Surface Wave Propagation Preliminary work developing a method for surface wave detection Amy Zheng Andrew Johnanneson.

Slides:



Advertisements
Similar presentations
Light Waves and Polarization Xavier Fernando Ryerson Communications Lab
Advertisements

AP Physics Mr. Jean March 30 th, The plan: Review of slit patterns & interference of light particles. Quest Assignment #2 Polarizer More interference.
Waves Sending energy at different wavelengths. Outline Waves and Solar Energy Definitions and Descriptions Sources and disturbances Velocity and the medium.
Q3. Use your answer from Q2 to find the angle of refraction when the angle of incident is; a) 30 o b) 80 o c) 0 o Q4. What happens to the period of the.
Jeopardy ELECTROMAGNE TIC SPECTRUM WAVESSOUND LIGHT MIX UP Q $100 Q $200 Q $300 Q $400 Q $500 Q $100 Q $200 Q $300 Q $400 Q $500 Final Jeopardy.
Waves and Light. A wave is a pattern that moves. A wave is a pattern that moves. As the pattern moves, the medium may “jiggle”, but on average it stays.
LIGHT A FORM OF ELECTROMAGNETIC RADIATION THAT STIMULATES THE EYE.
July 29, 2003; M.Chiba1 Study of salt neutrino detector for GZK neutrinos.
Phys 102 – Lecture 22 Interference 1. Physics 102 lectures on light Lecture 15 – EM waves Lecture 16 – Polarization Lecture 22 & 23 – Interference & diffraction.
Lecture 8: Measurement of Nanoscale forces II. What did we cover in the last lecture? The spring constant of an AFM cantilever is determined by its material.
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.
Chapter 33 Electromagnetic Waves
6. Interference by thin films t No phase shift (if n 2 < n 1 ) Phase shift -_____ (if n 2 > n 1 ) If there is a very thin film of material – a few wavelengths.
Electromagnetic Waves
6. Interference by thin films
Electromagnetic waves Physics 2102 Gabriela González.
1© Manhattan Press (H.K.) Ltd. The composition of electromagnetic waves electromagnetic waves Electromagnetic spectrum Electromagnetic spectrum 8.5 Electromagnetic.
Wave Behavior BY JON. The Physics of Waves  All waves follow the laws of physics no matter what type  Waves can be reflected, refracted, diffracted.
Physics 2112 Lecture 23 Electricity & Magnetism Lecture 23, Slide 1.
Stellar Parallax & Electromagnetic Radiation. Stellar Parallax Given p in arcseconds (”), use d=1/p to calculate the distance which will be in units “parsecs”
The Hong Kong Polytechnic University Optics II----by Dr.H.Huang, Department of Applied Physics1 Light Waves Nature of Light: Light can be viewed as both.
3.1 - RADIATION.  When you admire the colors of a rainbow, you are seeing light behave as a wave.  When you use a digital camera to take a picture of.
Simulation Issues for Radio Detection in Ice and Salt Amy Connolly UCLA May 18 th, 2005.
SOUND Sound is energy transferred by the compression & rarefaction of matter: sound waves are compressional waves Collisions between molecules transfer.
Waves S8P4: Students will explore the wave nature of sound and electromagnetic radiation.
MECHANICAL WAVES WAVE PROPERTIES SOUND…“WHAT?”
Goal: To understand the basics of reflection and refraction Objectives: 1)To understand the Propagation of light 2)To understand the following possibilities.
February 15 You will take a few notes about sound Then you will have some time to finish up the work from yesterday and/or the wave calculations.
Physics 1C Lecture 14B Today: End of Chapter 14 Start of Chapter 24.
Types of Traveling Waves
Waves: An introduction
Waves. Wave-Particle Duality The electron was previously describe by J.J. Thompson as a particle. He won a Nobel prize for his research His son, George.
Lecture 20 Electromagnetic Waves Nature of Light
Physics 1202: Lecture 18 Today’s Agenda Announcements: –Lectures posted on: –HW assignments, etc.
Waves and Energy Transfer 14.1 Wave Properties Wave A repeating disturbance or movement that transfers energy through matter or space.
M.Chiba_ARENA20061 Measurement of Attenuation Length for Radio Wave in Natural Rock Salt and Performance of Detecting Ultra High- Energy Neutrinos M.Chiba,
General Frequency Ranges Microwave frequency range –1 GHz to 40 GHz –Directional beams possible –Suitable for point-to-point transmission –Used for satellite.
Solids and Light – Introduction to Light
Weather and Climate Unit Investigative Science. * All materials are made of particles (atoms and molecules), which are constantly moving in random directions.
RICE: ICRC 2001, Aug 13, Recent Results from RICE Analysis of August 2000 Data See also: HE228: Ice Properties (contribution) HE241: Shower Simulation.
Wave Properties. S8P4. Students will explore the wave nature of sound and electromagnetic radiation. d. Describe how the behavior of waves is affected.
Waves S8P4 - Students will explore the wave nature of sound and electromagnetic radiation. a. Identify the characteristics of electromagnetic and mechanical.
June 27 th 2008ARENA Permafrost - An Alternative Target Material for Ultra High Energy Neutrino Detection ? R. Nahnhauer, A. Rostovtsev and D. Tosi.
Signal Propagation Basics
Surface plasmon resonance
Waves Vocabulary words are in red. Mechanical Wave A disturbance in matter that carries energy from one place to another Require matter (solid, liquid,
Antennas and Propagation
Week Four Principles of EMR and how EMR is used to perform RS
17. Electromagnetic waves
6. Interference by thin films
الفيزياء د/هالة مصطفى احمد.
Review of basic EM concepts
Waves.
Waves & Sound I. Characteristics of Waves Waves Transverse waves
Waves.
Unit 9 WAVES.
Electromagnetic Waves
GZK Neutrino Spectrum. GZK Neutrino Spectrum How the detection scheme words.
Waves.
Electromagnetic Radiation
Review of basic EM concepts
Think, Pair, Share Activity
4th Quarter Week 6 Vocabulary.
B. Wave optics Huygens’ principle
6. Interference by thin films
Reflection Amplitude Pitch Dictionary Definition 3 Examples
الفيزياء الحيوية الطبية Medical Biophysics
Propagation Effects on Communication Links
WAVES.
Electromagnetic Waves
Presentation transcript:

Surface Wave Propagation Preliminary work developing a method for surface wave detection Amy Zheng Andrew Johnanneson

Ultrahigh Energy Neutrino Detection Particles with velocity > will emit radiation due to the Askaryan effect [1] Detection is difficult due to internally reflected waves dying off quickly [2]

Surface Waves as an Detection Tool Radiation from Askaryan cascade is trapped in Air- dielectric layer between ice and firn [2] In tandem with existing experiments RICE [3] and ANITA [4]

Why Use Surface Waves? Surface waves travel between two mediums [5] ▫Amplitudes fall at the rate ▫Attenuation length times > bulk waves ~800 times more efficient than bulk waves If detection is viable, expanding existing experiments would be far less expensive Surface waves may carry information about neutrinos and their interactions with ice better than the current method

Procedure 1 sending + 2 receiving antennas displayed waveshape Physically moved antennas to determine wavelength and thus index of refraction

Example Antenna Placements “Surface” “In” “Air”

Translating to refractive index (1) (2) Definition of Refractive Index Sellmeier Equation

Refractive Index of Air Calculated (2) 1000MHz & 1500MHz n= [6] Single or Half λ λ (cm)

Refractive Index of Water (rms) Calculated (2) n~1.3333[7] Single or Half λ λ (cm)

Refractive Index of NaCl (rms) Single or Half λ λ (cm) Calculated (2) n~1.544[8]

Refractive Index of Granulated Fused Silica (sand) Calculated (2)1000MHz n= [9] Calculated (2) 1500MHz n= Single or Half λ λ (cm)

Refractive Index of Granulated Fused Silica (sand) Calculated (2) 1000MHz n= [9] Calculated (2) 1500MHz n= Multiple λ λ (cm)

Measurement Complications Mechanical water waves appeared to alter EM waveform Imprecise measurements due to hand & eye observation Sand and water tend to collect in the connectors Angular error from planar disparity Waveforms disappeared & reappeared on and off Waveforms constantly shift amplitude Background EM noise & reflections often interfered

Future Steps Experiment using ice as a medium Change antenna size; more precision Change experimental scale

References [1] G.A. Askaryan, Sov. Phys. JETP 14, 441 (1961) [2]J.P. Ralston, Phys. Rev. D 71, (2005) [3] RICE Collaboration, I. Kravchenko et al., Astropart. Phys. 19, 15 (2003); S. Razzaque, Sseunarine, D.Z. Besson, D.W. McKay, J.P. Ralston, and D. Seckel, Phys. Rev. D 65, (2002); Phys. Rev. D 69, (2004). [4] For information on ANITA, see [5] J. P. Ralston “An Experiment to Detect Surface Waves on Polar Ice” (2005) [6] Philip E. Ciddor. Refractive index of air: new equations for the visible and near infrared, Appl. Optics 35, (1996) doi: /AO [7]P. Schiebener, J. Straub, J.M.H. Levelt Sengers and J.S. Gallagher, J. Phys. Chem. Ref. Data 19, 677, (1990) [8] Faughn, Jerry S., Raymond A. Serway. College Physics, 6th Edition. Toronto: Brooks/Cole, 2003: 692. [9] I. H. Malitson. Interspecimen Comparison of the Refractive Index of Fused Silica, J. Opt. Soc. Am. 55, (1965) doi: /JOSA [misc] Colloquium Notes from John P. Ralston Refractive index calculations for relative reference only: ▫n found for granulated fused silica was found using Sellmeier constants for solid fused silica; granulation affects density. ▫Calculated n for water is for λ of nm ▫Calculated n for NaCl is for λ of 589 nm

Acknowledgements Dave Besson Marie Piasecki Carolyn Bandle