The Cosmic Ray Observatory Project (CROP): An outreach and education experiment in Nebraska
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Transcript of The Cosmic Ray Observatory Project (CROP): An outreach and education experiment in Nebraska
The Cosmic Ray Observatory Project (CROP): An outreach and education experiment in Nebraska
Funded by a $1,342,000 grant from the National Science FoundationTeacher Enhancement Program and High Energy Physics
A high school based Pierre Auger Observatory
State of Nebraska
Pierre Auger northern hemisphere
site in Utah
Where isNebraska?
FermilabBatavia, Illinois
CROP Project Goals
EducationalPrepare teams of high school teachers and students to get involved in studies of extended cosmic ray showers using modern research techniques.
• 4-week summer intensive training program at UNL• Biweekly phone conferences or chat rooms• Two 1-day meetings every year• Web-based help pages
ScientificBuild a statewide network of cosmic ray detectors.
• Retired CASA detectors in weather-proof enclosures on roof• GPS receiver gives local time stamp for shower arrival• PC inside school takes data through a DAQ card at each site• Student teams share data over Internet searching for time coincidences
Search for the sources of ultra-high energy cosmic rays.
CROP Personnel at UNL, 2003
CROP staff at University of Nebraska• Faculty: Dan Claes and Greg Snow• Educational evaluator: Dr. Duane Shell• Physics graduate student: Aidyl Galafa
• September 2002, Computer Science graduate students:
Steve Becker: Programming of DAQ card
Jared Kite: LabView control screen for DAQ card
Cory Strope: Computer simulations of cosmic ray air showers
• January 2003 Secondary science ed graduate student: Tracie Evans
• Undergraduate research assistants: M. Dennsberger, M. Everett, A. Fuchser, P. Jacobson, A. Kubik, D. Larsen, S. Mahoney• Administrative Secretary: Marilyn McDowell• Lab manager: High school teacher, John Rogers
Summer 2003
CROP article in Lincoln Journal Star, 7 August 2003
CROP schools enlisted in 2000 2001 2002 2003
250 miles
450 miles
The Cosmic Ray Observatory ProjectA grid of cosmic ray research stations
expanding across the state
Coleridge
McPherson
MullenLoup
Spalding
High school teams attend a 4-week summerworkshop at UNL with class and lab activities
2000: Lincoln Zoo, Lincoln Northeast, Mt. Michael,Marian, Norfolk
2001: Lincoln Lutheran, Lincoln High, Omaha Westside,Anselmo-Merna, Osceola, Wayne State College
… and new schoolswill be
enlisted in CROP
each year
2002: Fairbury, Wayne, Roncalli Catholic,Bancroft-Rosalie, Waterloo
2003: Coleridge, Loup, McPherson, Mullen, Spalding,
The Chicago Air Shower ArrayThe Chicago Air Shower Array
• CROP uses retired detectors from the Chicago Air Shower Array• 1089 boxes each with:
• 4 scintillators and photomultiplier tubes (PMT)• 1 high voltage and 1 low voltage power supply
• Two removal trips (September 1999, May 2001) yielded over 2000 scintillator panels, 2000 PMTs, 500 low and power supplies• Sufficient hardware for all Nebraska high schools
U.S. Army PhotoSeptember 30,
1999
The CROP team at Chicago Air Shower Array (CASA) site
Equipment recovery trip to Dugway, Utah, May 2001
The Science of CROP
• Each school records building-sized showers -- plenty of rate.• 2500 ft2 shower (1014 eV )
• Neighboring schools in same city (Lincoln, Omaha) see coincidences from highest-energy showers -- low rate.
• 10 sq.mi shower ~1019 eV• 50 sq.mi shower ~1020 eV
• Nebraska is 450 x 250 square miles -- schools separated by very large distances explore whether showers come in large, correlated bursts
That is, does the whole state of Nebraska ever light up?
The Cosmic Ray Energy Spectrum
(1 particle per m2 per sec)
(1 particle per m2 per year)
(1 particle per km2 per year)
Cosmic Ray Flux
Energy (eV)
Building-sizedshowers
City-sizedshowers
The Science Reachof CROP
250 miles
450 miles
CROP can also search for coincidencesover large distances
Does the whole state ever light up at once?
Size of Pierre Auger site, 1600 detectors
Possible Source of Coincident,Widely-Separated Showers
The GZ Effect (Gerasimova-Zatsepin)
Cosmic ray iron nucleus
Optical photon from the sun
Earth’s Surface
Nuclear fragments from photo-disintegration
• Watson and Medina-Tanco revisit this 1960-predicted phenomenon in astro-ph/9808033
• Calculation for 6 × 1017 eV Fe Mn + proton
• Shower separations of 100’s to 1000’s of kilometers possible, dominated by deflections by interplanetary magnetic fields
• Rates not encouraging
Lab Curriculum• Polishing, cleaning scintillator• Gluing PMT and wrapping scintillator• Assembling high-voltage supply• Oscilloscope lesson• Turning on counters, source tests, finding/fixing light leaks• Measure counter efficiency, high voltage plateau
Class Curriculum• History of cosmic rays• Interaction of charged particles with matter• Scintillators and photomultiplier tubes• Cosmic ray energy spectrum• Julian calendar, UTM, galactic coordinates• Global positioning system• Ionizing particle detectors• Calorimeters and showering• Particle zoo and the Standard Model• Tour of high-energy particle accelerators• Random events, probability• Monte Carlo simulations• Lightning protection
Curriculum Topics
Available
What we expectto accomplish
in 4 weeks
Preparingdetectors totake to your
schools,experimentaltechniques
Learningthe physicsof cosmicrays andparticle
detectors
Photomultiplier Tubes
Schematic drawing of a photomultiplier tube
Photons eject electrons via photoelectric effect
Photocathode
Each incidentelectron ejectsabout 4 newelectrons at eachdynode stage
Vacuum inside tube
“Multiplied” signalcomes out here
An applied voltagedifference betweendynodes makeselectrons acceleratefrom stage to stage
Incident light from scintillator
CROP teachers and students gain valuablehands-on experience in bona fide research
Student team at Lincoln’sZoo School with their detectors
Marian High School’s measurementof cosmic ray rate vs. barometric
pressureStudents present results in
conference-style meetings at UNL
Students refurbish and assemble their own
detectors before installing them at school
Participants learn oscilloscope useand build electronics
Increasing barometric pressure
Nu
mb
er
of
cosm
ic r
ays d
ete
cte
d
Endless scraping, polishing, and soldering
Endless wrapping, taping, and observing
Endless cabling and adjusting
Pre-workshop and Post-workshop testing
Positive outcomes-assessment results from professional evaluator
Detectors in a vertical“telescope”
Mini-experiments
• Coincidence rate vs. barometric pressure• Day-night variation of cosmic ray rate• Coincidence rate vs. angle of incidence• Coincidence rate vs. vertical separation
Electronics Configuration for Telescope
Detector set-ups at schools
“Telescope” set-ups forindoor experiments
Barometric Pressure (mmHg)727 747
4-F
old
Coi
ncid
ence
s / 2
hou
rs
3000
4200
• Statistical error bars shown• 1.3% decrease per mmHg
Marian High School’s Measurementof Cosmic Ray Rate vs. Barometric Pressure
Mount Michael High School “The Science Teacher”, November 2001
5 VoltDC power
To PCserial port
Four analogPMT inputs
Discriminatorthreshold
adjust
GPS receiverinput
Eventcounter
Programmablelogic device
Time-to-digitalconverters
CROP data acquisition electronics card
Developed by Univ. Nebraska, Fermilab (Quarknet), Univ. Washington
• 43 Mhz (24 nsec) clock interpolates between 1 pps GPS ticks for trigger time• TDC’s give relative times of 4 inputs with 75 psec resolution
User-friendly, LabView-based control and monitoring GUI
Two detectorsfiring at thesame time
Data streamfor eachevent
Eventcounter
Elapsedrun
time
Students familiarizing themselves with data-acquisition card and PC
Students familiarizing themselves with data-acquisition card and PC
Rooftop mini-experiments for CROP Schools
1
11
3
2
2 2
3 3
With counters spread out in horizontal plane• 2/4, 3/4, 4/4 coincidence rates vs. detector separation• Different configurations (square, triangle as shown)• Optimization of counter geometry on school rooftop• Singles rates vs. rainfall• Simultaneous data taking with other schools
Coincidence Rates vs. Separation ExperimentOctober – December 2002
Installation on Physics Department roof, February 2002
4 detectors on corners of a square
15 meter(45 feet)
separation shown
15 m15 m
15 m
4-fold Coincidence Ratesvs. Separation
4fold/hour vs Tstart
0
5
10
15
20
25
30
35
40
45
50
4 14 24 34 44 54 64 74 84 94
Day in October
4fo
ld/h
ou
r
4fold/DelT
4fold/DelT, 15 feet
4fold/DelT, 15 feet, 1 lead sheet
4fold/DelT, 15 feet, 2 lead sheets
4fold/DelT, 30 feet
4fold/DelT, 45 feet
Days since October 1, 2002
4-fo
ld c
ount
s/ h
our
Touching
15 ft
15 ft, 1 lead
15 ft, 2 lead
30 ft
45 ft
Rates high enough to sustain student interest
Lincoln High School rooftop
Presently taking data simultaneously at 3 sites
• 21 schools received data-acquisition cards at September 27 meeting at UNL
• All schools start taking data this semester
CROP
Pierre Auger northern hemisphere site in Utah
SCRODSALTA
CHICOS
WALTA ALTA
NALTAThe North American Large-Scale Time-Coincidence
Array
http://csr.phys.ualberta.ca/nalta/• Includes links to individual project Web pages
Colorado• Aspen High School, Aspen, CO
• Basalt High School, Basalt, CO
• Roaring Fork Valley High School, Carbondale, CO
• Lake County High School, Leadville, CO The highest-elevation school in the U.S. -- 10,152 feet ASL Illinois• Wheaton North High School, Wheaton, IL
SALTA: Snowmass Area Large Time-Coincidence Array
Initiated during Snowmass 2001Future of HEP Conference
Replica of Replica of Hess’ ElectroscopeHess’ Electroscope
Portable GeigerPortable GeigerCounters Counters
Wilkes inWilkes inHessianHessianOutfitOutfit
Lift off !
Data transmitted liveto ground via radio
Crowd gathersto watch
Victor Hessflight reenactment
Unicorn Balloon Company, Snowmass, CO
Snowmass Balloon Flight 2001
65
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110
70008000
900010000
11000
12000
13000
Altitude (feet)
Co
un
ts/m
inu
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July 7 flight
July 8 flight
Ground level at Snowmass
• Two flights with consistent results
• Hovered at 1000 ft increments in altitude for 5 minutes
• Cosmic ray rates measured with portable Geiger counters
• Same effects observed by Victor Hess
• See FermiNews, July 27, 2001
The Washington-Area Large-ScaleTime-Coincidence Array
http://www.phys.washington.edu/~waltahttp://www.phys.washington.edu/~walta
Seattle area map showing schools
• CROP’s closest relative• Run by University of Washington, Seattle Jeff Wilkes, et al.• WALTA also uses refurbished CASA detectors
Institutions• LA area schools• California Institute of Technology• California State University, Northridge• University of California, Irvine
Funding• Caltech• NSF Nuclear Physics
Los Angeles Area Schools
(Animation by L.A. school teacher)
• 164 detector stations recovered
• 2 detectors per school foreseen
• About 39 schools in process of being outfitted
Conclusions on CROP
* CROP, in its 4th year, will soon reach a major milestone: Simultaneous data-taking at all schools, offline searches for extensive air shower coincidences
* Other emerging efforts will enable the NALTA consortium to search for very long-range correlations
* Curriculum, hardware, software has been developed to facilitate the start-up of new efforts
• Nationwide program which links high energy physicists with teams of local high school physics teachers to engage in active research projects
• Funded by the U.S. National Science Foundation and Department of Energy, project office at Fermilab
• In its 5th year, QuarkNet centers established in 29 states involving over 400 teachers and their students
QuarkNet continues to grow in the U.S.http://quarknet.fnal.gov
• Wide range of ongoing activities, examples:• Hardware: CMS hadron calorimeter optical decoder units, PMT testing and database• Analysis: Using distilled Tevatron data, Z mass peak reconstruction, top quark decay kinematics
• Growing emphasis on local cosmic ray studies with various techniques: scintillators, Geiger counters, proportional tubes
• Ongoing work to disseminate activities developed at a given site to all QuarkNet participants
U.S. QuarkNet sites
Some QuarkNet Activities
CMS phototube test setup (Univ. Iowa)
Counting cosmic ray muons on top of SearsTower in Chicago (Univ. Illinois, Chicago)
Extensive air shower array at University of Washington
CROP, QuarkNet, and many other U.S. Education/Outreach programs are summarized in the booklet
“Particle Physics Education and Outreach 2001”
Available at http://www-ed.fnal.gov/hep/home.html
Education/Outreach Committee of the American Physical Society’sDivision of Particles and Fields (formed 2003)
Members: Liz Simmons (chair), Michael Barnett, Marcela Carena,Judy Jackson, Harrison Prosper, Randy Ruchti, Jim Siegrist, Greg Snow
Activities:• Feed info on EPO efforts to Interactions.org web site
coordinated by all HEP labs worldwide
• Advocate for EPO plenary talks at future DPF meetings to educate wider community and get more people involved
• Coordinate widely dispersed EPO efforts of each HEP experiment to establish communication, avoid duplication of materials and activities development
• Provide guidance and “best practices” to investigators writing the now-required EPO part of their NSF and DoE base funding proposals
• Contribute to planning of U.S. activities in 2005 World Year of Physics
World Year of Physics 2005in the United States
“Einstein in the 21st Century”
• Planned Projects
• Poster Contest • Interactive Website
• PhysicsQuest • Public Lectures
• Physics on the Road • APS Meeting Events
• Distributed Computing Project
Planned Projects: Poster Contest
• Nationwide poster contest aimed at U.S. 5th graders (generally aged 10). There are ~4,000,000 U.S. students.
• Theme: “Einstein in Everyday Life” contest instructions will be accompanied by lessons and activities that fit in with national science and history guidelines for U.S. 5th graders.
• Winning poster nationwide will be made into a promotional poster for WYP2005; distributed to U.S. schools.
Planned Projects: PhysicsQuest
• Fictional physics “mystery” aimed at U.S. middle school students (generally aged 11-13). There are ~12,000,000 such students.
• Students will receive an “evidence kit” they will use to solve the mystery.
• “Clues” will be available online.
• Involves students in the process of using science to solve problems.
Planned Projects: Physics on the Road
• “Branding” existing traveling programs usually run by university/college physics department personnel (approximately 25 programs).
• Some are demonstration based, others are “hands-on” experiments that travel to primary and secondary schools exposing the students to physics.
• Developing one or two 2005-related physics demos to be used by all POTR teams.
Planned Projects: Interactive Websitehttp://www.physics2005.org
• Website will include:
• Searchable database of Nationwide events
• Kits on how to plan your own 2005 event
• Puzzles and activities for teachers and students
• Contest information (Poster contest, PhysicsQuest and others)
• Einstein History in collaboration with AIP’s Center for the History of Physics
Planned Projects: Public Lectures
• We will encourage physics departments across the country to host public lectures focusing on physics.
• Our Topical Group on Gravitation can help us create a Speakers List for physics departments to use.
Planned Projects: APS Meeting Events
• The American Physical Society has ~ 20 national, topical and regional meetings annually.
• We plan to have special exhibits/displays at many of the APS meetings.
• Larger meetings could have special “Physics Expositions” designed especially for the public.
Planned Projects:Distributed Computing Project
• A grass-roots, distributed computing search that would be similar to SETI@home screen-saver, which utilizes CPU time of idle computers to analyze radio antennae data for signs of extra-terrestrial life. In this project, participants would aid in the search for gravitational wave signals in data collected by the LIGO Observatory.
Collaborations
Although the American Physical Society is spearheading the U.S. efforts to celebrate the World Year of Physics, it is collaborating with many other organizations.
• American Association of Physics Teachers
• American Institute of Physics
• Society of Physics Students
• National Science Foundation
• U.S. Department of Energy
• NASA
• U.S. Science Museums
Vinaya K. Sathyasheelappa
U.S. WYP2005 Project Coordinator
(301) 209-3217