All Hands Meeting Status of Fermilab
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Transcript of All Hands Meeting Status of Fermilab
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All Hands MeetingStatus of Fermilab
Pier Oddone
September 9, 2009
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Pier Oddone, All hands meeting, September 9th, 20092
Outline
• Operational Highlights
IQA: Integrated Quality Assurance Engineering Standards: Manual and Teamcenter Health and Safety: H1N1, needed improvement
• The future program
The big picture A strategy for the US and Fermilab
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Quality
• We all have an intuitive understanding of a quality product: it does what it is supposed to do without trouble
• In scientific research quality means achieving correct, reproducible results, maximizing the information we get from data
• There are many processes to get there: administrative, operational, scientific. They all must be done with quality
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Quality Assurance
• All the processes that we put in place to make sure that we deliver quality in all our diverse activities
• We analyze what we do and make sure that we have the processes necessary to deliver expected results consistently and efficiently
• We already do a lot of it – but not in a consistent and systematic way and not in all our activities
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Integrated Quality Assurance
• Our program is called Integrated Quality Assurance or IQA – because it really must be a state of mind
• Do we need it? The consequences of faulty assurance processes
can be severe: many examples It is one of the foundations of continuous
improvement It is also a requirement of our contract to have a
quality assurance program that meets expectations: we must be smart on how we accomplish this
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IQA: Foundational Principle
• QA is integrated into our everyday work and is both a personal responsibility as well as a collective one. It is modeled after the successful Integrated Safety Management or ISM. What it is NOT: a layer of processes imposed externally.
• Implementation of IQA is a line management responsibility: line organizations have the authority, responsibility, and are accountable for integrating QA into all work
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IQA: Line Management Responsibility
• Office of Quality and Best Practices (OQBP) - Developed framework, provides oversight for
implementation, performs/coordinates independent assessments
Assist D/S/Cs in implementing IQA – training, assistance to QARs, data archival and trending
• AD’s, Heads of Programs, D/S/C Implement IQA in accord with principles &
requirements of IQA including continuous improvement
Perform self assessments to make sure performance objectives and requirements are met
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IQA: Standards
• The requirement is the implementation of the Quality Assurance Order DOE 414.1C
• The order allows a great lead of latitude in choosing a consensus standard: we chose ANSI/ASQ Z1.13, Quality Guidelines for Research
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NQA-1ANSI/ASQ
Z1.13X X
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How do we do this?
• We need a recognizable approach. We are audited on this requirement so auditors have to recognize how we assure quality
• Many of our existing processes were not cast in a standard framework and some processes are missing
• We help ourselves with: a) a standard framework that makes explicit our processes as part of IQA and b) we fill the gaps
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IQA: not free
• It is a considerable effort by the laboratory and an investment for the future
• We have four new QA Engineers (QAEs) under the guidance of the Office of Quality and Best Practices (OQBP) Provide support and guidance to D/S/Cs Train and support QARs Assist in development and review of Corrective
Action Plans Perform Independent Assessments
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QAEs
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Jed Heyes
QA Manager
Kurt Mohr, QAE Tom King, QAE Tom Gehrke, QAE
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Quality Assurance Representatives
12
Bakul Banerjee
CD
Frank Cesarano
BSS
Nicole Gee
WDRS
Tim Miller
ES&H
Jim Rife
TD
Don Rhode
AD
Kieth Schuh
PPD
Rod Walton
FESS
Jim Wollwert
FI
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Where are we?
• Completed to Date:
Establish team of QA professionals; QAEs and D/S/C QARs
QAR orientation & training, including Audit Training As-Is baseline – WELL DONE! Development of Corrective Action Plans to close
gaps discovered during As-Is baseline Reconciliation of all points from the DOE 2006 QA
audit (21 findings completed, 5 nearing completion)
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Where are we going?
• Next DOE audit starting September 14th, 2009 Build Assessment Plans, identifying gaps and
inadequacies Determine response using a graded approach to
ensure application of controls are “right-sized” for risks posed by Fermilab processes
Implement response and corrective actions Embed in the culture of the laboratory
http://www.fnal.gov/pub/quality/
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Engineering Manual
• Root-cause analysis of the LHC triplet failure led to task force on engineering practices
• Events at LHC have further highlighted the need for systematic approach: standard practices, risk based reviews and documentation
• With engineering in different Fermilab organizations, we must make special efforts to have common practices
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Engineering Manual
• Nine Major Elements are covered in the manual: Requirements and Specifications Engineering Risk Assessment Requirements and Specifications Review System Design Engineering Design Review Procurement and Implementation Testing and Validation Release to Operations Final Documentation
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Key feature of the manual
• Created by engineers from different parts of the laboratory under guidance of Paul Czarapata
• The main body is short – 33 pages – to allow easy reading
• Useful examples are shown in the Appendix
• It is a LIVING document: controlled copy on the web
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Key feature of the manual
• Defines roles and responsibilities through the engineering process
• Defines requirements for risk analysis and level of formality based on risk
• Puts requirements on documentation on all phases of engineering process
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Teamcenter
• We are investing on Teamcenter license to use a modern EDMS system for engineering documentation
• Teamcenter will be used to Capture all elements of the approved Fermilab
engineering process and documents Connect and control engineering specifications,
design analysis, CAD drawings, safety documentation, and QC reports in a central repository
Allow more efficient data sharing across organizations
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Teamcenter and engineering
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EH&S
• H1N1 Pandemic
Get a seasonal flu shot (available early October)
Practice good hand hygiene and cough etiquette
Stay home if you are sick - call medical (x3232) if you suspect you have the flu and stay home for 24 hours after you are fever free with no medication
Use our website for current information: http://www.fnal.gov/pub/fluquestions/
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EH&S
• Fermilab Director’s Triennial Self-Assessment of ES&H – recommendations:
Educate supervisors in Human Performance Improvement
Standardize a Reward & Recognition program for ES&H
Document ES&H performance on performance reviews
Communicate the importance of SMART (Specific, Measurable,Attainable, Relevant, and Time-bound) goals for Fermilab personnel ES&H goals.
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Injuries are a matter of concern
0.0
0.5
1.0
1.5
2.0
2.5
3.0
3.5
4.0
4.5
5.0
DART Case Rate by Calendar Quarter(Error Bars are One Standard Deviation)
Fall 2002
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CYQ
CY97.2
CY97.4
CY98.2
CY98.4
CY99.2
CY99.4
CY00.2
CY00.4
CY01.2
CY01.4
CY02.2
CY02.4
CY03.2
CY03.4
CY04.2
CY04.4
CY05.2
CY05.4
CY06.2
CY06.4
CY07.2
CY07.4
CY08.2
CY08.4
CY09.2
0.0
1.0
2.0
3.0
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5.0
6.0
7.0
8.0
9.0
TRC Case Rate by Calendar Quarter(Error Bars are One Standard Deviation)
Fall 2002
Injuries are a matter of concern
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The big picture
• The laboratory is doing very well: many results from the Tevatron, leading programs in neutrinos and particle astrophysics. Fermilab provided most results at Lepton-Photon 2009
• The shutdown has gone well and we are ready for a two year run with great discovery potential pending DOE support in FY11
• Base budget is in reasonably good shape and we have received nearly $150M ARRA funds
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The big picture
• The strategy for the future has broad support: it is a challenging and exciting program
• • Several briefings to the Director of the Office
of Science, Bill Brinkman: laboratory planning, neutrinos, Project X. Also visit to the laboratory by Bill Brinkman and Pat Dehmer
• The program places strong demands on us to manage well and efficiently and work closely with our partner institutions
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Facilities and experiments
Pier Oddone, All hands meeting, September 9th, 200927
Tevatron
LHCLHC
LHC upgrades
Minos
MiniBooNENOvA
MicroBooNE
MINERvA
LHC
ILC or
Muon Collider
Now 2015
LHC
ILC??
LBNE
Mu2e
Project X+LBNE
Mu2e
n Factory
2012 2018
P Auger
DM Searches
P Auger
DM: scalable?
DESJDEM
DM searchesJDEM
Ene
rgy
Inte
nsity
Cos
mic
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Energy Frontier: Tevatron
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10/1/2
003
4/1/20
04
10/1/2
004
4/2/20
05
10/2/2
005
4/3/20
06
10/3/2
006
4/4/20
07
10/4/2
007
4/4/20
08
10/4/2
008
4/5/20
09
10/5/2
009
4/6/20
10
10/6/2
010
4/7/20
11
10/7/2
0110
1
2
3
4
5
6
7
8
9
10
11
12
13
Green curve: same rates as 09
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Lepton colliders beyond LHC
LHC Results
ILC Enough
ILC not enough
CLIC
Muon collider
or
or
By far the easiest!
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HEP world: need TeV lepton collider
e- e+
p p
ILC
LHC
International
Linear
Collider (ILC)
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Pier Oddone, All hands meeting, September 9th, 2009
ILC/Project X technology at Fermilab
Vertical Test Stand
Horizontal Test Stand
1st cryomodule
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Muon collider layout
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4 TeV
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Muon collider functional layout
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Target Capture Cool Format Accel Collide
Color indicates degree of needed
R&D (difficulty) and demonstration
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Muon collider/ILC/Project X
• ILC and Project X developing very efficient accelerating structures that can be run economically
• Muon collider requires substantial acceleration (few km) that ideally would use ILC/ Project X technology
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Facilities and experiments
Pier Oddone, All hands meeting, September 9th, 200937
Tevatron
LHCLHC
LHC upgrades
Minos
MiniBooNENOvA
MicroBooNE
MINERvA
LHC
ILC or
Muon Collider
Now 2015
LHC
ILC??
LBNE
Mu2e
Project X+LBNE
Mu2e
n Factory
2012 2018
P Auger
DM Searches
P Auger
DM: scalable?
DESJDEM
DM searchesJDEM
Ene
rgy
Inte
nsity
Cos
mic
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Two avenues to real understanding !
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Intensity frontier:
the most particlesAllows the study of neutrinos and rare process
Sensitive to physics far beyond the LHC, but only indirectly
Need to measure multiple processes
LHC: direct production
of heavy particles
Wonderful direct discoveries of physics beyond the Standard Model
Very difficult and often impossible to study how new particles couple to each other and to ordinary particles
Need both for a complete understanding
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Interplay: LHC Intensity Frontier
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LHC
nothing
Lots
Intensity
Frontier
Only handle on the
next energy scale
Determine/verify
structure of new
physics. Anything
beyond?
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Progress: neutrinos
Minos Far Detector
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• NOvA is optimized for the detection of νμ→νe and νμ→νe
oscillations
• NOvA is:
An upgrade of the NuMI beam intensity from 400 kW to 700 kW
A 14 kt “totally active” tracking liquid scintillator calorimeter sited 14 mrad off the NuMI beam axis at a distance of 810 km
A 215 ton near detector identical to the far detector sited 14 mrad off the NuMI beam axis at a distance of 1 km
2.5 GeV νe + p →1.9 GeV e- + 1.1 GeV p + 0.2 GeV π+
20 cm
20 c
m
MIPs
MIPs
NOvA
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Progress: NOvA groundbreaking
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The NOvA Collaborationat Argonne National Lab, 25 April 2009
180 Scientists and Engineers from 26 InstitutionsArgonne National Laboratory - University of Athens - California Institute of Technology - University of California, Los Angeles - Fermi National Accelerator
Laboratory - Harvard University - Indiana University - Lebedev Physical Institute - Michigan State University - University of Minnesota, Duluth - University of Minnesota, Minneapolis - The Institute for Nuclear Research, Moscow - Technische Universität München, Munich - State University of New York, Stony Brook - Northwestern University - University of South Carolina, Columbia - Southern Methodist University - Stanford University - University of Tennessee - Texas A&M University - University of Texas, Austin - University of Texas, Dallas - Tufts University - University of Virginia, Charlottesville - The College of William and Mary -
Wichita State University
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MINERvA Sees!
Prototype took data Apr.15 ~Jun.15
15k events, publishable physics
Data taking with 50% det: Oct.2009
Full det.: Summer.2010
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p?
m
p0
p
e
p
m
nmn→m-p nen→e-p nmn→m-p0X
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First ArgoNeut LAr TPC events
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L = 1290 km
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Intensity frontier: DUSEL
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m to e Conversion (mN eN)
MECO spectrometer design
for every incident proton 0.0025 m-’s are stopped in
the 17 0.2 mm Al target foils
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Evolution of the Project X concept
• Originally an 8 GeV pulsed linac (5Hz, 1 msec pulses) with accumulation in the Recycler storage ring and acceleration to high energy in the Main Injector
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Original
Idea
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Evolution of Project X
• Work on Project X has led to a much better idea for a unique and flexible facility
• Instead of an 8 GeV pulsed linac (1 msec pulses at 5 Hz) use a CW linac (continuous pulses at 325 MHz) delivering 2 MW at 2 GeV of either protons or H- ions
• These pulses can be directed flexibly to different experiments with different time patterns and pulse intensities
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Project X and LBNE to Homestake
• 5% of the time line, the 2 GeV linac feeds a simple Rapid Cycling Synchrotron (RCS), 500m circumference, to strip, accumulate and boost the energy to 8 GeV
• Six pulses of the SAB are transferred to the recycler, filling the existing recycler, and every 1.4 sec transferred to the Main Injector for acceleration to high energies (60 GeV to 120 GeV)
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Project X and 8 GeV beams
• 8/14 RCS cycles are available for an 8 GeV program driven by a fast spill (single turn). An example is a much upgraded muon g-2
• Slow extraction as needed for rare processes is very limited from circular machines: only method is resonance extraction which is “rad dirty” and limits extraction to 10s of kW.
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Project X and 2 GeV beams
• The greatest potential for rare processes comes from 2 MW continuous beam. Intensity experiments need continuous beam: pile up is the main limitation in pulsed beams
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Facilities and experiments
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Tevatron
LHCLHC
LHC upgrades
Minos
MiniBooNENOvA
MicroBooNE
MINERvA
LHC
ILC or
Muon Collider
Now 2015
LHC
ILC??
LBNE
Mu2e
Project X+LBNE
Mu2e
n Factory
2012 2018
P Auger
DM Searches
P Auger
DM: scalable?
DESJDEM
DM searchesJDEM
Ene
rgy
Inte
nsity
Cos
mic
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Pier Oddone, All hands meeting, September 9th, 20095555
COUPPRoom temp. CF3I Bubble Chamber
CDMSLow temp. Ge / Si crystals
COUPP
60 kg / 30 liter
2 kg / 1 liter4 kg 15 kg
Underground dark matter detectors
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Probing Dark Energy
Pier Oddone, All hands meeting, September 9th, 20095656
SDSS
DES
JDEM¼ scale model DECAM
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Pier Oddone, All hands meeting, September 9th, 200957
UHE Cosmic Frontier: Pierre Auger
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Cosmic frontier: new ideas
• One ton detector scale dark matter searches
• Pierre Auger North
• 21 cm radio band survey (dark matter distribution)
• Holographic noise
• Axion searches
Pier Oddone, All hands meeting, September 9th, 200958
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A formidable program ahead
• Very demanding of ourselves at all levels
• Must leverage our efforts by involving the national and international community in developing the program
• Must have the underlying management and information systems that make us effective at delivering such a program
Pier Oddone, All hands meeting, September 9th, 200959