Anita-Sim David Seckel, ANITA Collab. Mtg. Nov. 24-25, /2002 Notes on building a full ANITA simulation.

Slides:



Advertisements
Similar presentations
Practical techniques and tips for probing and de-embedding.
Advertisements

Testing of ILS Receivers in a Multipath Propagation Environment International Flight Inspection Symposium Oklahoma City, OK USA June 2008 Jochen Bredemeyer,
Surface Wave Propagation Preliminary work developing a method for surface wave detection Amy Zheng Andrew Johnanneson.
Air Shower Simulations for ANITA K. Belov UCLA. Goals Approach Estimate the energy of the UHECRs detected by ANITA using MC simulations Use well known.
ANITA: Results from ANITA-lite test flight and warming up for this year’s ANITA flight Amy Connolly for the ANITA Collaboration International Tau Neutrino.
E.g. an IceCube Surfave Veto Array TAXI. Transportable Array for eXtremely large area Instrumentation studies Timo Karg, Rolf Nahnhauer DESY IceCube Collaboration.
The GRAND proto A prototype array to evaluate the potential of EAS identification of the radio technique.
High-Multiplicity Events Analysis Group March 28, 2005 Leon R.
By Devin Gay Radio Ice Cerenkov Experiment. RICE got off the ground and into the ice in 1995 They got started when AMANDA collaborations agreed to co-
M. Kowalski Search for Neutrino-Induced Cascades in AMANDA II Marek Kowalski DESY-Zeuthen Workshop on Ultra High Energy Neutrino Telescopes Chiba,
Calibration of the 10inch PMT for IceCube Experiment 03UM1106 Kazuhiro Fujimoto A thesis submitted in partial fulfillment of the requirements of the degree.
Tampa APS Meeting April 2004 P. Gorham 1 UH ANITA monte carlo Peter Gorham University of Hawaii A N I T A.
Shower & RF theory David Seckel, ANITA Collab. Mtg. Nov , /2002 Theory Notes on Shower and Radio Pulse.
Tuning in to UHE Neutrinos in Antarctica – The ANITA Experiment J. T. Link P. Miočinović Univ. of Hawaii – Manoa Neutrino 2004, Paris, France ANITA-LITE.
Wireless Transmission Fundamentals (Physical Layer) Professor Honggang Wang
Search for isotropic microwave radiation from electron beam in the atmosphere T. Yamamoto a, I. S. Ohota a, Y. Inome a, D. Ikeda b, H. Sagawa b, S. Ogio.
July 10, 2007 Detection of Askaryan radio pulses produced by cores of air showers. Suruj Seunarine, Amir Javaid, David Seckel, Philip Wahrlich, John Clem.
RADAR Detection of Extensive Air Showers Nils Scharf III. Physikalisches Institut A Bad Honnef Nils Scharf III. Physikalisches Institut A Bad.
Studies of the Energy Resolution of the ANITA Experiment Amy Connolly University of California, Los Angeles CALOR06 June 6 th, 2006.
Simulation Issues for Radio Detection in Ice and Salt Amy Connolly UCLA May 18 th, 2005.
Antares simulation tools J. Brunner CPPM. Software scheme Calibrations Main stream External input Simulation Reconstruction.
1 of 22 Glaciers and Ice Sheets Interferometric Radar (GISIR) Center for Remote Sensing of Ice Sheets, University of Kansas, Lawrence, KS
14/02/2007 Paolo Walter Cattaneo 1 1.Trigger analysis 2.Muon rate 3.Q distribution 4.Baseline 5.Pulse shape 6.Z measurement 7.Att measurement OUTLINE.
IRA April 2006 D.F. Cowen/IceCube Collab. Beyond IceCube Beijing UHE  Workshop 1 Beyond the South Pole Outline  Introduction: Optical vs. Radio.
K.C.RAVINDRAN,GRAPES-3 EXPERIMENT,OOTY 1 Development of fast electronics for the GRAPES-3 experiment at Ooty K.C. RAVINDRAN On Behalf of GRAPES-3 Collaboration.
Future Directions Radio A skaryan U nder ice R adio A rray Hagar Landsman Science Advisory Committee meeting March 1 st, Madison.
1 N eutrino E xtended S ubmarine T elescope with O ceanographic R esearch Operation and performance of the NESTOR test detector.
Performance of CRTNT for Sub-EeV Cosmoc Ray Measurement Zhen Cao IHEP, Beijing & Univ. of Utah, SLC Aspen, CO, 04/2005.
Acoustics Research Group, Department of Electrical & Computer Engineering, University of Canterbury, New Zealand Acoustics Research Group Towards an understanding.
ACoRNE*, UK The calibration and experiment of transmitter array for the acoustic neutrino detection W. Ooppakaew*, S. Danaher*, R. Lahmann**, K. Graf**
Propagation Models Large scale models predict behavior averaged over distances >>  Function of distance & significant environmental features, roughly.
radio lobe sound disk  t p ~ km  optical light cone The Vision *) see e.g. A. Ringwald,ARENA 2005 Build ~100 km 3 hybrid detector to: Confirm GZK cutoff.
NESTOR SIMULATION TOOLS AND METHODS Antonis Leisos Hellenic Open University Vlvnt Workhop.
The Interconnect Modeling Company™ High-Speed Interconnect Measurements and Modeling Dima Smolyansky TDA Systems, Inc.
Mobile Computing and Wireless Networking Lec 02
Detection of UHE Shower Cores by ANITA By Amir Javaid University Of Delaware.
COMMUNICATION SYSTEMS (5marks)
I3/CA Europlanet - EC Contract Space Research Institute Austrian Academy of Sciences Non-thermal radio emission fundamentals:
RICE David Seckel, NeSS02, Washington DC, Sept ,/2002 R adio I ce C herenkov E xperiment PI presenter.
ANtarctic Impulsive Transient Antenna University of Hawaii at Manoa Peter Gorham, PI John Learned and Gary S. Varner Ohio-State University Jim Beatty and.
EAS Time Structures with ARGO-YBJ experiment 1 - INFN-CNAF, Bologna, Italy 2 - Università del Salento and INFN Lecce, Italy A.K Calabrese Melcarne 1, G.Marsella.
May 17-19, 2005D. Zaborov, ARENA workshop1 Dmitry Zaborov for the ITEP group Berlin, May 2005 Analysis methods of ITEP Baikal data.
Detection of UHE Shower Cores by ANITA By Amir Javaid University Of Delaware.
IceTop DAQ: 1 David Seckel – 8/27/2003, College Park, MD IceTop Data Handler and Triggers David Seckel University of Delaware.
RICE: ICRC 2001, Aug 13, Recent Results from RICE Analysis of August 2000 Data See also: HE228: Ice Properties (contribution) HE241: Shower Simulation.
Another Straw-person SALSA Simulation Amy Connolly UCLA February 4 th, 2005 Work by A. Connolly, D. Saltzerg and D. Williams.
Studies of Askaryan Effect, 1 of 18 Status and Outlook of Experimental Studies of Askaryan RF Radiation Predrag Miocinovic (U. Hawaii) David Saltzberg.
HEP Tel Aviv UniversityLumical - A Future Linear Collider detector Lumical R&D progress report Ronen Ingbir.
South Pole Astro April 4, 2011 Tom Gaisser1 125 m Cosmic-ray physics with IceCube IceTop is the surface component of IceCube as a three-dimensional cosmic-ray.
Search for UHE Neutrinos with AMANDA Stephan Hundertmark University of California, Irvine Methodical Aspects of Underwater/Ice Neutrino Telescopes Hamburg,
June 19, 2009 Simulation of Askaryan Detectors and Events (SADE) David Seckel, Pat Stengel, Shahid Hussain D. Seckel, Univ. of Delaware.
IceTop Design: 1 David Seckel – 3/11/2002 Berkeley, CA IceTop Overview David Seckel IceTop Group University of Delaware.
June 18-20, 2009 Detection of Askaryan radio pulses produced by cores of air showers. Suruj Seunarine, David Seckel, Pat Stengel, Amir Javaid, Shahid Hussain.
Signal Propagation Basics
IceRay: an IceCube-Centered Radio GZK Array John Kelley for Bob Morse and the IceRay collaboration April 30, 2008.
The ARA concept and history construction activities Future plans The ARA concept and history construction activities Future plans Kara.
IceRay: an IceCube-Centered Radio GZK Array John Kelley University of Wisconsin, Madison for the IceRay working group ARENA08, Rome.
1 Cosmic Ray Physics with IceTop and IceCube Serap Tilav University of Delaware for The IceCube Collaboration ISVHECRI2010 June 28 - July 2, 2010 Fermilab.
Shih-Hao Wang 王士豪 Graduate Institute of Astrophysics & Leung Center for Cosmology and Particle Astrophysics (LeCosPA), National Taiwan University 1 This.
Passive Microwave Remote Sensing
The GRAND proto A prototype array to evaluate the potential of the radio polarization measurement for EAS identification.
Simulation of a hybrid optical-radio-acoustic neutrino detector at South Pole D. Besson [1], R. Nahnhauer [2], P. B. Price [3], D. Tosi [2], J. Vandenbroucke.
SADE ANITA Monte Carlo(SAM) Test Results Amir Javaid University of Delaware.
Topics The case for remote radio detection of neutrinos
Systematic uncertainties in MonteCarlo simulations of the atmospheric muon flux in the 5-lines ANTARES detector VLVnT08 - Toulon April 2008 Annarita.
Transmission lines I 1.
GZK Neutrino Spectrum. GZK Neutrino Spectrum How the detection scheme words.
8.7 Gated Integration instrument description
ANITA simulations P. Gorham 5/12/2019 P. Gorham.
Project: IEEE P Working Group for Wireless Personal Area Networks (WPANs) Submission Title: [Channel characterization proposed for Body Area Network]
Presentation transcript:

Anita-Sim David Seckel, ANITA Collab. Mtg. Nov , /2002 Notes on building a full ANITA simulation.

Anita-Sim David Seckel, ANITA Collab. Mtg. Nov , /2002 Outline Event Generator Shower parameterization Pulse Propagation through ice Ice/air interface Propagation through air Antennas Instrument model 1: trigger side Instrument model 2: waveform side

Anita-Sim David Seckel, ANITA Collab. Mtg. Nov , /2002 Event Generator Earth model Need local topography, geology, air Neutrino cross-sections standard model PQCD (+/- 25%) –NC/CC different levels of agreement. Non standard model cross-sections Tau propagation Other particles…Monopoles…

Anita-Sim David Seckel, ANITA Collab. Mtg. Nov , /2002 Shower parameterization simple: N max, curvature d 2 N/dx 2 list of sub-showers … tbd

Anita-Sim David Seckel, ANITA Collab. Mtg. Nov , /2002 Pulse creation Real pulse includes all the propagation issues… Do a spectral analysis, reconstruct at the antenna

Anita-Sim David Seckel, ANITA Collab. Mtg. Nov , /2002 Propagation through Ice Attenuation (temperature, composition) Refraction Scattering ? bi-refringence

Anita-Sim David Seckel, ANITA Collab. Mtg. Nov , /2002 Ice/Air interface Surface roughness Multiple lines of site Shadowing Polarization

Anita-Sim David Seckel, ANITA Collab. Mtg. Nov , /2002 Propagation through air Dispersion Refraction

Anita-Sim David Seckel, ANITA Collab. Mtg. Nov , /2002 Antennas Angular and spectral, polarization response. Mutual impedence Calibrated instrument Simulate noise

Anita-Sim David Seckel, ANITA Collab. Mtg. Nov , /2002 Instrument trigger TBD Frequency domain until it hits the discriminator convert to time domain at disc

Anita-Sim David Seckel, ANITA Collab. Mtg. Nov , /2002 Instrument Waveform Digization TBD RF instrument freq -> time domain Characteristics of digitizers… Maintain database of instrument state channel characteristics

Feedback: Privacy Policy Feedback
Do Not Sell My Personal Information
About project: SlidePlayer Terms of Service

© 2025 SlidePlayer.com. Inc. All rights reserved.