Status and future of beamline control software at ESRF. Beamline Control Unit
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2 Status and future of beamline control software at ESRF E.Papillon, Beamline Control Unit
3 ISDD Instrument Services and Development Divisions SOFTWARE GROUP A.Goetz Data Analysis Unit C.Ferrero Accelerator Control U. JM.Chaize Beamline Control Unit L.Claustre Beamline Control Unit (former BLISS) Support and Development of beamline control software 29 ESRF and 12 CRG beamlines, 6 Laboratories 16 people E.Papillon, 2010, NSLSII 3
4 Outline Beamline control today: Software architecture Continuous scans Fast 2D detectors Graphical Interfaces Evolution Conclusion E.Papillon, 2010, NSLSII 4
5 Software overview USERS Beamline GUI/O Online display SPEC TACO / TANGO Linux / Windows drivers HARDWARE E.Papillon, 2010, NSLSII 5
6 Hardware overview : Network Linux workstation Industrial PC / Linux VME + Bus Coupler ICEPAP motor controller Detectors E.Papillon, 2010, NSLSII 6
7 TACO / TANGO Control of distributed hardware TACO TANGO Developed at ESRF Obj. C / RPC Client and server API in C/python/matlab/labview/ Only commands Widely used on beamlines: ~100 different servers devices exported Collaboration ESRF, Elettra, Soleil, ALBA, DESY C++ / CORBA Client and server API in C/C++/python/java Commands, attributes, properties Multi-thread Events support All new servers in tango E.Papillon, 2010, NSLSII 7
8 What is SPEC for the beamline? Command Line Interface Main sequencer Handle diffractometers geometries Device controller: Integrated in SPEC Taco interface: Motors / Counters MCA / CCD Generic Interface to: Serial Line GPIB Socket Taco / Tango E.Papillon, 2010, NSLSII 8
9 Macro motors: SPEC macros Physical : ICEPAP (socket), piezo (GPIB), Calculational : slit offset/gap, 3 legs table, Macro counters: Physical : eurotherm, lakeshore, Calculational : ratio, attenuators transmission, Other Macros: Other type of devices : beam shutters, filter box, New sequences : exafs scans, gap scans, Very flexible : many devices/sequences written limited data types, no debugger, no multi-threads E.Papillon, 2010, NSLSII 9
10 Continuous scans From Sequential MOVE EXPOSURE READOUT Time To Paralell Practical Issues Distributed System Multiple detectors Short exposure time MOVE EXPOSURE READOUT Synchronization Data Buffering Time E.Papillon, 2010, NSLSII 10
11 Continuous scans : synchronization By software : Synchro. with time: no wiring, i good on single host By hardware : Needs wiring, good for distributed hosts Synchro. with time : P201, OPIOM boards Need more : motor position, mixed time/position, MUSST board Very flexible event generator 6 x input signals : Digital it counter Analog Positioning (motor steps and encoders) 16 x digital I/O Host Interface : GPIB E.Papillon, 2010, NSLSII 11
12 Continuous scans : data buffering Software implementation : HOOK Kernel driver + TACO device server Hardware readout + buffering For In-house developed hardware PCI and VME boards Software event generator Hardware implementation : MUSST Encoders, motor steps Counters, ADC Canberra MCA (ICB) Data handling: SPEC polls data buffers Counters / motors saved by SPEC E.Papillon, 2010, NSLSII 12
13 Continuous scans : detectors t Canberra MCA (ICB) Data buffering on MUSST XIA XMAP PXI board 4 channels PXI/PCI bus coupler External sync. Signal 4MB memory / board Data buffering in TACO 10 ms / spectra 1 ms / spectra (one board) Spectras saved by device servers Integrated ROIs transferred to SPEC (online plotting) Configuration issues No generic counter interface E.Papillon, 2010, NSLSII 13
14 2D detectors t TACO CCD interface in SPEC Many CCDs supported: Princeton, Sensicam, PCO, Andor, Photonic Science, Standard macro set Beam parameters, Multi-frame buffer, Parallel saving, Per device development LIMA: Library for Image Acquisition Reuse of common code generic procedures + interfaces Support recent fast detectors E.Papillon, 2010, NSLSII 14
15 2D detectors: t LIMA Hardware layer Control layer Software features fallback if hardware has limited capabilities: RoI, Binning, Frame Accumulation Basic processing and data reduction: Beam parameters, RoI statistics, parallel saving, dark substraction Specific data reduction algorithms through plug-ins (C++) Low level: C++ (multi-threaded) High level: C++ / Python (SIP) Generic TANGO interface + detector configuration Currently integrated: Pilatus, Frelon, Maxipix E.Papillon, 2010, NSLSII 15
16 2D detectors t : ESPIA card Designed to interface the FReLoN 2k Collaboration ESRF + SECAD, S.A. 2 Gbps fiber optic link (> 100 m) PCI 64 bits / 66 MHz ~180 MB/s maximum data rate FOCLA : 2xCameraLink connectors FReLoN HD (PSB-2) 2048 x 32 fps ~125 MB/s E.Papillon, 2010, NSLSII 16
17 2D detectors t : Medipix2 i / Maxipix i Pixel detector photon counting 256 x bit 0.3 ms readout time Max: 1400 fps 180 MB/s Maxipix: i Medipix2 i array 5x1,2x2 2 Image reconstruction in LIMA 1000 fps 650 MB/s ESPIA next generation: PCI-Express 8x lanes 4 fiber optic 250 MB/s 1 GB/s Espia E.Papillon, 2010, NSLSII 17
18 Online Display Standalone tool for visualisation (python/qt) Work online : use SPEC shared memory Work offline : specfiles, edf files, hdf files PyMCA Oxidis E.Papillon, 2010, NSLSII 18
19 Beamline GUI : BlissFramework Written in python/qt MVC architecture GUI application is made of cemented bricks Communication to SPEC: server mode Socket interface SpecClient python module First GUI: MxCube (MaxLab, Soleil, Bessy) Hardware Repository server Spec Spec Client Taco Tango DS Taco/ Tango Poller Hardware Object Hardware Objects pool GUI brick GUI application E.Papillon, 2010, NSLSII 19
20 Beamline GUI : example E.Papillon, 2010, NSLSII 20
21 Beamline GUI : example E.Papillon, 2010, NSLSII 21
22 Evolution : on-going Common 2D detectors framework : LIMA More detectors to come New interface in spec More beamline GUI: BlissFramework4 ready First application : BioSaxsCube TANGO to replace TACO whenever possible Hardware upgrade : replace VME E.Papillon, 2010, NSLSII 22
23 Evolution Integrated beamline configuration tool Continuous scans Easier integration on beamline Easier integration ti of detectors t New data format: Specfiles + EDF Files HDF5 Experiment database : ISpyB?? keep SPEC?? E.Papillon, 2010, NSLSII 23
24 Evolution : alternatives ti to SPEC Evaluation of 3 control systems: GDA (diamond) Most advanced solution SARDANA (alba) Based on already used tools (python, qt, tango) No beamline yet In-house solution E.Papillon, 2010, NSLSII 24
25 Conclusion Keep improving existing system Maintain i support of running beamlines Prepare new upgrade beamlines (start in 2011) Investigate new solutions E.Papillon, 2010, NSLSII 25
26 Thank you! E.Papillon, 2010, NSLSII 26
27 E.Papillon, 2010, NSLSII 27
28 Continuous scans configuration start event DISPLAY storage HW trigger data buffering data polling datafiles SPEC HOOK PCI / VME boards XMAP TACO XMAP PXI crate Motor Encoder E.Papillon, 2010, NSLSII 28
29 FOCLA module 2D detectors t : Camera Link Connects to ESPIA 2 X Camera Link connectors Multiple pixel packing formats Test image ~180 MB/s Dalsa Pantera 1M60 Frame transfer technology 1024 x 60 fps 120 MB/s Sarnoff CAM512 2 x 8 ADCs 12 bit 512 x 300 fps 150 MB/s 512 x 500 fps 125 MB/s E.Papillon, 2010, NSLSII 29
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