SlideShare a Scribd company logo
1 of 74
Download to read offline
Monitoring and Data Acquisition of the Laser
Calibration System of Muon g-2 Experiment
Atanu Nath
(On behalf of the Muon g-2 collaboration)
104° Congresso Nazionale
21st
September 2018, Cosenza, Calabria
21 September 2018 Atanu Nath 2
Outline
The main components
– Laser control system
– Source Monitors
– Local Monitors
Data acquisition & monitoring systems
– MIDAS DAQ
– Naples DAQ
21 September 2018 Atanu Nath 3
21 September 2018 Atanu Nath 4
21 September 2018 Atanu Nath 5
Laser Controller
21 September 2018 Atanu Nath 6
Laser Control System
In-Fill : 2 pulses 200 us apart are sent every fill to minimize
the damage
Then these pulses are shifted by 5 us to scan the whole
range of 400 us fill window.
In standard DAQ in-fill pulses are sent every 10 fills.
Out of fill : laser pulses sent outside the muon fill over longer
period of time to study the long-term gain stability.
affects due Temperature variation, aging etc can be
corrected.
double-pulses : additional (1 %) gain drop due to very
close (~ 10 ns) positron hits, to study this two very close
laser pulses are sent and the response is studied.
flight-simulator : positron events are simulated using
laser pulses that can also mimic the infamoussplash.
Laser Pulse Tagging :
1.8 GeV pulse that is found almost (in more than 50
crystals) in all crystals is definitely a laser.
burst Test pulse
500 ns
40 us
21 September 2018 Atanu Nath 7
Laser Control System
In-Fill : 2 pulses 200 us apart are sent every fill to minimize the
damage
Then these pulses are shifted by 5 us, it takes 40 such
steps (40 fills and not necessarily consecutive fills) to scan
the whole range of 400 us fill window.
In standard DAQ in-fill pulses are sent every 10 fills.
●
Out of fill : laser pulses sent outside the muon fill over longer
period of time to study the long-term gain stability.
– affects due Temperature variation, aging etc can be
corrected.
– double-pulses : additional (1 %) gain drop due to very
close (~ 10 ns) positron hits, to study this two very close
laser pulses are sent and the response is studied.
– flight-simulator : positron events are simulated using
laser pulses that can also mimic the infamoussplash.
Laser Pulse Tagging :
1.8 GeV pulse that is found almost (in more than 50
crystals) in all crystals is definitely a laser.
burst Test pulse
500 ns
40 us
21 September 2018 Atanu Nath 8
Laser Control System
In-Fill : 2 pulses 200 us apart are sent every fill to minimize the
damage
Then these pulses are shifted by 5 us, it takes 40 such
steps (40 fills and not necessarily consecutive fills) to scan
the whole range of 400 us fill window.
In standard DAQ in-fill pulses are sent every 10 fills.
f fill : laser pulses sent outside the muon fill over longer period
of time to study the long-term gain stability.
affects due Temperature variation, aging etc can be
corrected.
double-pulses : additional (1 %) gain drop due to very
close (~ 10 ns) positron hits, to study this two very close
laser pulses are sent and the response is studied.
flight-simulator : positron events are simulated using
laser pulses that can also mimic the infamoussplash.
●
Laser Pulse Tagging :
– 1.8 GeV pulse that is found almost (in more than 50
crystals) in all crystals is definitely a laser.
burst Test pulse
500 ns
40 us
21 September 2018 Atanu Nath 9
The Monitors...
21 September 2018 Atanu Nath 10
Source Monitors × 66
PiDPiD
PiDPiD
PMTPMT
21 September 2018 Atanu Nath 11
Source Monitors × 66
PMT PiD-1 PiD-2
21 September 2018 Atanu Nath 12
Source Monitors × 66
PiDPiD
PiDPiD
PMTPMT
● 2 Pin Diodes : receive laser pulses directly from the source.
Pin-1/Pin-2 ~
stability at sub per
mil
1 PMT : receives laser light from
laser source plus light generated
by (NaI) an americium source.
Laser/Americium
~ the laser-source
variation. which will
be useful for the
long term calibration.
60 HOURS
21 September 2018 Atanu Nath 13
Source Monitors × 66
PiDPiD
PiDPiD
PMTPMT
Pin Diodes : receive laser pulses directly from the source.
Pin-1/Pin-2 ~
stability at sub per
mil
● 1 PMT : receives laser light from laser source plus light generated by (NaI) an
americium source.
– Laser/Americium ~ the laser-source variation. which will be useful
for the long term calibration.
60 HOURS
21 September 2018 Atanu Nath 14
Local monitors × 2424
21 September 2018 Atanu Nath 15
Local monitors × 2424
●
1 PMT (Plan of 2 actually) : receives laser pulses directly from
the Source Monitors (Pulse-1) as well as light coming back from
the calorimeters (Pulse-2).
– Pulse-1/Pulse-2 ~ stability of the Local Monitors.
1 PMT : receives laser light
from laser plus americium
source.
Laser/Americiu
m ~ the
laser-source
variation. which
will be useful
for the long
term calibration.
,
Hours (July 1st
– 4th
, 2017)
Pulse-1/Pulse-2
Run 1791 - 1796
AnnaDriutti
21 September 2018 Atanu Nath 16
Data Acquisition Systems
21 September 2018 Atanu Nath 17
MIDAS DAQ & Monitoring System
21 September 2018 Atanu Nath 18
MIDAS DAQ
uTCA based
WFDs
GPUs
(Graphics
Processing)
20
GB/s
ODB
(PostgreSQL)200
MB/s
Fermilab
Storage200
MB/s
Online
Data Quality
Monitoring
Maximum Integrated Data Acquisition System
21 September 2018 Atanu Nath 19
MIDAS DAQ
●
Runs can be started and
managed from the web-interface.
●
Alarm goes off when something
goes wrong.
●
Configurations can be changed in
the Online DataBase.
21 September 2018 Atanu Nath 20
Online Database
●
Various configurations like
laser mode
filter-wheel position
etc can be set in the
Online DataBase page.
21 September 2018 Atanu Nath 21
Online Data Quality Monitor
*.mid bnary file ROOT files
Art-based
Analysis
Online Plots
21 September 2018 Atanu Nath 22
Online Data Quality Monitor
●
Server connection
status.
●
Traces of laser
signals.
●
Stability of laser
pulses over
various runs.
●
Alarms go off
when things go
wrong.
21 September 2018 Atanu Nath 23
Slow-control DQM
1 WEEK
1 DAY
TEMP.
BIAS & HVs
FILTERS
& MIRRORS
NETWORKS
21 September 2018 Atanu Nath 24
Naples DAQ & Monitoring System
21 September 2018 Atanu Nath 25
Naples DAQ
6 x
Custom made
Digitizer Board
Custom Made
Event-builder
Controller Board
Naples
Database
Naples
Storage
Online
Monitoring
Custom made (bash, c++, ROOT) Naples DAQ and Monitoring PackageRelayed
ToWFDs
21 September 2018 Atanu Nath 26
PMT
Pin-1
Pin-2
S
M
B
#
1
PMT
Pin-1
Pin-2
S
M
B
#
2
PMT
Pin-1
Pin-2
S
M
B
#
3
PMT
Pin-1
Pin-2
S
M
B
#
4
PMT
Pin-1
Pin-2
S
M
B
#
5
PMT
Pin-1
Pin-2
S
M
B
#
6
CONTROLLER BOARD
SERVER
DATA STORAGE
&
MONITORING SERVER
I
N
T
E
R
N
E
T
21 September 2018 Atanu Nath 27
Naples DAQ
Custom made Source Monitor crate of Naples.
Laser Control
21 September 2018 Atanu Nath 28
Naples DAQ
Custom made Source Monitor crate of Naples.
Laser Control
21 September 2018 Atanu Nath 29
Naples DAQ
Custom made Source Monitor crate of Naples.
SM Digitizer – 1 to 6
Pre-amplifier
Shaper
Digitizer.
Provides bias/HV to the
detectors.
21 September 2018 Atanu Nath 30
Naples DAQ
Custom made Source Monitor crate of Naples.
SM Digitizer – 1 to 6
PiD/PMT
Signal
Shaper
Long-tail (20 us)
Semi Gaussian)
Baseline restorer
Digitizer
21 September 2018 Atanu Nath 31
Naples DAQ
Custom made Source Monitor crate of Naples.
SM Event Builder
(Controller Board)
Receives data frame from all
the 66 SM boards and checks
for errors and then builds the
final data frame containing
information of 6x3 = 1818
channels.
Sends the data frame to
Naples Database over
ethernet.
21 September 2018 Atanu Nath 32
Naples DAQ
Custom made Source Monitor crate of Naples.
SM Event Builder
(Controller Board)
Receives data frame from all
the 66 SM boards and checks
for errors and then builds the
final data frame containing
information of 6x3 = 1818
channels.
Sends the data frame to the
data farm over ethernet.
21 September 2018 Atanu Nath 33
Naples DAQ
Custom made Source Monitor crate of Naples.
3 x 6 = 18 Board Temp. sensors
3 x 6 = 18 Pre Amp. Temp. sensors
2 x 6 = 12 Laser-hut Temp. sensors
0.1 o
C
Sensitivity
21 September 2018 Atanu Nath 34
Naples Monitoring...
21 September 2018 Atanu Nath 35
DATA FRAMEDATA FRAME
In the Controller BoardIn the Controller Board
21 September 2018 Atanu Nath 36
CONTROLLER BOARD
MONITORING SERVER
Asks the controller board to send the latest data frame.
Analyzes the latest frame on arrival and stores the results in a
buffer…
Displays the results of last minute.
Displays the results of last several hours.
21 September 2018 Atanu Nath 37
Online Summary Table
21 September 2018 Atanu Nath 38
Short Term Trends
21 September 2018 Atanu Nath 39
Long Term Trends
21 September 2018 Atanu Nath 40
STABILITY OF THE MONITORS
21 September 2018 Atanu Nath 41
CALCULATION OF STABILITY
~ 1 MINUTE
21 September 2018 Atanu Nath 42
CALCULATION OF STABILITY
~ 1 MINUTE
21 September 2018 Atanu Nath 43
CALCULATION OF STABILITY
~ 1 MINUTE
Pinratiofluctuation
21 September 2018 Atanu Nath 44
FLUCTUATION OVER LONGER TIME
21 September 2018 Atanu Nath 45
Stability Plots
21 September 2018 Atanu Nath 46
Electronic Calibration DAQ
21 September 2018 Atanu Nath 47
Calibration of The Electronics
PMT Pre-amp.
S
M
B
PiD-1 Pre-amp.
PiD-1 Pre-amp.
A chain of known charge pulses
Called “DAC”s
21 September 2018 Atanu Nath 48
Linearity Test
S
M
B
A chain of known charge pulses
Called “DAC”s
21 September 2018 Atanu Nath 49
Temperature Correction
PMT PIN-1 PIN-2
CALIBRATION RAMPING
21 September 2018 Atanu Nath 50
Temperature Correction
PMT 0.1 % / o
C
Pin 1, 2 ~ 0.4 % / o
C
21 September 2018 Atanu Nath 51
Temperature Correction
UNCORRECTED
CORRECTED
10 DAYS
OctavioEscalante
21 September 2018 Atanu Nath 52
Current Status and Plans
●
Laser DAQs (MIDAS & Naples) are running 24x7 flawlessly since the beginning (2017).
●
Monitoring of short-term
– event by event
– last minute
and
●
long-term
– last 24 hours of laser trend
– last few weeks of temperature trends
are running smoothly.
21 September 2018 Atanu Nath 53
GRAZIE
21 September 2018 Atanu Nath 54
21 September 2018 Atanu Nath 55
Numbers:
●
SM input 150 pJ/pulse
●
LM input 0.01 pJ/pulse
●
Americium ~ 10 Hz
●
Laser source: pico quant, 750 pJ @ 450 nm, average power
28 mW
●
21 September 2018 Atanu Nath 56
Why Laser Calibration?
21 September 2018 Atanu Nath 57
Why laser calibration?
Time [ns]
Two nano-secs apart particles hitting the
calorimeter ~ typical SiPM charging up time.
-4%
-8%
VERY SHORT
IN-FILL
DocDb10818-v3
21 September 2018 Atanu Nath 58
Why laser calibration?
Time [us]
IN-FILL
High load in the first few micro-secs after
the injection results in a SiPM gain recovery
time ~ few tens of micro-secs
QUITE LONG
DocDb10818-v3
21 September 2018 Atanu Nath 59
Why laser calibration?
Time [hours]
Variation[%]
Temperature[0
C]
LONG TERM
Much slower gain changes over longer time
(hours/days) Can occur due to temperature
change, aging etc.
VERY LONG
DocDb10818-v3
21 September 2018 Atanu Nath 60
Why laser calibration?
Gain Sagging
Short-term
Expected < 1% but we have seen ~ 10%
Megaboxes improves the situation, reduces the time
constant, but the drop is there.
Long-term
Huge temperature variation, different beam conditions, aging
etc can affect the gain significantly over longer time scale.
.
Calorimeter Number Calorimeter Number
Run 11224
~ 1 WEEK~ 1 WEEK
Gainvariationbetween35-40us
Gainvariationbetween35-40us
Run 09183
In-fill gain function can be different in different
runs separated by weeks due to different beam
conditions.
ANOTHER LONG ONE..
SAME CALO CAN SAG DIFFERENTLY @ DIFFERENT TIMES
DocDb10818-v3
DocDb10818-v3
21 September 2018 Atanu Nath 61
The laser calibration system
● Using laser pulses of known amplitude we can extract those “3 kinds” of gain functions and correct the real data.
But those pulses have to be known, stuff like temperature and aging can also affect the laser sources, that’s why we
need a monitoring system for the laser sources right after the light leaves the source :
the Source Monitors
They must also remain known till the end right before hitting the calorimeters after traveling through a long distribution
system, therefore a monitoring system that monitors the local (light coming back from the calorimeters) situation is
needed :
the Local Monitors
But wouldn’t these laser pulses mess with the positron signals? They would! That’s why we need to control the laser
pulses in a specific manner so that a few pulses during the muon fills and a few outside of that suffice to get us the gain
function :
the Laser Control
21 September 2018 Atanu Nath 62
21 September 2018 Atanu Nath 63
● Using laser pulses of known amplitude we can extract those “3 kinds” of gain functions and correct the real data.
But those pulses have to be known, stuff like temperature and aging can also affect the laser sources, that’s why we
need a monitoring system for the laser sources right after the light leaves the source :
●
the Source Monitors
They must also remain known till the end right before hitting the calorimeters after traveling through a long distribution
system, therefore a monitoring system that monitors the local (light coming back from the calorimeters) situation is
needed :
the Local Monitors
But wouldn’t these laser pulses mess with the positron signals? They would! That’s why we need to control the laser
pulses in a specific manner so that a few pulses during the muon fills and a few outside of that suffice to get us the gain
function :
the Laser Control
The laser calibration system
21 September 2018 Atanu Nath 64
21 September 2018 Atanu Nath 65
The laser calibration system
● Using laser pulses of known amplitude we can extract those “3 kinds” of gain functions and correct the real data.
But those pulses have to be known, stuff like temperature and aging can also affect the laser sources, that’s why we
need a monitoring system for the laser sources right after the light leaves the source :
●
the Source Monitors
They must also remain known till the end right before hitting the calorimeters after traveling through a long distribution
system, therefore a monitoring system that monitors the local (light coming back from the calorimeters) situation is
needed :
●
the Local Monitors
But wouldn’t these laser pulses mess with the positron signals? They would! That’s why we need to control the laser
pulses in a specific manner so that a few pulses during the muon fills and a few outside of that suffice to get us the gain
function :
the Laser Control
21 September 2018 Atanu Nath 66
21 September 2018 Atanu Nath 67
The laser calibration system
● Using laser pulses of known amplitude we can extract those “3 kinds” of gain functions and correct the real data.
But those pulses have to be known, stuff like temperature and aging can also affect the laser sources, that’s why we
need a monitoring system for the laser sources right after the light leaves the source :
●
the Source Monitors
They must also remain known till the end right before hitting the calorimeters after traveling through a long distribution
system, therefore a monitoring system that monitors the local (light coming back from the calorimeters) situation is
needed :
●
the Local Monitors
– But wouldn’t these laser pulses mess with the positron signal? They would! That’s why we need to control the laser
pulses in a specific manner so that a few pulses during the muon fills and a few outside of that suffice to get us the gain
function :
●
the Laser Control
21 September 2018 Atanu Nath 68
21 September 2018 Atanu Nath 69
Laser Control System
●
In-Fill : 2 pulses 200 us apart are sent in a fill to minimize the
damage
– Then these pulses are shifted by 5 us, it takes 40 such
steps (40 fills and not necessarily consecutive fills) to scan
the whole range of 400 us fill window.
– In standard DAQ in-fill pulses are sent every 10 fills.
Out of fill : laser pulses sent outside the muon fill over longer
period of time to study the long-term gain stability.
affects due Temperature variation, aging etc can be
corrected.
ble-pulses : additional (1 %) gain drop due to veryclose (~
10 ns) positron hits, to study this two very close laser
pulses are sent and the response is studied.
flight-simulator : positron events are simulated using
laser pulses that can also mimic the infamoussplash.
Pulse Tagging :
1.8 GeV pulse that is found almost (in more than 50
crystals) in all crystals is definitely a laser.
DocDb10818-v3
21 September 2018 Atanu Nath 70
Laser Control System
●
In-Fill : 2 pulses 200 us apart are sent in a fill to minimize the
damage
– Then these pulses are shifted by 5 us, it takes 40 such
steps (40 fills and not necessarily consecutive fills) to scan
the whole range of 400 us fill window.
– In standard DAQ in-fill pulses are sent every 10 fills.
Out of fill : laser pulses sent outside the muon fill over longer
period of time to study the long-term gain stability.
affects due Temperature variation, aging etc can be
corrected.
ble-pulses : additional (1 %) gain drop due to veryclose (~
10 ns) positron hits, to study this two very close laser
pulses are sent and the response is studied.
flight-simulator : positron events are simulated using
laser pulses that can also mimic the infamoussplash.
Pulse Tagging :
1.8 GeV pulse that is found almost (in more than 50
crystals) in all crystals is definitely a laser.
DocDb10818-v3
21 September 2018 Atanu Nath 71
Laser Control System
●
In-Fill : 2 pulses 200 us apart are sent in a fill to minimize the
damage
– Then these pulses are shifted by 5 us, it takes 40 such
steps (40 fills and not necessarily consecutive fills) to scan
the whole range of 400 us fill window.
– In standard DAQ in-fill pulses are sent every 10 fills.
Out of fill : laser pulses sent outside the muon fill over longer
period of time to study the long-term gain stability.
affects due Temperature variation, aging etc can be
corrected.
ble-pulses : additional (1 %) gain drop due to veryclose (~
10 ns) positron hits, to study this two very close laser
pulses are sent and the response is studied.
flight-simulator : positron events are simulated using
laser pulses that can also mimic the infamoussplash.
Pulse Tagging :
1.8 GeV pulse that is found almost (in more than 50
crystals) in all crystals is definitely a laser.
DocDb10818-v3
21 September 2018 Atanu Nath 72
Laser Control System
●
In-Fill : 2 pulses 200 us apart are sent in a fill to minimize the
damage
– Then these pulses are shifted by 5 us, it takes 40 such
steps (40 fills and not necessarily consecutive fills) to scan
the whole range of 400 us fill window.
– In standard DAQ in-fill pulses are sent every 10 fills.
Out of fill : laser pulses sent outside the muon fill over longer
period of time to study the long-term gain stability.
affects due Temperature variation, aging etc can be
corrected.
ble-pulses : additional (1 %) gain drop due to veryclose (~
10 ns) positron hits, to study this two very close laser
pulses are sent and the response is studied.
flight-simulator : positron events are simulated using
laser pulses that can also mimic the infamoussplash.
Pulse Tagging :
1.8 GeV pulse that is found almost (in more than 50
crystals) in all crystals is definitely a laser.
DocDb10818-v3
21 September 2018 Atanu Nath 73
Laser Control System
●
In-Fill : 2 pulses 200 us apart are sent in a fill to minimize the
damage
– Then these pulses are shifted by 5 us, it takes 40 such
steps (40 fills and not necessarily consecutive fills) to scan
the whole range of 400 us fill window.
– In standard DAQ in-fill pulses are sent every 10 fills.
Out of fill : laser pulses sent outside the muon fill over longer
period of time to study the long-term gain stability.
affects due Temperature variation, aging etc can be
corrected.
ble-pulses : additional (1 %) gain drop due to veryclose (~
10 ns) positron hits, to study this two very close laser
pulses are sent and the response is studied.
flight-simulator : positron events are simulated using
laser pulses that can also mimic the infamoussplash.
Pulse Tagging :
1.8 GeV pulse that is found almost (in more than 50
crystals) in all crystals is definitely a laser.
ODB: Laser pulse settings.
DocDb10818-v3
21 September 2018 Atanu Nath 74
Temperature Correlations...
0.4% per o
C 0.5% per o
C 0.1% per o
C
OctavioEscalante
OctavioEscalante
OctavioEscalante

More Related Content

What's hot

Particle flow calorimeter with ASIC readout
Particle flow calorimeter with ASIC readoutParticle flow calorimeter with ASIC readout
Particle flow calorimeter with ASIC readouteguliyev
 
IRJET-Weather Radar Range Velocity Ambiguity Analysis using Staggered PRT
IRJET-Weather Radar Range Velocity Ambiguity Analysis using Staggered PRTIRJET-Weather Radar Range Velocity Ambiguity Analysis using Staggered PRT
IRJET-Weather Radar Range Velocity Ambiguity Analysis using Staggered PRTIRJET Journal
 
Validation of different nowcasting models based on the Meteosat Second Genera...
Validation of different nowcasting models based on the Meteosat Second Genera...Validation of different nowcasting models based on the Meteosat Second Genera...
Validation of different nowcasting models based on the Meteosat Second Genera...Michele de Rosa
 
Oscilloscope Fundamentals, Hands-On Course at EELive 2014
Oscilloscope Fundamentals, Hands-On Course at EELive 2014Oscilloscope Fundamentals, Hands-On Course at EELive 2014
Oscilloscope Fundamentals, Hands-On Course at EELive 2014Rohde & Schwarz North America
 
Big Data Analytics for Power Grid Operations
Big Data Analytics for Power Grid OperationsBig Data Analytics for Power Grid Operations
Big Data Analytics for Power Grid OperationsPower System Operation
 
Radiation detection instrumentation fundamentals
Radiation detection instrumentation fundamentalsRadiation detection instrumentation fundamentals
Radiation detection instrumentation fundamentalsNitish Virmani
 
Atomic Absorption Spectrophotometer (AAS) by ACMAS Technologies Pvt Ltd.
Atomic Absorption Spectrophotometer (AAS) by ACMAS Technologies Pvt Ltd.Atomic Absorption Spectrophotometer (AAS) by ACMAS Technologies Pvt Ltd.
Atomic Absorption Spectrophotometer (AAS) by ACMAS Technologies Pvt Ltd.Acmas Technologies Pvt. Ltd.
 
Synchronization protection &amp; redundancy in ng networks itsf 2015
Synchronization protection &amp; redundancy in ng networks   itsf 2015Synchronization protection &amp; redundancy in ng networks   itsf 2015
Synchronization protection &amp; redundancy in ng networks itsf 2015Daniel Sproats
 
detectıon of dıseases usıng ECG signal
detectıon of dıseases usıng ECG signaldetectıon of dıseases usıng ECG signal
detectıon of dıseases usıng ECG signalSerhat Dağ
 
Patch Cord Test Adapter Data Sheet
Patch Cord Test Adapter Data SheetPatch Cord Test Adapter Data Sheet
Patch Cord Test Adapter Data SheetFluke Networks
 

What's hot (11)

Particle flow calorimeter with ASIC readout
Particle flow calorimeter with ASIC readoutParticle flow calorimeter with ASIC readout
Particle flow calorimeter with ASIC readout
 
IRJET-Weather Radar Range Velocity Ambiguity Analysis using Staggered PRT
IRJET-Weather Radar Range Velocity Ambiguity Analysis using Staggered PRTIRJET-Weather Radar Range Velocity Ambiguity Analysis using Staggered PRT
IRJET-Weather Radar Range Velocity Ambiguity Analysis using Staggered PRT
 
Real-Time Jitter Measurements
Real-Time Jitter Measurements Real-Time Jitter Measurements
Real-Time Jitter Measurements
 
Validation of different nowcasting models based on the Meteosat Second Genera...
Validation of different nowcasting models based on the Meteosat Second Genera...Validation of different nowcasting models based on the Meteosat Second Genera...
Validation of different nowcasting models based on the Meteosat Second Genera...
 
Oscilloscope Fundamentals, Hands-On Course at EELive 2014
Oscilloscope Fundamentals, Hands-On Course at EELive 2014Oscilloscope Fundamentals, Hands-On Course at EELive 2014
Oscilloscope Fundamentals, Hands-On Course at EELive 2014
 
Big Data Analytics for Power Grid Operations
Big Data Analytics for Power Grid OperationsBig Data Analytics for Power Grid Operations
Big Data Analytics for Power Grid Operations
 
Radiation detection instrumentation fundamentals
Radiation detection instrumentation fundamentalsRadiation detection instrumentation fundamentals
Radiation detection instrumentation fundamentals
 
Atomic Absorption Spectrophotometer (AAS) by ACMAS Technologies Pvt Ltd.
Atomic Absorption Spectrophotometer (AAS) by ACMAS Technologies Pvt Ltd.Atomic Absorption Spectrophotometer (AAS) by ACMAS Technologies Pvt Ltd.
Atomic Absorption Spectrophotometer (AAS) by ACMAS Technologies Pvt Ltd.
 
Synchronization protection &amp; redundancy in ng networks itsf 2015
Synchronization protection &amp; redundancy in ng networks   itsf 2015Synchronization protection &amp; redundancy in ng networks   itsf 2015
Synchronization protection &amp; redundancy in ng networks itsf 2015
 
detectıon of dıseases usıng ECG signal
detectıon of dıseases usıng ECG signaldetectıon of dıseases usıng ECG signal
detectıon of dıseases usıng ECG signal
 
Patch Cord Test Adapter Data Sheet
Patch Cord Test Adapter Data SheetPatch Cord Test Adapter Data Sheet
Patch Cord Test Adapter Data Sheet
 

Similar to Monitoring and Data Acquisition of the Laser Calibration System of Muon g-2 Experiment

Synchronization in SDH network
Synchronization in SDH networkSynchronization in SDH network
Synchronization in SDH networkasifmatin
 
Atc On An Simd Cots System Wmpp05
Atc On An Simd Cots System   Wmpp05Atc On An Simd Cots System   Wmpp05
Atc On An Simd Cots System Wmpp05Ülger Ahmet
 
Metal Detector Project
Metal Detector ProjectMetal Detector Project
Metal Detector ProjectDanish Bangash
 
Nano_PI_rvw
Nano_PI_rvwNano_PI_rvw
Nano_PI_rvwRaj Nair
 
Behalf Of Pamela Collaboration
Behalf Of Pamela CollaborationBehalf Of Pamela Collaboration
Behalf Of Pamela Collaborationahmad bassiouny
 
A CMOS 79GHz PMCW radar SOC
A CMOS 79GHz PMCW radar SOCA CMOS 79GHz PMCW radar SOC
A CMOS 79GHz PMCW radar SOCDr. Jianying Guo
 
Short Range Radar System using Arduino Uno
Short Range Radar System using Arduino UnoShort Range Radar System using Arduino Uno
Short Range Radar System using Arduino UnoIRJET Journal
 
Future accelerator scenarios
Future accelerator scenariosFuture accelerator scenarios
Future accelerator scenariosESS BILBAO
 
Basic Pitfalls in Waveform Analysis
Basic Pitfalls in Waveform AnalysisBasic Pitfalls in Waveform Analysis
Basic Pitfalls in Waveform AnalysisYukio Okuda
 
Williams_FR1_TO4_5_2011_07_29v1.ppt
Williams_FR1_TO4_5_2011_07_29v1.pptWilliams_FR1_TO4_5_2011_07_29v1.ppt
Williams_FR1_TO4_5_2011_07_29v1.pptgrssieee
 
Deep Dive 5G NR-RAN Release 2018 Q4 Swisscom - L1 & RM.pdf
Deep Dive 5G NR-RAN Release 2018 Q4 Swisscom - L1 & RM.pdfDeep Dive 5G NR-RAN Release 2018 Q4 Swisscom - L1 & RM.pdf
Deep Dive 5G NR-RAN Release 2018 Q4 Swisscom - L1 & RM.pdfDaniel Estrada
 
Review regional Source Specific Station Corrections (SSSCs) developed for no...
Review regional Source Specific Station Corrections (SSSCs) developed for  no...Review regional Source Specific Station Corrections (SSSCs) developed for  no...
Review regional Source Specific Station Corrections (SSSCs) developed for no...Ivan Kitov
 
Asiasim2004 final
Asiasim2004 finalAsiasim2004 final
Asiasim2004 finalvrsim
 
ALPIDE_65_02_09_2020.pptx submission of the
ALPIDE_65_02_09_2020.pptx submission of theALPIDE_65_02_09_2020.pptx submission of the
ALPIDE_65_02_09_2020.pptx submission of theManojYarlanki
 
2015_Mead_Patrick_Design_Portfolio_PCB
2015_Mead_Patrick_Design_Portfolio_PCB2015_Mead_Patrick_Design_Portfolio_PCB
2015_Mead_Patrick_Design_Portfolio_PCBPatrick Mead
 
Handheld Infrared Thermometer
Handheld Infrared ThermometerHandheld Infrared Thermometer
Handheld Infrared ThermometerPremier Farnell
 

Similar to Monitoring and Data Acquisition of the Laser Calibration System of Muon g-2 Experiment (20)

Synchronization in SDH network
Synchronization in SDH networkSynchronization in SDH network
Synchronization in SDH network
 
Atc On An Simd Cots System Wmpp05
Atc On An Simd Cots System   Wmpp05Atc On An Simd Cots System   Wmpp05
Atc On An Simd Cots System Wmpp05
 
CAPE Buoy
CAPE BuoyCAPE Buoy
CAPE Buoy
 
Metal Detector Project
Metal Detector ProjectMetal Detector Project
Metal Detector Project
 
Nano_PI_rvw
Nano_PI_rvwNano_PI_rvw
Nano_PI_rvw
 
An adjustable Comparator for 2-bit/step SAR ADC Configuring with multiple sam...
An adjustable Comparator for 2-bit/step SAR ADC Configuring with multiple sam...An adjustable Comparator for 2-bit/step SAR ADC Configuring with multiple sam...
An adjustable Comparator for 2-bit/step SAR ADC Configuring with multiple sam...
 
Behalf Of Pamela Collaboration
Behalf Of Pamela CollaborationBehalf Of Pamela Collaboration
Behalf Of Pamela Collaboration
 
A CMOS 79GHz PMCW radar SOC
A CMOS 79GHz PMCW radar SOCA CMOS 79GHz PMCW radar SOC
A CMOS 79GHz PMCW radar SOC
 
Short Range Radar System using Arduino Uno
Short Range Radar System using Arduino UnoShort Range Radar System using Arduino Uno
Short Range Radar System using Arduino Uno
 
Future accelerator scenarios
Future accelerator scenariosFuture accelerator scenarios
Future accelerator scenarios
 
Basic Pitfalls in Waveform Analysis
Basic Pitfalls in Waveform AnalysisBasic Pitfalls in Waveform Analysis
Basic Pitfalls in Waveform Analysis
 
Williams_FR1_TO4_5_2011_07_29v1.ppt
Williams_FR1_TO4_5_2011_07_29v1.pptWilliams_FR1_TO4_5_2011_07_29v1.ppt
Williams_FR1_TO4_5_2011_07_29v1.ppt
 
Deep Dive 5G NR-RAN Release 2018 Q4 Swisscom - L1 & RM.pdf
Deep Dive 5G NR-RAN Release 2018 Q4 Swisscom - L1 & RM.pdfDeep Dive 5G NR-RAN Release 2018 Q4 Swisscom - L1 & RM.pdf
Deep Dive 5G NR-RAN Release 2018 Q4 Swisscom - L1 & RM.pdf
 
Review regional Source Specific Station Corrections (SSSCs) developed for no...
Review regional Source Specific Station Corrections (SSSCs) developed for  no...Review regional Source Specific Station Corrections (SSSCs) developed for  no...
Review regional Source Specific Station Corrections (SSSCs) developed for no...
 
Psat toolbox-8631349
Psat toolbox-8631349Psat toolbox-8631349
Psat toolbox-8631349
 
Asiasim2004 final
Asiasim2004 finalAsiasim2004 final
Asiasim2004 final
 
ALPIDE_65_02_09_2020.pptx submission of the
ALPIDE_65_02_09_2020.pptx submission of theALPIDE_65_02_09_2020.pptx submission of the
ALPIDE_65_02_09_2020.pptx submission of the
 
2015_Mead_Patrick_Design_Portfolio_PCB
2015_Mead_Patrick_Design_Portfolio_PCB2015_Mead_Patrick_Design_Portfolio_PCB
2015_Mead_Patrick_Design_Portfolio_PCB
 
Handheld Infrared Thermometer
Handheld Infrared ThermometerHandheld Infrared Thermometer
Handheld Infrared Thermometer
 
GR820
GR820GR820
GR820
 

More from Atanu Nath

Fermilab Muon g − 2 Experiment: Laser Based Gain Calibration System
Fermilab Muon g − 2 Experiment: Laser Based Gain Calibration SystemFermilab Muon g − 2 Experiment: Laser Based Gain Calibration System
Fermilab Muon g − 2 Experiment: Laser Based Gain Calibration SystemAtanu Nath
 
Fermilab Muon g − 2 Experiment: Current Status
Fermilab Muon g − 2 Experiment: Current StatusFermilab Muon g − 2 Experiment: Current Status
Fermilab Muon g − 2 Experiment: Current StatusAtanu Nath
 
The Calibration System For The Muon g-2 Experiment @ Fermilab
The Calibration System For The Muon g-2 Experiment @ FermilabThe Calibration System For The Muon g-2 Experiment @ Fermilab
The Calibration System For The Muon g-2 Experiment @ FermilabAtanu Nath
 
Magnetic Moment of Muons and New Physics
Magnetic Moment of Muons and New PhysicsMagnetic Moment of Muons and New Physics
Magnetic Moment of Muons and New PhysicsAtanu Nath
 
Muon g-2 and Physics Beyond Standard Model
Muon g-2 and Physics Beyond Standard ModelMuon g-2 and Physics Beyond Standard Model
Muon g-2 and Physics Beyond Standard ModelAtanu Nath
 
Rare Kaon Decays: Matching Long and Short Distance Physics in K-> Pi e+ e-
Rare Kaon Decays: Matching Long and Short Distance Physics in K-> Pi e+ e-Rare Kaon Decays: Matching Long and Short Distance Physics in K-> Pi e+ e-
Rare Kaon Decays: Matching Long and Short Distance Physics in K-> Pi e+ e-Atanu Nath
 

More from Atanu Nath (7)

Fermilab Muon g − 2 Experiment: Laser Based Gain Calibration System
Fermilab Muon g − 2 Experiment: Laser Based Gain Calibration SystemFermilab Muon g − 2 Experiment: Laser Based Gain Calibration System
Fermilab Muon g − 2 Experiment: Laser Based Gain Calibration System
 
Fermilab Muon g − 2 Experiment: Current Status
Fermilab Muon g − 2 Experiment: Current StatusFermilab Muon g − 2 Experiment: Current Status
Fermilab Muon g − 2 Experiment: Current Status
 
The Calibration System For The Muon g-2 Experiment @ Fermilab
The Calibration System For The Muon g-2 Experiment @ FermilabThe Calibration System For The Muon g-2 Experiment @ Fermilab
The Calibration System For The Muon g-2 Experiment @ Fermilab
 
Magnetic Moment of Muons and New Physics
Magnetic Moment of Muons and New PhysicsMagnetic Moment of Muons and New Physics
Magnetic Moment of Muons and New Physics
 
Muon g-2 and Physics Beyond Standard Model
Muon g-2 and Physics Beyond Standard ModelMuon g-2 and Physics Beyond Standard Model
Muon g-2 and Physics Beyond Standard Model
 
finalreport
finalreportfinalreport
finalreport
 
Rare Kaon Decays: Matching Long and Short Distance Physics in K-> Pi e+ e-
Rare Kaon Decays: Matching Long and Short Distance Physics in K-> Pi e+ e-Rare Kaon Decays: Matching Long and Short Distance Physics in K-> Pi e+ e-
Rare Kaon Decays: Matching Long and Short Distance Physics in K-> Pi e+ e-
 

Recently uploaded

❤Jammu Kashmir Call Girls 8617697112 Personal Whatsapp Number 💦✅.
❤Jammu Kashmir Call Girls 8617697112 Personal Whatsapp Number 💦✅.❤Jammu Kashmir Call Girls 8617697112 Personal Whatsapp Number 💦✅.
❤Jammu Kashmir Call Girls 8617697112 Personal Whatsapp Number 💦✅.Nitya salvi
 
Justdial Call Girls In Indirapuram, Ghaziabad, 8800357707 Escorts Service
Justdial Call Girls In Indirapuram, Ghaziabad, 8800357707 Escorts ServiceJustdial Call Girls In Indirapuram, Ghaziabad, 8800357707 Escorts Service
Justdial Call Girls In Indirapuram, Ghaziabad, 8800357707 Escorts Servicemonikaservice1
 
SCIENCE-4-QUARTER4-WEEK-4-PPT-1 (1).pptx
SCIENCE-4-QUARTER4-WEEK-4-PPT-1 (1).pptxSCIENCE-4-QUARTER4-WEEK-4-PPT-1 (1).pptx
SCIENCE-4-QUARTER4-WEEK-4-PPT-1 (1).pptxRizalinePalanog2
 
Call Girls Alandi Call Me 7737669865 Budget Friendly No Advance Booking
Call Girls Alandi Call Me 7737669865 Budget Friendly No Advance BookingCall Girls Alandi Call Me 7737669865 Budget Friendly No Advance Booking
Call Girls Alandi Call Me 7737669865 Budget Friendly No Advance Bookingroncy bisnoi
 
Introduction,importance and scope of horticulture.pptx
Introduction,importance and scope of horticulture.pptxIntroduction,importance and scope of horticulture.pptx
Introduction,importance and scope of horticulture.pptxBhagirath Gogikar
 
High Profile 🔝 8250077686 📞 Call Girls Service in GTB Nagar🍑
High Profile 🔝 8250077686 📞 Call Girls Service in GTB Nagar🍑High Profile 🔝 8250077686 📞 Call Girls Service in GTB Nagar🍑
High Profile 🔝 8250077686 📞 Call Girls Service in GTB Nagar🍑Damini Dixit
 
pumpkin fruit fly, water melon fruit fly, cucumber fruit fly
pumpkin fruit fly, water melon fruit fly, cucumber fruit flypumpkin fruit fly, water melon fruit fly, cucumber fruit fly
pumpkin fruit fly, water melon fruit fly, cucumber fruit flyPRADYUMMAURYA1
 
Pests of mustard_Identification_Management_Dr.UPR.pdf
Pests of mustard_Identification_Management_Dr.UPR.pdfPests of mustard_Identification_Management_Dr.UPR.pdf
Pests of mustard_Identification_Management_Dr.UPR.pdfPirithiRaju
 
GBSN - Microbiology (Unit 2)
GBSN - Microbiology (Unit 2)GBSN - Microbiology (Unit 2)
GBSN - Microbiology (Unit 2)Areesha Ahmad
 
STS-UNIT 4 CLIMATE CHANGE POWERPOINT PRESENTATION
STS-UNIT 4 CLIMATE CHANGE POWERPOINT PRESENTATIONSTS-UNIT 4 CLIMATE CHANGE POWERPOINT PRESENTATION
STS-UNIT 4 CLIMATE CHANGE POWERPOINT PRESENTATIONrouseeyyy
 
GBSN - Biochemistry (Unit 1)
GBSN - Biochemistry (Unit 1)GBSN - Biochemistry (Unit 1)
GBSN - Biochemistry (Unit 1)Areesha Ahmad
 
9999266834 Call Girls In Noida Sector 22 (Delhi) Call Girl Service
9999266834 Call Girls In Noida Sector 22 (Delhi) Call Girl Service9999266834 Call Girls In Noida Sector 22 (Delhi) Call Girl Service
9999266834 Call Girls In Noida Sector 22 (Delhi) Call Girl Servicenishacall1
 
High Class Escorts in Hyderabad ₹7.5k Pick Up & Drop With Cash Payment 969456...
High Class Escorts in Hyderabad ₹7.5k Pick Up & Drop With Cash Payment 969456...High Class Escorts in Hyderabad ₹7.5k Pick Up & Drop With Cash Payment 969456...
High Class Escorts in Hyderabad ₹7.5k Pick Up & Drop With Cash Payment 969456...chandars293
 
SAMASTIPUR CALL GIRL 7857803690 LOW PRICE ESCORT SERVICE
SAMASTIPUR CALL GIRL 7857803690  LOW PRICE  ESCORT SERVICESAMASTIPUR CALL GIRL 7857803690  LOW PRICE  ESCORT SERVICE
SAMASTIPUR CALL GIRL 7857803690 LOW PRICE ESCORT SERVICEayushi9330
 
COMPUTING ANTI-DERIVATIVES (Integration by SUBSTITUTION)
COMPUTING ANTI-DERIVATIVES(Integration by SUBSTITUTION)COMPUTING ANTI-DERIVATIVES(Integration by SUBSTITUTION)
COMPUTING ANTI-DERIVATIVES (Integration by SUBSTITUTION)AkefAfaneh2
 
Pests of cotton_Borer_Pests_Binomics_Dr.UPR.pdf
Pests of cotton_Borer_Pests_Binomics_Dr.UPR.pdfPests of cotton_Borer_Pests_Binomics_Dr.UPR.pdf
Pests of cotton_Borer_Pests_Binomics_Dr.UPR.pdfPirithiRaju
 
Module for Grade 9 for Asynchronous/Distance learning
Module for Grade 9 for Asynchronous/Distance learningModule for Grade 9 for Asynchronous/Distance learning
Module for Grade 9 for Asynchronous/Distance learninglevieagacer
 
Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b
Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 bAsymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b
Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 bSérgio Sacani
 
Chemical Tests; flame test, positive and negative ions test Edexcel Internati...
Chemical Tests; flame test, positive and negative ions test Edexcel Internati...Chemical Tests; flame test, positive and negative ions test Edexcel Internati...
Chemical Tests; flame test, positive and negative ions test Edexcel Internati...ssuser79fe74
 
Pests of cotton_Sucking_Pests_Dr.UPR.pdf
Pests of cotton_Sucking_Pests_Dr.UPR.pdfPests of cotton_Sucking_Pests_Dr.UPR.pdf
Pests of cotton_Sucking_Pests_Dr.UPR.pdfPirithiRaju
 

Recently uploaded (20)

❤Jammu Kashmir Call Girls 8617697112 Personal Whatsapp Number 💦✅.
❤Jammu Kashmir Call Girls 8617697112 Personal Whatsapp Number 💦✅.❤Jammu Kashmir Call Girls 8617697112 Personal Whatsapp Number 💦✅.
❤Jammu Kashmir Call Girls 8617697112 Personal Whatsapp Number 💦✅.
 
Justdial Call Girls In Indirapuram, Ghaziabad, 8800357707 Escorts Service
Justdial Call Girls In Indirapuram, Ghaziabad, 8800357707 Escorts ServiceJustdial Call Girls In Indirapuram, Ghaziabad, 8800357707 Escorts Service
Justdial Call Girls In Indirapuram, Ghaziabad, 8800357707 Escorts Service
 
SCIENCE-4-QUARTER4-WEEK-4-PPT-1 (1).pptx
SCIENCE-4-QUARTER4-WEEK-4-PPT-1 (1).pptxSCIENCE-4-QUARTER4-WEEK-4-PPT-1 (1).pptx
SCIENCE-4-QUARTER4-WEEK-4-PPT-1 (1).pptx
 
Call Girls Alandi Call Me 7737669865 Budget Friendly No Advance Booking
Call Girls Alandi Call Me 7737669865 Budget Friendly No Advance BookingCall Girls Alandi Call Me 7737669865 Budget Friendly No Advance Booking
Call Girls Alandi Call Me 7737669865 Budget Friendly No Advance Booking
 
Introduction,importance and scope of horticulture.pptx
Introduction,importance and scope of horticulture.pptxIntroduction,importance and scope of horticulture.pptx
Introduction,importance and scope of horticulture.pptx
 
High Profile 🔝 8250077686 📞 Call Girls Service in GTB Nagar🍑
High Profile 🔝 8250077686 📞 Call Girls Service in GTB Nagar🍑High Profile 🔝 8250077686 📞 Call Girls Service in GTB Nagar🍑
High Profile 🔝 8250077686 📞 Call Girls Service in GTB Nagar🍑
 
pumpkin fruit fly, water melon fruit fly, cucumber fruit fly
pumpkin fruit fly, water melon fruit fly, cucumber fruit flypumpkin fruit fly, water melon fruit fly, cucumber fruit fly
pumpkin fruit fly, water melon fruit fly, cucumber fruit fly
 
Pests of mustard_Identification_Management_Dr.UPR.pdf
Pests of mustard_Identification_Management_Dr.UPR.pdfPests of mustard_Identification_Management_Dr.UPR.pdf
Pests of mustard_Identification_Management_Dr.UPR.pdf
 
GBSN - Microbiology (Unit 2)
GBSN - Microbiology (Unit 2)GBSN - Microbiology (Unit 2)
GBSN - Microbiology (Unit 2)
 
STS-UNIT 4 CLIMATE CHANGE POWERPOINT PRESENTATION
STS-UNIT 4 CLIMATE CHANGE POWERPOINT PRESENTATIONSTS-UNIT 4 CLIMATE CHANGE POWERPOINT PRESENTATION
STS-UNIT 4 CLIMATE CHANGE POWERPOINT PRESENTATION
 
GBSN - Biochemistry (Unit 1)
GBSN - Biochemistry (Unit 1)GBSN - Biochemistry (Unit 1)
GBSN - Biochemistry (Unit 1)
 
9999266834 Call Girls In Noida Sector 22 (Delhi) Call Girl Service
9999266834 Call Girls In Noida Sector 22 (Delhi) Call Girl Service9999266834 Call Girls In Noida Sector 22 (Delhi) Call Girl Service
9999266834 Call Girls In Noida Sector 22 (Delhi) Call Girl Service
 
High Class Escorts in Hyderabad ₹7.5k Pick Up & Drop With Cash Payment 969456...
High Class Escorts in Hyderabad ₹7.5k Pick Up & Drop With Cash Payment 969456...High Class Escorts in Hyderabad ₹7.5k Pick Up & Drop With Cash Payment 969456...
High Class Escorts in Hyderabad ₹7.5k Pick Up & Drop With Cash Payment 969456...
 
SAMASTIPUR CALL GIRL 7857803690 LOW PRICE ESCORT SERVICE
SAMASTIPUR CALL GIRL 7857803690  LOW PRICE  ESCORT SERVICESAMASTIPUR CALL GIRL 7857803690  LOW PRICE  ESCORT SERVICE
SAMASTIPUR CALL GIRL 7857803690 LOW PRICE ESCORT SERVICE
 
COMPUTING ANTI-DERIVATIVES (Integration by SUBSTITUTION)
COMPUTING ANTI-DERIVATIVES(Integration by SUBSTITUTION)COMPUTING ANTI-DERIVATIVES(Integration by SUBSTITUTION)
COMPUTING ANTI-DERIVATIVES (Integration by SUBSTITUTION)
 
Pests of cotton_Borer_Pests_Binomics_Dr.UPR.pdf
Pests of cotton_Borer_Pests_Binomics_Dr.UPR.pdfPests of cotton_Borer_Pests_Binomics_Dr.UPR.pdf
Pests of cotton_Borer_Pests_Binomics_Dr.UPR.pdf
 
Module for Grade 9 for Asynchronous/Distance learning
Module for Grade 9 for Asynchronous/Distance learningModule for Grade 9 for Asynchronous/Distance learning
Module for Grade 9 for Asynchronous/Distance learning
 
Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b
Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 bAsymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b
Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b
 
Chemical Tests; flame test, positive and negative ions test Edexcel Internati...
Chemical Tests; flame test, positive and negative ions test Edexcel Internati...Chemical Tests; flame test, positive and negative ions test Edexcel Internati...
Chemical Tests; flame test, positive and negative ions test Edexcel Internati...
 
Pests of cotton_Sucking_Pests_Dr.UPR.pdf
Pests of cotton_Sucking_Pests_Dr.UPR.pdfPests of cotton_Sucking_Pests_Dr.UPR.pdf
Pests of cotton_Sucking_Pests_Dr.UPR.pdf
 

Monitoring and Data Acquisition of the Laser Calibration System of Muon g-2 Experiment

  • 1. Monitoring and Data Acquisition of the Laser Calibration System of Muon g-2 Experiment Atanu Nath (On behalf of the Muon g-2 collaboration) 104° Congresso Nazionale 21st September 2018, Cosenza, Calabria
  • 2. 21 September 2018 Atanu Nath 2 Outline The main components – Laser control system – Source Monitors – Local Monitors Data acquisition & monitoring systems – MIDAS DAQ – Naples DAQ
  • 3. 21 September 2018 Atanu Nath 3
  • 4. 21 September 2018 Atanu Nath 4
  • 5. 21 September 2018 Atanu Nath 5 Laser Controller
  • 6. 21 September 2018 Atanu Nath 6 Laser Control System In-Fill : 2 pulses 200 us apart are sent every fill to minimize the damage Then these pulses are shifted by 5 us to scan the whole range of 400 us fill window. In standard DAQ in-fill pulses are sent every 10 fills. Out of fill : laser pulses sent outside the muon fill over longer period of time to study the long-term gain stability. affects due Temperature variation, aging etc can be corrected. double-pulses : additional (1 %) gain drop due to very close (~ 10 ns) positron hits, to study this two very close laser pulses are sent and the response is studied. flight-simulator : positron events are simulated using laser pulses that can also mimic the infamoussplash. Laser Pulse Tagging : 1.8 GeV pulse that is found almost (in more than 50 crystals) in all crystals is definitely a laser. burst Test pulse 500 ns 40 us
  • 7. 21 September 2018 Atanu Nath 7 Laser Control System In-Fill : 2 pulses 200 us apart are sent every fill to minimize the damage Then these pulses are shifted by 5 us, it takes 40 such steps (40 fills and not necessarily consecutive fills) to scan the whole range of 400 us fill window. In standard DAQ in-fill pulses are sent every 10 fills. ● Out of fill : laser pulses sent outside the muon fill over longer period of time to study the long-term gain stability. – affects due Temperature variation, aging etc can be corrected. – double-pulses : additional (1 %) gain drop due to very close (~ 10 ns) positron hits, to study this two very close laser pulses are sent and the response is studied. – flight-simulator : positron events are simulated using laser pulses that can also mimic the infamoussplash. Laser Pulse Tagging : 1.8 GeV pulse that is found almost (in more than 50 crystals) in all crystals is definitely a laser. burst Test pulse 500 ns 40 us
  • 8. 21 September 2018 Atanu Nath 8 Laser Control System In-Fill : 2 pulses 200 us apart are sent every fill to minimize the damage Then these pulses are shifted by 5 us, it takes 40 such steps (40 fills and not necessarily consecutive fills) to scan the whole range of 400 us fill window. In standard DAQ in-fill pulses are sent every 10 fills. f fill : laser pulses sent outside the muon fill over longer period of time to study the long-term gain stability. affects due Temperature variation, aging etc can be corrected. double-pulses : additional (1 %) gain drop due to very close (~ 10 ns) positron hits, to study this two very close laser pulses are sent and the response is studied. flight-simulator : positron events are simulated using laser pulses that can also mimic the infamoussplash. ● Laser Pulse Tagging : – 1.8 GeV pulse that is found almost (in more than 50 crystals) in all crystals is definitely a laser. burst Test pulse 500 ns 40 us
  • 9. 21 September 2018 Atanu Nath 9 The Monitors...
  • 10. 21 September 2018 Atanu Nath 10 Source Monitors × 66 PiDPiD PiDPiD PMTPMT
  • 11. 21 September 2018 Atanu Nath 11 Source Monitors × 66 PMT PiD-1 PiD-2
  • 12. 21 September 2018 Atanu Nath 12 Source Monitors × 66 PiDPiD PiDPiD PMTPMT ● 2 Pin Diodes : receive laser pulses directly from the source. Pin-1/Pin-2 ~ stability at sub per mil 1 PMT : receives laser light from laser source plus light generated by (NaI) an americium source. Laser/Americium ~ the laser-source variation. which will be useful for the long term calibration. 60 HOURS
  • 13. 21 September 2018 Atanu Nath 13 Source Monitors × 66 PiDPiD PiDPiD PMTPMT Pin Diodes : receive laser pulses directly from the source. Pin-1/Pin-2 ~ stability at sub per mil ● 1 PMT : receives laser light from laser source plus light generated by (NaI) an americium source. – Laser/Americium ~ the laser-source variation. which will be useful for the long term calibration. 60 HOURS
  • 14. 21 September 2018 Atanu Nath 14 Local monitors × 2424
  • 15. 21 September 2018 Atanu Nath 15 Local monitors × 2424 ● 1 PMT (Plan of 2 actually) : receives laser pulses directly from the Source Monitors (Pulse-1) as well as light coming back from the calorimeters (Pulse-2). – Pulse-1/Pulse-2 ~ stability of the Local Monitors. 1 PMT : receives laser light from laser plus americium source. Laser/Americiu m ~ the laser-source variation. which will be useful for the long term calibration. , Hours (July 1st – 4th , 2017) Pulse-1/Pulse-2 Run 1791 - 1796 AnnaDriutti
  • 16. 21 September 2018 Atanu Nath 16 Data Acquisition Systems
  • 17. 21 September 2018 Atanu Nath 17 MIDAS DAQ & Monitoring System
  • 18. 21 September 2018 Atanu Nath 18 MIDAS DAQ uTCA based WFDs GPUs (Graphics Processing) 20 GB/s ODB (PostgreSQL)200 MB/s Fermilab Storage200 MB/s Online Data Quality Monitoring Maximum Integrated Data Acquisition System
  • 19. 21 September 2018 Atanu Nath 19 MIDAS DAQ ● Runs can be started and managed from the web-interface. ● Alarm goes off when something goes wrong. ● Configurations can be changed in the Online DataBase.
  • 20. 21 September 2018 Atanu Nath 20 Online Database ● Various configurations like laser mode filter-wheel position etc can be set in the Online DataBase page.
  • 21. 21 September 2018 Atanu Nath 21 Online Data Quality Monitor *.mid bnary file ROOT files Art-based Analysis Online Plots
  • 22. 21 September 2018 Atanu Nath 22 Online Data Quality Monitor ● Server connection status. ● Traces of laser signals. ● Stability of laser pulses over various runs. ● Alarms go off when things go wrong.
  • 23. 21 September 2018 Atanu Nath 23 Slow-control DQM 1 WEEK 1 DAY TEMP. BIAS & HVs FILTERS & MIRRORS NETWORKS
  • 24. 21 September 2018 Atanu Nath 24 Naples DAQ & Monitoring System
  • 25. 21 September 2018 Atanu Nath 25 Naples DAQ 6 x Custom made Digitizer Board Custom Made Event-builder Controller Board Naples Database Naples Storage Online Monitoring Custom made (bash, c++, ROOT) Naples DAQ and Monitoring PackageRelayed ToWFDs
  • 26. 21 September 2018 Atanu Nath 26 PMT Pin-1 Pin-2 S M B # 1 PMT Pin-1 Pin-2 S M B # 2 PMT Pin-1 Pin-2 S M B # 3 PMT Pin-1 Pin-2 S M B # 4 PMT Pin-1 Pin-2 S M B # 5 PMT Pin-1 Pin-2 S M B # 6 CONTROLLER BOARD SERVER DATA STORAGE & MONITORING SERVER I N T E R N E T
  • 27. 21 September 2018 Atanu Nath 27 Naples DAQ Custom made Source Monitor crate of Naples. Laser Control
  • 28. 21 September 2018 Atanu Nath 28 Naples DAQ Custom made Source Monitor crate of Naples. Laser Control
  • 29. 21 September 2018 Atanu Nath 29 Naples DAQ Custom made Source Monitor crate of Naples. SM Digitizer – 1 to 6 Pre-amplifier Shaper Digitizer. Provides bias/HV to the detectors.
  • 30. 21 September 2018 Atanu Nath 30 Naples DAQ Custom made Source Monitor crate of Naples. SM Digitizer – 1 to 6 PiD/PMT Signal Shaper Long-tail (20 us) Semi Gaussian) Baseline restorer Digitizer
  • 31. 21 September 2018 Atanu Nath 31 Naples DAQ Custom made Source Monitor crate of Naples. SM Event Builder (Controller Board) Receives data frame from all the 66 SM boards and checks for errors and then builds the final data frame containing information of 6x3 = 1818 channels. Sends the data frame to Naples Database over ethernet.
  • 32. 21 September 2018 Atanu Nath 32 Naples DAQ Custom made Source Monitor crate of Naples. SM Event Builder (Controller Board) Receives data frame from all the 66 SM boards and checks for errors and then builds the final data frame containing information of 6x3 = 1818 channels. Sends the data frame to the data farm over ethernet.
  • 33. 21 September 2018 Atanu Nath 33 Naples DAQ Custom made Source Monitor crate of Naples. 3 x 6 = 18 Board Temp. sensors 3 x 6 = 18 Pre Amp. Temp. sensors 2 x 6 = 12 Laser-hut Temp. sensors 0.1 o C Sensitivity
  • 34. 21 September 2018 Atanu Nath 34 Naples Monitoring...
  • 35. 21 September 2018 Atanu Nath 35 DATA FRAMEDATA FRAME In the Controller BoardIn the Controller Board
  • 36. 21 September 2018 Atanu Nath 36 CONTROLLER BOARD MONITORING SERVER Asks the controller board to send the latest data frame. Analyzes the latest frame on arrival and stores the results in a buffer… Displays the results of last minute. Displays the results of last several hours.
  • 37. 21 September 2018 Atanu Nath 37 Online Summary Table
  • 38. 21 September 2018 Atanu Nath 38 Short Term Trends
  • 39. 21 September 2018 Atanu Nath 39 Long Term Trends
  • 40. 21 September 2018 Atanu Nath 40 STABILITY OF THE MONITORS
  • 41. 21 September 2018 Atanu Nath 41 CALCULATION OF STABILITY ~ 1 MINUTE
  • 42. 21 September 2018 Atanu Nath 42 CALCULATION OF STABILITY ~ 1 MINUTE
  • 43. 21 September 2018 Atanu Nath 43 CALCULATION OF STABILITY ~ 1 MINUTE Pinratiofluctuation
  • 44. 21 September 2018 Atanu Nath 44 FLUCTUATION OVER LONGER TIME
  • 45. 21 September 2018 Atanu Nath 45 Stability Plots
  • 46. 21 September 2018 Atanu Nath 46 Electronic Calibration DAQ
  • 47. 21 September 2018 Atanu Nath 47 Calibration of The Electronics PMT Pre-amp. S M B PiD-1 Pre-amp. PiD-1 Pre-amp. A chain of known charge pulses Called “DAC”s
  • 48. 21 September 2018 Atanu Nath 48 Linearity Test S M B A chain of known charge pulses Called “DAC”s
  • 49. 21 September 2018 Atanu Nath 49 Temperature Correction PMT PIN-1 PIN-2 CALIBRATION RAMPING
  • 50. 21 September 2018 Atanu Nath 50 Temperature Correction PMT 0.1 % / o C Pin 1, 2 ~ 0.4 % / o C
  • 51. 21 September 2018 Atanu Nath 51 Temperature Correction UNCORRECTED CORRECTED 10 DAYS OctavioEscalante
  • 52. 21 September 2018 Atanu Nath 52 Current Status and Plans ● Laser DAQs (MIDAS & Naples) are running 24x7 flawlessly since the beginning (2017). ● Monitoring of short-term – event by event – last minute and ● long-term – last 24 hours of laser trend – last few weeks of temperature trends are running smoothly.
  • 53. 21 September 2018 Atanu Nath 53 GRAZIE
  • 54. 21 September 2018 Atanu Nath 54
  • 55. 21 September 2018 Atanu Nath 55 Numbers: ● SM input 150 pJ/pulse ● LM input 0.01 pJ/pulse ● Americium ~ 10 Hz ● Laser source: pico quant, 750 pJ @ 450 nm, average power 28 mW ●
  • 56. 21 September 2018 Atanu Nath 56 Why Laser Calibration?
  • 57. 21 September 2018 Atanu Nath 57 Why laser calibration? Time [ns] Two nano-secs apart particles hitting the calorimeter ~ typical SiPM charging up time. -4% -8% VERY SHORT IN-FILL DocDb10818-v3
  • 58. 21 September 2018 Atanu Nath 58 Why laser calibration? Time [us] IN-FILL High load in the first few micro-secs after the injection results in a SiPM gain recovery time ~ few tens of micro-secs QUITE LONG DocDb10818-v3
  • 59. 21 September 2018 Atanu Nath 59 Why laser calibration? Time [hours] Variation[%] Temperature[0 C] LONG TERM Much slower gain changes over longer time (hours/days) Can occur due to temperature change, aging etc. VERY LONG DocDb10818-v3
  • 60. 21 September 2018 Atanu Nath 60 Why laser calibration? Gain Sagging Short-term Expected < 1% but we have seen ~ 10% Megaboxes improves the situation, reduces the time constant, but the drop is there. Long-term Huge temperature variation, different beam conditions, aging etc can affect the gain significantly over longer time scale. . Calorimeter Number Calorimeter Number Run 11224 ~ 1 WEEK~ 1 WEEK Gainvariationbetween35-40us Gainvariationbetween35-40us Run 09183 In-fill gain function can be different in different runs separated by weeks due to different beam conditions. ANOTHER LONG ONE.. SAME CALO CAN SAG DIFFERENTLY @ DIFFERENT TIMES DocDb10818-v3 DocDb10818-v3
  • 61. 21 September 2018 Atanu Nath 61 The laser calibration system ● Using laser pulses of known amplitude we can extract those “3 kinds” of gain functions and correct the real data. But those pulses have to be known, stuff like temperature and aging can also affect the laser sources, that’s why we need a monitoring system for the laser sources right after the light leaves the source : the Source Monitors They must also remain known till the end right before hitting the calorimeters after traveling through a long distribution system, therefore a monitoring system that monitors the local (light coming back from the calorimeters) situation is needed : the Local Monitors But wouldn’t these laser pulses mess with the positron signals? They would! That’s why we need to control the laser pulses in a specific manner so that a few pulses during the muon fills and a few outside of that suffice to get us the gain function : the Laser Control
  • 62. 21 September 2018 Atanu Nath 62
  • 63. 21 September 2018 Atanu Nath 63 ● Using laser pulses of known amplitude we can extract those “3 kinds” of gain functions and correct the real data. But those pulses have to be known, stuff like temperature and aging can also affect the laser sources, that’s why we need a monitoring system for the laser sources right after the light leaves the source : ● the Source Monitors They must also remain known till the end right before hitting the calorimeters after traveling through a long distribution system, therefore a monitoring system that monitors the local (light coming back from the calorimeters) situation is needed : the Local Monitors But wouldn’t these laser pulses mess with the positron signals? They would! That’s why we need to control the laser pulses in a specific manner so that a few pulses during the muon fills and a few outside of that suffice to get us the gain function : the Laser Control The laser calibration system
  • 64. 21 September 2018 Atanu Nath 64
  • 65. 21 September 2018 Atanu Nath 65 The laser calibration system ● Using laser pulses of known amplitude we can extract those “3 kinds” of gain functions and correct the real data. But those pulses have to be known, stuff like temperature and aging can also affect the laser sources, that’s why we need a monitoring system for the laser sources right after the light leaves the source : ● the Source Monitors They must also remain known till the end right before hitting the calorimeters after traveling through a long distribution system, therefore a monitoring system that monitors the local (light coming back from the calorimeters) situation is needed : ● the Local Monitors But wouldn’t these laser pulses mess with the positron signals? They would! That’s why we need to control the laser pulses in a specific manner so that a few pulses during the muon fills and a few outside of that suffice to get us the gain function : the Laser Control
  • 66. 21 September 2018 Atanu Nath 66
  • 67. 21 September 2018 Atanu Nath 67 The laser calibration system ● Using laser pulses of known amplitude we can extract those “3 kinds” of gain functions and correct the real data. But those pulses have to be known, stuff like temperature and aging can also affect the laser sources, that’s why we need a monitoring system for the laser sources right after the light leaves the source : ● the Source Monitors They must also remain known till the end right before hitting the calorimeters after traveling through a long distribution system, therefore a monitoring system that monitors the local (light coming back from the calorimeters) situation is needed : ● the Local Monitors – But wouldn’t these laser pulses mess with the positron signal? They would! That’s why we need to control the laser pulses in a specific manner so that a few pulses during the muon fills and a few outside of that suffice to get us the gain function : ● the Laser Control
  • 68. 21 September 2018 Atanu Nath 68
  • 69. 21 September 2018 Atanu Nath 69 Laser Control System ● In-Fill : 2 pulses 200 us apart are sent in a fill to minimize the damage – Then these pulses are shifted by 5 us, it takes 40 such steps (40 fills and not necessarily consecutive fills) to scan the whole range of 400 us fill window. – In standard DAQ in-fill pulses are sent every 10 fills. Out of fill : laser pulses sent outside the muon fill over longer period of time to study the long-term gain stability. affects due Temperature variation, aging etc can be corrected. ble-pulses : additional (1 %) gain drop due to veryclose (~ 10 ns) positron hits, to study this two very close laser pulses are sent and the response is studied. flight-simulator : positron events are simulated using laser pulses that can also mimic the infamoussplash. Pulse Tagging : 1.8 GeV pulse that is found almost (in more than 50 crystals) in all crystals is definitely a laser. DocDb10818-v3
  • 70. 21 September 2018 Atanu Nath 70 Laser Control System ● In-Fill : 2 pulses 200 us apart are sent in a fill to minimize the damage – Then these pulses are shifted by 5 us, it takes 40 such steps (40 fills and not necessarily consecutive fills) to scan the whole range of 400 us fill window. – In standard DAQ in-fill pulses are sent every 10 fills. Out of fill : laser pulses sent outside the muon fill over longer period of time to study the long-term gain stability. affects due Temperature variation, aging etc can be corrected. ble-pulses : additional (1 %) gain drop due to veryclose (~ 10 ns) positron hits, to study this two very close laser pulses are sent and the response is studied. flight-simulator : positron events are simulated using laser pulses that can also mimic the infamoussplash. Pulse Tagging : 1.8 GeV pulse that is found almost (in more than 50 crystals) in all crystals is definitely a laser. DocDb10818-v3
  • 71. 21 September 2018 Atanu Nath 71 Laser Control System ● In-Fill : 2 pulses 200 us apart are sent in a fill to minimize the damage – Then these pulses are shifted by 5 us, it takes 40 such steps (40 fills and not necessarily consecutive fills) to scan the whole range of 400 us fill window. – In standard DAQ in-fill pulses are sent every 10 fills. Out of fill : laser pulses sent outside the muon fill over longer period of time to study the long-term gain stability. affects due Temperature variation, aging etc can be corrected. ble-pulses : additional (1 %) gain drop due to veryclose (~ 10 ns) positron hits, to study this two very close laser pulses are sent and the response is studied. flight-simulator : positron events are simulated using laser pulses that can also mimic the infamoussplash. Pulse Tagging : 1.8 GeV pulse that is found almost (in more than 50 crystals) in all crystals is definitely a laser. DocDb10818-v3
  • 72. 21 September 2018 Atanu Nath 72 Laser Control System ● In-Fill : 2 pulses 200 us apart are sent in a fill to minimize the damage – Then these pulses are shifted by 5 us, it takes 40 such steps (40 fills and not necessarily consecutive fills) to scan the whole range of 400 us fill window. – In standard DAQ in-fill pulses are sent every 10 fills. Out of fill : laser pulses sent outside the muon fill over longer period of time to study the long-term gain stability. affects due Temperature variation, aging etc can be corrected. ble-pulses : additional (1 %) gain drop due to veryclose (~ 10 ns) positron hits, to study this two very close laser pulses are sent and the response is studied. flight-simulator : positron events are simulated using laser pulses that can also mimic the infamoussplash. Pulse Tagging : 1.8 GeV pulse that is found almost (in more than 50 crystals) in all crystals is definitely a laser. DocDb10818-v3
  • 73. 21 September 2018 Atanu Nath 73 Laser Control System ● In-Fill : 2 pulses 200 us apart are sent in a fill to minimize the damage – Then these pulses are shifted by 5 us, it takes 40 such steps (40 fills and not necessarily consecutive fills) to scan the whole range of 400 us fill window. – In standard DAQ in-fill pulses are sent every 10 fills. Out of fill : laser pulses sent outside the muon fill over longer period of time to study the long-term gain stability. affects due Temperature variation, aging etc can be corrected. ble-pulses : additional (1 %) gain drop due to veryclose (~ 10 ns) positron hits, to study this two very close laser pulses are sent and the response is studied. flight-simulator : positron events are simulated using laser pulses that can also mimic the infamoussplash. Pulse Tagging : 1.8 GeV pulse that is found almost (in more than 50 crystals) in all crystals is definitely a laser. ODB: Laser pulse settings. DocDb10818-v3
  • 74. 21 September 2018 Atanu Nath 74 Temperature Correlations... 0.4% per o C 0.5% per o C 0.1% per o C OctavioEscalante OctavioEscalante OctavioEscalante