Small, fast, low-pressure gas detector E. Norbeck, J. E. Olson, and Y. Onel University of Iowa For DNP04 at Chicago October 2004.

Slides:



Advertisements
Similar presentations
Chapter 4 Radiation Dosimeters
Advertisements

General Characteristics of Gas Detectors
Radiation Detection ionization chambers (dosimeters, pulse chambers, particle track chambers) scintillation detectors semiconductor detectors photographic.
Gamma-Ray Spectra _ + The photomultiplier records the (UV) light emitted during electronic recombination in the scintillator. Therefore, the spectrum collected.
GM COUNTER.
Black body radiation BBR is the radiation emitted by a non-reflecting solid body. A perfect black body is one which absorbs all the radiations falling.
6. Atomic and Nuclear Physics Chapter 6.4 Interactions of matter with energy.
Magnetic Field Patterns
Radiation Detectors / Particle Detectors
Quartz Plate Calorimeter Prototype Ugur Akgun The University of Iowa APS April 2006 Meeting Dallas, Texas.
1 Methods of Experimental Particle Physics Alexei Safonov Lecture #12.
Atomic Absorption Spectroscopy Prof Dr Hisham E Abdellatef 2011.
History of Particle Detectors
Aging, High Rate and Shielding L. Lopes Lip-Coimbra.
M. Palm, CERN1 Performance test of ACEM-detector (Aluminum Cathode Electron Multiplier) Marcus Palm AB-ATB-EA.
CMS Calorimetry in the Very Forward Direction E. Norbeck, P. Debbins, and Y. Onel University of Iowa For the 23 rd Winter Workshop on Nuclear Dynamics.
Directional Detectors and Digital Calorimeters Ed Norbeck and Yasar Onel University of Iowa For the 25 th Winter Workshop on Nuclear Dynamics Big Sky,
Detectors. Measuring Ions  A beam of charged particles will ionize gas. Particle energy E Chamber area A  An applied field will cause ions and electrons.
Scintillators.
Main detector types Scintillation Detector Spectrum.
Far forward angle physics at the LHC E. Norbeck and Y. Onel University of Iowa For the 24th Winter Workshop on Nuclear Dynamics South Padre Island
Radiation Sensors Zachariadou K. | TEI of Piraeus.
Photomultiplier Tube. What is it? Extremely sensitive detector of light in the ultraviolet, visible and near infrared Multiplies the signal produced by.
Lecture 11  Production of Positron Emitters, Continued  The Positron Tomograph.
E. Norbeck U. IowaFast Gas Detector APR 05 Tampa1 Small Fast Gas Detector for High-Energy Electrons E. Norbeck, J.E. Olson, and Y. Onel University of Iowa.
1 Alpha Emissions (How a Smoke Alarm Works). 2 Radioactive Emissions (Radiation) Penetrating Power SymbolEquivalentDescriptionType He Stopped by thick.
Rad Hard Active Media for Calorimeters E. Norbeck, J.E. Olson, A. Moeller, and Y. Onel University of Iowa PPAC Čerenkov Liquid with Tungsten metal.
Energy Resolution of a Parallel- Plate-Avalanche-Chamber Kausteya Roy Professors E. Norbeck and Y. Onel.
1 Semiconductor Detectors  It may be that when this class is taught 10 years on, we may only study semiconductor detectors  In general, silicon provides.
1 Scintillators  One of the most widely used particle detection techniques Ionization -> Excitation -> Photons -> Electronic conversion -> Amplification.
HABIS X-RAY PRODUCTION AND EXPOSURE FACTORS X-RAY PRODUCTION AND EXPOSURE FACTORS PREPARED BY PREPARED BY Dr fahad albadr radiology chairman radiology.
Jackson Choate.  High-energy electrons and photons lose energy primarily through Bremsstrahlung and pair production, respectively.  Bremsstrahlung.
TRIGGERING EXCIMER LASERS BY PHOTOIONIZATION FROM A CORONA DISCHARGE* Zhongmin Xiong and Mark J. Kushner University of Michigan Ann Arbor, MI USA.
C.Shalem et al, IEEE 2004, Rome, October 18 R. Chechik et al. ________________RICH2004_____________ Playa del Carmen, Mexico 1 Thick GEM-like multipliers:
Status of PNPI R&D for choice of the MUCH tracking base detector (this work is supported by INTAS) ■ Introduction ■ MICROMEGAS ■ GEM ■ MICROMEGAS+GEM ■
Tools for Nuclear & Particle Physics Experimental Background.
Muon Detector Jiawen ZHANG Introduction The Detector Choices Simulation The structure and detector design The Expected performance Schedule.
GEM: A new concept for electron amplification in gas detectors Contents 1.Introduction 2.Two-step amplification: MWPC combined with GEM 3.Measurement of.
C. Fischer – LHC Instrumentation Review – 19-20/11/2001 Gas Monitors for Transverse Distribution Studies in the LHC LHC Instrumentation Review Workshop.
Study of UV absorption and photoelectron emission in RPC (Resistive Plate Counters) detector with an UV source Carlo Gustavino (INFN-LNGS) RPC and their.
Ionization Detectors Basic operation
Scintillation Detectors
Techniques for Nuclear and Particle Physics Experiments By W.R. Leo Chapter Eight:
CALICE 03/14/05Ed Norbeck U. of Iowa1 PPACs in a Calorimeter Edwin Norbeck University of Iowa.
26 Apr 2009Paul Dauncey1 Digital ECAL: Lecture 3 Paul Dauncey, Imperial College London.
Ion signals with R134a and R134 in a parallel plate proportional counter Edwin Norbeck, J. E. Olson, Y. Onel University of Iowa For Sec. DH-3 of DNP06.
Quartz Plates R&D Status By F. Duru, S. Ayan, U. Akgun, J. Olson, Y. Onel The University Of Iowa V.Podrasky, C. Sanzeni, D.R.Winn Fairfield University.
December 10, The Parallel Plate Chamber CERN Presentation Wout Kremers Detector R&D NIKHEF.
Ion signals with R134a and R134 in a parallel plate proportional counter Y. Onel, E. Norbeck, J. E. Olson University of Iowa For HCAL meeting at Fermilab.
Chem. 133 – 2/11 Lecture. Announcements Lab today –Will cover 4 (of 8) set 2 labs (remainder covered on Tuesday) –Period 1 will extend one day Website/Homework.
PPAC in ZDC for Trigger and Luminosity Edwin Norbeck University of Iowa Luminosity Workshop November 5, 2004.
Quartz Plate Calorimeter Prototype Hardware & Preliminary Test Beam Data Anthony Moeller The University of Iowa.
Gas detectors in a ZDC (at LHC) Edwin Norbeck and Yasar Onel University of Iowa For7 th CMS Heavy-Ion meeting at Delphi June 2003.
Development of a Single Ion Detector for Radiation Track Structure Studies F. Vasi, M. Casiraghi, R. Schulte, V. Bashkirov.
W Prototype Simulations Linear Collider Physics & Detector Meeting December 15, 2009 Christian Grefe CERN, Bonn University.
PPAC Jonathan Olson University of Iowa Thesis Defense 8 April 2005.
PPAC Parallel Plate Avalanche Counter Edwin Norbeck University of Iowa For meeting at SLAC June 2, 2004.
PPAC Jonathan Olson University of Iowa HCAL November 11-13, 2004.
PreShower Characterisations
Ionizing Radiation
Ultra fast SF57 based SAC M. Raggi Sapienza Università di Roma
Plan for prototype production and test
Dr: Mohamed Afifi By Lecturer Radiological Science
Radiation Detectors : Detection actually means measurement of the radiation with its energy content and other related properties. The detection system.
Chem. 133 – 2/9 Lecture.
Ionization detectors ∆
Motion of charged particles in an electric field
Performance test of ACEM-detector (Aluminum Cathode Electron Multiplier) Marcus Palm AB-ATB-EA M. Palm, CERN.
Semiconductor Detectors
Presentation transcript:

Small, fast, low-pressure gas detector E. Norbeck, J. E. Olson, and Y. Onel University of Iowa For DNP04 at Chicago October 2004

E. Norbeck U. IowaDNP04 BB.014 Gas Detector2 Typical low-pressure PPAC Two flat plates Separated by1-3 mm Filled with torr isobutane V between plates (Parallel Plate Avalanche Counter)

E. Norbeck U. IowaDNP04 BB.014 Gas Detector3 Small PPAC for showers from high-energy ( GeV) electrons The original object of this study was to determine the suitability of a PPAC as an inexpensive, very fast, rad-hard pixel detector to use in a calorimeter for electrons. Our measurements have broader application.

E. Norbeck U. IowaDNP04 BB.014 Gas Detector4 Single Pixel PPAC For Test With High- Energy Electrons Gap 1.0 mm Cathode 7X 0 = 29 mm of tantalum Area of anode is 1.0 cm 2 Guard ring to simulate neighboring pixels Gas is isobutane at 10 to 100 torr

E. Norbeck U. IowaDNP04 BB.014 Gas Detector5 Detail of 1 mm gap and guard ring

E. Norbeck U. IowaDNP04 BB.014 Gas Detector6 A MIP will usually leave no ionization in the low pressure gas. With a high-energy electron shower there are 100s or 1000s of electrons contributing to the signal. To date we have not yet put a high-energy electron into the detector. Our measurements have all been with Compton electrons from a 137 Cs gamma source. With the source to the side of the PPAC, a few of the electrons travel parallel to the face of the plates and produce a usable amount of ionization in the gas.

E. Norbeck U. IowaDNP04 BB.014 Gas Detector7 1.8 ns 50 torr 790 V 7 mv into 50  Electron signal Single peak with considerable noise. The noise is large because of the small size of the signal using our 137 Cs source. With the much larger signals from high-energy electrons, the noise will be negligible.

E. Norbeck U. IowaDNP04 BB.014 Gas Detector8 For high speed, the RC time constant must be kept small. Only PPACs of small area are fast ~1 ns R = 50 Ω (coax cable). C is the capacity between the plates C =.885 pF for 1 mm gap and area of 1 cm 2 For our larger PPAC with C = 168 pF rise time ~5 ns fall time ~7 ns Fast enough for a Zero Degree Calorimeter at the LHC where minimum beam crossing time is 25 ns.

E. Norbeck U. IowaDNP04 BB.014 Gas Detector9 Ion collection time.3  s 0.5  s 50 torr 790 V

E. Norbeck U. IowaDNP04 BB.014 Gas Detector10 Signal out Guard ring Reflections are a problem with such fast signals. Should be 50 Ω all the way to the anode. View with covers removed

E. Norbeck U. IowaDNP04 BB.014 Gas Detector11 At isobutane pressures less than 30 torr afterpulses sometimes occur during the first 20 ns. This is a worst case example. Total charge from the afterpulses can be much larger than primary signal. 10 torr 500 V

E. Norbeck U. IowaDNP04 BB.014 Gas Detector12 The afterpulses seen here are usually hidden inside of signals that are more than 20 ns wide. This may be the cause of the typically bad energy resolution of PPACs operated in the 5 to 20 torr range. What causes the afterpulses? They are most likely caused by UV photons producing photoelectrons at the cathode. These electrons then initiate a new avalanche. Changing the anode from stainless steel to graphite had no effect on the afterpulses. This shows that the photons do not come from the anode.

E. Norbeck U. IowaDNP04 BB.014 Gas Detector13 Perhaps the excited molecules emit photons with a lifetime long compared with 20 ns, with molecular collisions limiting the lifetime of the excitations. Collision time in isobutane gas is too long to account for the data. Isobutane speed 350 m/s Fragments are faster Ion speed > 2000 m/s (1 mm in 500 ns) Note also that electrons acquire a larger energy between collisions at the lower gas pressures. 500 V at 10 torr but 1000V at 80 torr

E. Norbeck U. IowaDNP04 BB.014 Gas Detector14 Ion current from same event Afterpulses are real avalanches

E. Norbeck U. IowaDNP04 BB.014 Gas Detector15 The area under the ion peak is clearly larger than the area under the electron peak. The signal is caused by the motion of the charges in the 1 mm gap (not by the collection of the charges). Most of the charges generated by the avalanche are produced close to the anode so that electrons move only a short distance, while the ion move almost the entire millimeter. Signal processing can easily remove the slow ion peak form the signal.

E. Norbeck U. IowaDNP04 BB.014 Gas Detector16 PPAC can be made resistant to radiation damage The walls and electrodes can be made of durable metal in high-energy applications. A single spark can make a sharp point on the metallic surface of the cathode that will make the PPAC inoperable. The energy carried by a spark must be kept small, and provision must be made to keep sparking to a minimum. Aging (polymerizing of the gas) must be prevented. (Low pressures and short distances require special considerations.)

E. Norbeck U. IowaDNP04 BB.014 Gas Detector17 Conclusions Small area PPACs can be made to be radhard and fast ~ ns. PPACs have been used for 30 years, but more research is still needed maximize their potential.