='111'))
    

    Use the mono='311' argument for the Si(311) monochromator. This will, in sequence, move to each edge and measure a XANES scan over a wide enough range that it should cover the edge (unless the mono is currently calibrated VERY wrongly). This will write a file called edges111.ini (or edges3111.ini). Each XANES scan uses the file /home/xf06bm/Data/Staff/mono_calibration/cal.ini as the INI file. Edge appropriate command line parameters will be added by the calibrate() plan.

  3. Examine the data in Athena. Make sure E0 is selected correctly for all 10 edges. Copy those values into the first column of edges111.ini (or edges311.ini).

    Attention

    It is no longer necessary to compute the angular positions of the monochromator. Those will be computed from the edge energy values you edited into the INI file by hand.

    Todo

    Implement on-the-fly determination of E0 to obviate the step of editing the INI file. Pb is tricky. Nb and Mo are kind of tricky.

  4. Run the command

    calibrate_mono(mono='111')
    

    (or use the '311' argument). This will show the fitting results and plot the best fit. It will also print in a text box instructions for modifying the BMM/dcm-parameters.py file to use the new calibration values.

    _images/Calibration_111.png

    Fig. 10.4 Example calibration curve#

  5. Edit BMM/dcm-parameters.py as indicated.

  6. Do

    %run -i 'home/xf06bm/.ipython/profile_collection/startup/BMM/dcm-parameters.py'
    

    then do

    dcm.set_crystal()
    

    Or simply restart bsui, which is usually the easier thing.

  7. Finally, do

    calibrate_pitch(mono='111')
    

    This performs a simple linear fit to the rocking curve peak positions for dcm_pitch found at each edge. Use the fitted slope and offset to modify approximate_pitch in BMM/functions.py.

The mono should now be correctly calibrated using the new calibration parameters.

10.9. Provision a new beamline computer#

This is a list of notes on how to finish the provisioning of a new beamline computer.

Firstly, make sure that /nsls2/data is a symlink to /nsls2/data3. If it is not, ask for help from DSSI.

10.9.1. install additional packages#

  • plasma-desktop (just … better)

  • redis (essential for operation of bsui)

  • most (used as the pager in BMM’s bsui profile)

  • ag (powerful ack-like grep alternative)

  • fswebcam (used to capture analog pinhole camera)

  • demeter and perl-Graphics-GnuplotIF (something silly, no doubt)

  • slack (communications)

  • ark (compression, useful in file manager)

To install these, do:

dzdo dnf install redis most ag fswebcam demeter perl-Graphics-GnuplotIF slack ark
dzdo dnf install --skip-broken --nobest @kde-desktop

The second command installs the KDE metapackage, skipping missing packages.

To finish installing sddm, do

dzdo systemctl stop gdm
dzdo systemctl start sddm

10.9.2. Desktop wallpaper#

This may not be provisioned correctly out of the box. Find the beamline wallpapers in /usr/share/nsls2/wallpapers/beamlines.

Right click on the desktop and select “Configure Desktop and Wallpaper”. Click on “Add Image” and navigate to the folder above.

10.9.3. Things to install from git#

  • BMM stuff: git clone git@github.com:NSLS-II-BMM/BMM-beamline-configuration.git + then, cd ~/bin and ln -s ~/git/BMM-beamline-configuration/tools/run-cadashboard

  • BMM user manual: git clone git@github.com:NSLS-II-BMM/BeamlineManual.git

  • BMM standards: git clone git@github.com:NSLS-II-BMM/bmm-standards.git

  • Switch visualization: git clone git@github.com:NSLS-II-BMM/switch-pretty-printer.git

Also do cd ~/bin and ln -s ~/.ipython/profile_collection/startup/consumer/run-consumer

10.9.4. Data collection folders#

Make the local data collection folders. The BMMuser.start_experiment() command (Section 10.1) will make symlinks under those folders to the correct place on central storage.

mkdir ~/Data
mkdir ~/Data/Visitors
mkdir ~/Data/Staff

Next need to recreate historical symlinks using the correct tool.

Todo

capture the make_links.py script and the ls-lR files. Also need to automate generating the ls-lR files.