Evaluation of disturbances due to test mass charging for LISA and LISA Pathfinder. DNA Shaul, HM Araujo, GK Rochester, TJ Sumner, PJ Wass

Size: px
Start display at page:

Download "Evaluation of disturbances due to test mass charging for LISA and LISA Pathfinder. DNA Shaul, HM Araujo, GK Rochester, TJ Sumner, PJ Wass"

Transcription

1 Evaluation of disturbances due to test mass charging for LISA and LISA Pathfinder DNA Shaul, HM Araujo, GK Rochester, J Sumner, PJ Wass 5 th International LISA Symposium, ESEC, Wednesday 14 th July 004

2 alk Outline Electrostatic analyses (LP GRS) - FE model of entire GRS - FE CM submodels + Comparison to // plate COULOMB Charging Disturbance Estimates LISA & LISA PF Solar Max & Min LORENZ Method to Cope with Charging

3 Why do Ms charge up? Ms can charge up due to: Galactic cosmic rays Solar particles Solar Flare (RACE) Crab Nebula More in later talks

4 Why does charging matter? Charging of Ms disturbs their geodesic motion Unwanted forces from: Coulomb interactions with surrounding conductors of GRS Charge-dependent Coulomb accn: a Qk = Q C m + QV mc Q mc N 1 i= 1 V i i,n => erms ~ k => erms~ V & V k Lorentz interactions as it moves through magnetic fields Lorentz accn: ( Q m) V B a L = Sun IMF Ulysses (GSFC) Earth

5 Main charging Disturbances 1. Acceleration Noise (from fluctuations in: charge, M position & velocity, voltages, magnetic field). Modification of stiffness (from position dependence) 3. Coherent Fourier components (as Q(t) ~t) Parasitic coupling arget LISA Strain Noise Stray forces x Courtesy: S. Vitale Q(t) t

6 Electrostatic FE model of LP GRS Coulomb accn is capacitance and hence geometry dependent 1 C C k C k = 0 + Move in 1 DOF, Sym => ( ) ( ) a Detere energy in system for given geometry & voltage distribution using FE analysis (ANSYS software) Change V distribution => capacitances between specific conductors Change M position => capacitance derivatives YZ-injection sensor design* (LISA PF LP GRS EM design) Qk = Q C k m C k C x + QV mc Q mc = 1.15 ± 0.01µ F/ m N 1 i= 1 V i i,n % > than ANSYS (1σ errors # ~ 1%) // plate ( = 0) = 33.7 ± 0.pF 30% 1% 46mm side M Gaps: X face: 4 mm sens Y face:.9 mm sens, 4 mm inj Z face: 3.5 mm sens, 4 mm inj z x * B Weber et al. 03 SPIE y C y C z =.50 ± 0.03µ F / m = 1.6 ± 0.03µ F / m # Shaul & Sumner 04 CNME 1% 7%

7 LP M CM: 1 Plunger, 4 stoppers & corresponding M recesses, per z face. (Plunger tip level with recessed, injection electrodes during science mode) (1) Pyramidal plunger & baseball-glove-shaped stoppers (ht 1.5mm)* OR () Pyramidal plunger & alternative, elongated stoppers (l gth 1mm, ht 1mm) * For either set of features, C & C unchanged to within 0.4σ & 1.σ respectively z * D Smart, S obin et al.

8 Submodel CM => estimate CM influence more accurately Positions of borders chosen as compromise between model size & distance from RoI => imise effect on couplings of interest. BCs were not derived from the full model => avoid confounding models accuracies Plunger Baseball glove stopper Alternative, elongated stopper Reduced model complexity (effects results only at the ~1% level) Sign depends on which side of the sensor the feature is located C M,CM: ( ± ) ± ( 1.10 ± 0.01) z + ( 3334 ± 58) z ( ± ) ± ( ± 0.01) z + ( 660 ± 6) z ( ± ) ± ( 9.31± 0.03) z + ( 879 ± 137) z Figures represent the properties of CM, NO increase in capacitance when CM added as not compared no CM case Other capacitances will be affected by the inclusion of CM. hese figures indicate CM level of influence.

9 Comparison of CM to full sensor otal C M,CM < 3% C for both types of stopper otal C < 4% & 9% for CM with bbg stoppers & elongated stoppers a Qk M, CM z C z Only 0.7% from plungers In dc /dk, this gets multiplied by M offset from the centre of opposing features C ease the positioning Q N 1 QV C Q Ci,N = + V => erms ~ z => requirements of the i C m mc mc i= 1 z retracted CM (E.g. M offset of 50µm from the centre of the plungers => contribution of ~3% of that when the M is offset 10µm wrt entire sensor) M, CM z < 9%, 6% & 14% of that of a single z-face, sensing electrode for a pyramidal plunger, a bbg stopper & an elongated stopper Q N 1 i,n a Qk =... Vi => erms ~ mc i= 1 => Need to maintain a high level of uniformity in the CM surfaces, to imise work function differences, as patch effects could multiply these gradients into significant effects Similarly, to imise the CM contribution to stiffness, the mean voltage of opposing features should also be imised. i z V i

10 Magnitude of Charging Disturbances (using ANSYS results for sensitive x-axis)

11 Net charging rate (GEAN GCR) (+e/s) "Worst case" net charging rate assumed (+e/s) Effective charging rate, R eff (+e/s) e x (t) (S/N) Stiffness, s Qx (s - ) Displacement noise (ms - Hz -0.5 ) Voltage noise (ms - Hz -0.5 ) Lorentz noise (ms - Hz -0.5 ) otal noise (ms - Hz -0.5 ) Charging Rates 4, Assume worst case charging conditions: f x (t) (S/N) + error margin of ~30% l x (t) (S/N) e/s+ (may ~cancel in the actual sensor) 100 ~30% on the GEAN GCR 7.35 charging rates e/s for kinetic low-energy secondary 0.57 electron 0.30 emission E E E-16 1.E-16 6.E-16 max , E E-18.39E E E , E E E E E-16 Within Limit? max , E E-18 Charge Rate of noise SEP (ms events - Hz -0.5 ) expected to be low 3.97E-16 enough that 3.07E-16 data acquisition 4.04E-16 could be suspended for their duration, but needs to be verified [δq (CHz -0.5 ) = (R eff ) 0.5 e/πf] 3.09E-16.5E E E-16 For f ~ 10-4 Hz charging & Lorentz noise and coherent component estimates largest LISA: Araujo H et al submitted to Astroparticle Physics, arxiv:astro-ph/ LISA PF: Wass P et al in preparation. ~

12 e x (t) (S/N) f x (t) (S/N) l x (t) (S/N) Coherent Charging Signals For f ~ 10-4 Hz estimates largest (τ = 1 yr; = 1day) S/N Stiffness, is the s Qx ratio (s - ) of the charging signal to -1.11E-08 the acceleration -5.7E-09 noise -1.00E-08 budget -4.93E-09 for LISA Displacement noise (ms - Hz -0.5 ) Charge noise (ms - Hz -0.5 ) Voltage noise (ms - Hz -0.5 ) Lorentz noise (ms - Hz -0.5 ) otal noise (ms - Hz -0.5 ) e f k (t) Θ t k QV & t mc k ( t) Ξkt t C m x f (Hz) 1E-04 1E-03 1E-0 1E-01 1E+00 resultant Q& Qt & mc N 1 V i= 1 i in () ( t Φ t ηq& t m)[ V B ] xˆ x e x (t) Accn noise l x (t) I f x (t) l IP 1E-09 1E-11 1E-13 1E-15 1E-17 (ms-hz-0.5) 4, E E-16 Acceleration spectral density 4.6E-16 1.E-16 6.E-16 Q(t) max, E E-16.39E E E-16 4, E E E E E-16 Within Limit? max, f (Hz) 1E-04 1E-03 1E-0 f x (t) Sens S/N = 5 Magnitudes plotted 1E-19 at primary peaks of sinc functions e x (t) WDB 8.0E E-16.5E E E-16 1E-0 1E-1 1E- 1E-3 1E-4 ~ Coulomb signals dependent on: k (10µm), V (1mV), V (100mV), V (100mV) Lorentz signal dependent on mean B IP (~ 0.5n -> ~ 40n; median ~6n). Even 40n < accn noise) (η = 0.01) Exact spectral shape depends on discharging scheme & variability of e.g. mean charging rate (Shaul et al, CQG 04) t Equivalent strain in space

13 Stiffness, s Qx (s - ) Stiffness: GRS Requirement: -x10-8 -> 8x10-8 s E-08 max -5.7E E-08 Within Limit? max -4.93E-09 s Qk = m a Qk N 1 1 C, QV C Q C Q C N i N C i, N QV C Vi + V + 3 i i= 1 C C C i= 1 C Q = C ~V (100mV) erms that doate are ~ independent of k ~V (100mV) Q C C Independent of voltage

14 For f ~ 10-4 Hz (Charge noise~1/f) Displacement noise (ms - Hz -0.5 ) Charge noise (ms - Hz -0.5 ) Voltage noise (ms - Hz -0.5 ) Lorentz noise (ms - Hz -0.5 ) otal noise Qk (ms - Hz -0.5 ) δa Qk a N 1 a = δk + k i = 1 Vi aqk 1 = m s Qk Qk δx =.5nmHz δv 0.5 a 1 N = + 1 Qk Q C V C Q C m mc mc i= 1 aqk Q Q p, = C p N, V mc mc p N Coulomb Noise i aqk + Q V Doant term i i, δv = 10 / δq N 1.70E E E-16 1.E-16 6.E-16 µ VHz 0.5 max 8.54E E-16.39E E E E E E E E-16 max 8.0E E-16.5E E E-16 : all terms same order of magnitude ~

15 For f ~ 10-4 Hz (Lorentz noise~1/f 1.6 ) Lorentz noise (ms - Hz -0.5 ) Lorentz Noise max max 1.E E E E-17 B IP = δb IP = Hz 0.5 B SC = δb SC = Hz 0.5 Lorentz accn: ( η Q& tvi BIP + ηqt & VI δbip + ηqt & δvi BIP + Qt & δvsc BSC + ηδqvi BIP ) m a L m Fluctuations in B IP Fluctuations in M velocity Charging shot noise Doant term by > 3 orders of magnitude so ~ insensitive to range of B IP Accn Noise

16 Charge noise (ms - Hz -0.5 ) Voltage noise (ms - Hz -0.5 ) Lorentz noise (ms - Hz -0.5 ) otal noise (ms - Hz -0.5 ) Magnitude of Charging Disturbances Net charging rate (GEAN GCR) (+e/s) "Worst case" net charging rate assumed (+e/s) Effective charging rate (+e/s) e x (t) (S/N) f x (t) (S/N) l x (t) (S/N) Stiffness, s Qx (s - ) Displacement noise (ms - Hz -0.5 ) , E E E E-16 1.E-16 6.E-16 max , E E E-16.39E E E , E E E E E E Noise Allocation =0% of LISA noise budget = ( f /3mHz) Within Limit? max , E E E-16.5E E E-16 [ ] 0. 5 ms Hz Reduce by ~ hrs => noise within spec If no contribution of secondaries -> net charging rate, total noise ~10-0% If V=1mV, the e(t) ~55%, stiffness ~90%, total noise ~0-30% ~

17 Comparison to //plate // plate approx overestimates Coulomb noise, stiffness, e x (t) by ~10% f x (t) by ~40% BU LEVEL OF AGREEMEN IS DEPENDEN ON SENSOR GEOMERY E.g. For similar rento torsion sensor design, FE results (validated in expt: Carbone et al 003 Physical Review Letters ) & // plate approx give similar levels of agreement But if exclude guard rings for this design, agreement : C (FE) = C (//) x 1.56 (from 1.30) agreement of nd derivatives wrt x, y & z ~same (~0-30%) //plate approx overestimates: noise, stiffness, e x (t) by ~30-40% f x (t) by ~110% guard rings imise fringing fields exact level of agreement between derived quantities also dependent on other parameters e.g. V => USE CAUION WHEN EMPLOY // PLAE APPROX

18 Management of disturbances UV light => discharge the Ms via pe effect. Noally, ~ 1 day => accn noise & stiffness within budget But coherent charging signals above noise target o remove charging signals: spectral analysis? continuous discharging of the Ms at a rate exceeding the charging rate? Disadvantage = increased noise 7.0E-16 Variation of total noise for LISA, with discharging rate, assug Q=0 Acceleration noise (ms - Hz -0.5 ) 6.5E E E E E E-16 hank-you Discharging rate (-e/s) Discharging rate = ~6 x Charging rate, to reach noal noise budget Variation in charging rate between & max ~ 50% => plausible that discharging rate could be set high enough to cope with variations in the GCR flux, without exceeding budgets Still need to quantify e.g. impact of restoration of equilibrium of charging and discharging currents following changes in the mean charging rate

2 Each satellite will have two test masses, each being the end mirror for an interferometer.

2 Each satellite will have two test masses, each being the end mirror for an interferometer. Ground Testing for LISA Test Masses with a Torsion Pendulum Matthew Schmidt Valdosta State University International REU: University of Trento, Italy Advisor: Dr. Bill Weber Abstract: One of the most important

More information

Simulation of the charging process of the LISA test masses due to solar particles.

Simulation of the charging process of the LISA test masses due to solar particles. Simulation of the charging process of the LISA test masses due to solar particles. 5 th International Lisa Symposium 14 July 2004 Helios Vocca INFN Pg Solar Energetic Particles (SEPs( SEPs) SEPs are particles

More information

Bayesian Statistics to calibrate the LISA Pathfinder experiment

Bayesian Statistics to calibrate the LISA Pathfinder experiment Bayesian Statistics to calibrate the LISA Pathfinder experiment Nikolaos Karnesis for the LTPDA team! http://gwart.ice.cat/! LISA Symposium X 20/05/2014 Outline LPF System Overview LPF System Identification

More information

PHOEBUS: Space Weather su LISA Helios Vocca

PHOEBUS: Space Weather su LISA Helios Vocca PHOEBUS: Space Weather su LISA Helios Vocca 1 a GW primer. Gravitational force cannot propagate instantaneously It can only propagate at the speed of light Conclusions: Gravitational force propagates as

More information

The Stanford Gravitational Reference Sensor

The Stanford Gravitational Reference Sensor The Stanford Gravitational Reference Sensor S. Buchman, B. Allard, G. Allen, R. Byer, W. Davis, D. DeBra, D. Gill, J. Hanson, G.M. Keiser, D. Lauben, I. Mukhar, N. A. Robertson, B. Shelef, K. Sun, S. Williams

More information

Electric Potential Energy Conservative Force

Electric Potential Energy Conservative Force Electric Potential Energy Conservative Force Conservative force or field is a force field in which the total mechanical energy of an isolated system is conserved. Examples, Gravitation, Electrostatic,

More information

Fundamental Physics in Space S. Vitale, University of Trento ESO-Garching S. Vitale 1

Fundamental Physics in Space S. Vitale, University of Trento ESO-Garching S. Vitale 1 Fundamental Physics in Space S. Vitale, University of Trento Vitale@science.unitn.it ESO-Garching-15-09-03 S. Vitale 1 Using Space to Investigate Fundamental Laws of Physics: Quantum measurements, entanglement,

More information

Electric Field of a uniformly Charged Thin Spherical Shell

Electric Field of a uniformly Charged Thin Spherical Shell Electric Field of a uniformly Charged Thin Spherical Shell The calculation of the field outside the shell is identical to that of a point charge. The electric field inside the shell is zero. What are the

More information

Exploring the Gravitational Wave Universe Challenges for a LISA Successor

Exploring the Gravitational Wave Universe Challenges for a LISA Successor Exploring the Gravitational Wave Universe Challenges for a LISA Successor H Ward University of Glasgow Cosmic Vision 2015 2025 Paris 15 th September 2004 With contributions from : P Bender, K Danzmann,

More information

Technology Readiness Level:

Technology Readiness Level: Technology Readiness Level: We plan to raise the TRL of the model with an acceleration noise performance requirement of < 10-12 m sec -2 Hz -1/2 at frequencies between 1 mhz and 1 Hz, from TRL 3 to TRL

More information

PETER: a double torsion pendulum to test quasi Free Fall on two Degrees of Freedom

PETER: a double torsion pendulum to test quasi Free Fall on two Degrees of Freedom PETER: a double torsion pendulum to test quasi Free Fall on two Degrees of Freedom Luciano Di Fiore Lorenzo Marconi, Ruggero Stanga, Noemi Finetti, INFN and Università di Firenze Massimo Bassan, Fabrizio

More information

LISA Pathfinder measuring pico-meters and femto-newtons in space

LISA Pathfinder measuring pico-meters and femto-newtons in space LISA Pathfinder measuring pico-meters and femto-newtons in space M Hewitson for the LPF team Barcelona, February 15th 2012 Observing from Space 2 Observing from Space 2 Observing from Space Push down to

More information

Catapult tests for microgravity characterization of the MICROSCOPE accelerometers. Manuel Rodrigues On behalf ONERA & ZARM team

Catapult tests for microgravity characterization of the MICROSCOPE accelerometers. Manuel Rodrigues On behalf ONERA & ZARM team Catapult tests for microgravity characterization of the MICROSCOPE accelerometers Manuel Rodrigues mrodrig@onera.fr On behalf ONERA & ZARM team 1 Instrument Description SU sqm Sensor Unit (SU) = differential

More information

EFFICIENT MULTI-PHYSICS MODELING OF THE DYNAMIC RESPONSE OF RF-MEMS SWITCHES

EFFICIENT MULTI-PHYSICS MODELING OF THE DYNAMIC RESPONSE OF RF-MEMS SWITCHES EFFICIENT MULTI-PHYSICS MODELING OF THE DYNAMIC RESPONSE OF RF-MEMS SWITCHES Jeroen Bielen 1, Jiri Stulemeijer 1 1 EPCOS Netherlands Deepak Ganjoo 2, Dale Ostergaard 2, Stephen Scampoli 2 2 Ansys Inc.

More information

ERROR SOURCE IDENTIFICATION AND STABILITY TEST OF A PRECISION CAPACITANCE MEASUREMENT SYSTEM

ERROR SOURCE IDENTIFICATION AND STABILITY TEST OF A PRECISION CAPACITANCE MEASUREMENT SYSTEM 106 SOUTH AFRICAN INSTITUTE OF ELECTRICAL ENGINEERS Vol.101(3) September 2010 ERROR SOURCE IDENTIFICATION AND STABILITY TEST OF A PRECISION CAPACITANCE MEASUREMENT SYSTEM S. Nihtianov* and X. Guo* # *

More information

A.M. THURSDAY, 23 May hour

A.M. THURSDAY, 23 May hour Surname Other Names Centre Number 0 Candidate Number GCSE 4503/02 PHYSICS PHYSICS 3 HIGHER TIER A.M. THURSDAY, 23 May 2013 1 hour ADDITIONAL MATERIALS In addition to this paper you may require a calculator.

More information

MARKING SCHEME SET 55/1/RU Q. No. Expected Answer / Value Points Marks Total Marks

MARKING SCHEME SET 55/1/RU Q. No. Expected Answer / Value Points Marks Total Marks MARKING SCHEME SET 55//RU Q. No. Expected Answer / Value Points Marks Total Marks Set, Q Set2,Q5 Set,Q4 Section A Self inductance of the coil is numerically equal to magnetic flux linked with it when unit

More information

Transducers. Today: Electrostatic Capacitive. EEL5225: Principles of MEMS Transducers (Fall 2003) Instructor: Dr. Hui-Kai Xie

Transducers. Today: Electrostatic Capacitive. EEL5225: Principles of MEMS Transducers (Fall 2003) Instructor: Dr. Hui-Kai Xie EEL55: Principles of MEMS Transducers (Fall 3) Instructor: Dr. Hui-Kai Xie Last lecture Piezoresistive Pressure sensor Transducers Today: Electrostatic Capacitive Reading: Senturia, Chapter 6, pp. 15-138

More information

Measurement of Angular Stray DC Potentials for. Test Masses in LISA Pathfinder

Measurement of Angular Stray DC Potentials for. Test Masses in LISA Pathfinder Measurement of Angular Stray DC Potentials for Test Masses in LISA Pathfinder Michael Aitken Università degli Studi di Trento European Space Agency University of Florida August 9, 2016 Abstract Launched

More information

EE C247B ME C218 Introduction to MEMS Design Spring 2016

EE C247B ME C218 Introduction to MEMS Design Spring 2016 EE C47B ME C18 Introduction to MEMS Design Spring 016 Prof. Clark T.-C. Nguyen Dept. of Electrical Engineering & Computer Sciences University of California at Berkeley Berkeley, CA 9470 Lecture EE C45:

More information

Coulomb s constant k = 9x10 9 N m 2 /C 2

Coulomb s constant k = 9x10 9 N m 2 /C 2 1 Part 2: Electric Potential 2.1: Potential (Voltage) & Potential Energy q 2 Potential Energy of Point Charges Symbol U mks units [Joules = J] q 1 r Two point charges share an electric potential energy

More information

PHYA4/2. General Certificate of Education Advanced Level Examination January Unit 4 Fields and Further Mechanics Section B

PHYA4/2. General Certificate of Education Advanced Level Examination January Unit 4 Fields and Further Mechanics Section B Centre Number Surname Candidate Number For Examiner s Use Other Names Candidate Signature Examiner s Initials Physics A Unit 4 Fields and Further Mechanics Section B General Certificate of Education Advanced

More information

Physics 1B Spring 2010: Final Version A 1 COMMENTS AND REMINDERS:

Physics 1B Spring 2010: Final Version A 1 COMMENTS AND REMINDERS: Physics 1B Spring 2010: Final Version A 1 COMMENTS AND REMINDERS: Closed book. No work needs to be shown for multiple-choice questions. 1. Four charges are at the corners of a square, with B and C on opposite

More information

Chapter 16 Electrical Energy Capacitance. HW: 1, 2, 3, 5, 7, 12, 13, 17, 21, 25, 27 33, 35, 37a, 43, 45, 49, 51

Chapter 16 Electrical Energy Capacitance. HW: 1, 2, 3, 5, 7, 12, 13, 17, 21, 25, 27 33, 35, 37a, 43, 45, 49, 51 Chapter 16 Electrical Energy Capacitance HW: 1, 2, 3, 5, 7, 12, 13, 17, 21, 25, 27 33, 35, 37a, 43, 45, 49, 51 Electrical Potential Reminder from physics 1: Work done by a conservative force, depends only

More information

Observing the gravitational universe from space

Observing the gravitational universe from space Observing the gravitational universe from space Peter Wass Tim Sumner, Daniel Hollington, Jonathon Baird High Energy Physics Group Imperial Space Lab 29 September 2015 Gravitational Waves Gravitational

More information

LISA Pathfinder Coldgas Thrusters

LISA Pathfinder Coldgas Thrusters LISA Pathfinder Coldgas Thrusters Joseph Martino/Eric Plagnol - LPF collaboration Lisa Symposium September 2016 Zurich Outline System Description External Disturbances and thruster noise In Flight dedicated

More information

LISA mission design. Guido Mueller. APS April Meeting, Jan 30th, 2017, Washington DC

LISA mission design. Guido Mueller. APS April Meeting, Jan 30th, 2017, Washington DC LISA mission design Guido Mueller University of Florida APS April Meeting, Jan 30th, 2017, Washington DC 1 L3 from ESA s perspective 2013: Selection of L3 Science Theme by ESA The Gravitational Universe

More information

CHAPTER 4 DESIGN AND ANALYSIS OF CANTILEVER BEAM ELECTROSTATIC ACTUATORS

CHAPTER 4 DESIGN AND ANALYSIS OF CANTILEVER BEAM ELECTROSTATIC ACTUATORS 61 CHAPTER 4 DESIGN AND ANALYSIS OF CANTILEVER BEAM ELECTROSTATIC ACTUATORS 4.1 INTRODUCTION The analysis of cantilever beams of small dimensions taking into the effect of fringing fields is studied and

More information

EE C245 ME C218 Introduction to MEMS Design

EE C245 ME C218 Introduction to MEMS Design EE C245 ME C218 Introduction to MEMS Design Fall 2007 Prof. Clark T.-C. Nguyen Dept. of Electrical Engineering & Computer Sciences University of California at Berkeley Berkeley, CA 94720 Lecture 22: Capacitive

More information

EE C245 ME C218 Introduction to MEMS Design

EE C245 ME C218 Introduction to MEMS Design EE C245 ME C218 Introduction to MEMS Design Fall 2007 Prof. Clark T.-C. Nguyen Dept. of Electrical Engineering & Computer Sciences University of California at Berkeley Berkeley, CA 94720 Lecture 23: Electrical

More information

Homework 2: Forces on Charged Particles

Homework 2: Forces on Charged Particles Homework 2: Forces on Charged Particles 1. In the arrangement shown below, 2 C of positive charge is moved from plate S, which is at a potential of 250 V, to plate T, which is at a potential of 750 V.

More information

NIST ELECTROSTATIC FORCE BALANCE EXPERIMENT

NIST ELECTROSTATIC FORCE BALANCE EXPERIMENT NIST ELECTROSTATIC FORCE BALANCE EXPERIMENT John A. Kramar, David B. Newell, and Jon R. Pratt National Institute of Standards and Technology, Gaithersburg, MD, USA We have designed and built a prototype

More information

UV LED charge control at 255 nm

UV LED charge control at 255 nm UV LED charge control at 255 nm Karthik Balakrishnan Department of Aeronautics and Astronautics Hansen Experimental Physics Labs Stanford University karthikb@stanford.edu Drag free concept and applications

More information

Space plasmas measurement techniques Milan Maksimovic CNRS & LESIA, Paris Observatory, France

Space plasmas measurement techniques Milan Maksimovic CNRS & LESIA, Paris Observatory, France Space plasmas measurement techniques Milan Maksimovic CNRS & LESIA, Paris Observatory, France Maksimovic : Space plasmas measurement techniques 1 ESA mission with NASA participation (launcher + two instruments)

More information

Chapter 16. Electric Energy and Capacitance

Chapter 16. Electric Energy and Capacitance Chapter 16 Electric Energy and Capacitance Electric Potential Energy The electrostatic force is a conservative force It is possible to define an electrical potential energy function with this force Work

More information

Review of Basic Electrical and Magnetic Circuit Concepts EE

Review of Basic Electrical and Magnetic Circuit Concepts EE Review of Basic Electrical and Magnetic Circuit Concepts EE 442-642 Sinusoidal Linear Circuits: Instantaneous voltage, current and power, rms values Average (real) power, reactive power, apparent power,

More information

SUPPLEMENTARY INFORMATION

SUPPLEMENTARY INFORMATION Systematic shift caused by trap asymmetry The major systematic correction in the reported cyclotron frequency ratio comparison of an antiproton at ν c, p and a negatively charged hydrogen ion (H ) at ν

More information

Chapter 19 Electric Potential and Electric Field

Chapter 19 Electric Potential and Electric Field Chapter 19 Electric Potential and Electric Field The electrostatic force is a conservative force. Therefore, it is possible to define an electrical potential energy function with this force. Work done

More information

Control of the Laser Interferometer Space Antenna

Control of the Laser Interferometer Space Antenna Control of the Laser Interferometer Space Antenna P. G. Maghami, T. T. Hyde NASA Goddard Space Flight Center Guidance, Navigation and Control Division Greenbelt, MD 20771 J. Kim Swales Aerospace, Inc.

More information

INTERNAL THALES ALENIA SPACE

INTERNAL THALES ALENIA SPACE Workshop Galileo Galilei (GG) and GGG lab prototype: state of the art and new possibilities Template reference : 100181670S-EN GG error budget from the end-to-end simulator developed at TAS-I Giuseppe

More information

SUPPLEMENTARY FIGURES

SUPPLEMENTARY FIGURES 1 SUPPLEMENTARY FIGURES Supplementary Figure 1: Schematic representation of the experimental set up. The PC of the hot line being biased, the temperature raises. The temperature is extracted from noise

More information

The Potential for Very High Frequency Gravitational Wave Science. Mike Cruise University of Birmingham GPhyS 2010 [In memory of P.

The Potential for Very High Frequency Gravitational Wave Science. Mike Cruise University of Birmingham GPhyS 2010 [In memory of P. The Potential for Very High Frequency Gravitational Wave Science Mike Cruise University of Birmingham GPhyS 2010 [In memory of P.Tourrenc] LISA, LIGO and VIRGO The obvious sources of gravitational waves

More information

MARK SCHEME for the October/November 2012 series 9702 PHYSICS

MARK SCHEME for the October/November 2012 series 9702 PHYSICS CAMBRIDGE INTERNATIONAL EXAMINATIONS GCE Advanced Subsidiary Level and GCE Advanced Level MARK SCHEME for the October/November 2012 series 9702 PHYSICS 9702/42 Paper 4 (A2 Structured Questions), maximum

More information

Review. Spring Semester /21/14. Physics for Scientists & Engineers 2 1

Review. Spring Semester /21/14. Physics for Scientists & Engineers 2 1 Review Spring Semester 2014 Physics for Scientists & Engineers 2 1 Notes! Homework set 13 extended to Tuesday, 4/22! Remember to fill out SIRS form: https://sirsonline.msu.edu Physics for Scientists &

More information

is at the origin, and charge q μc be located if the net force on q

is at the origin, and charge q μc be located if the net force on q Term: 152 Saturday, April 09, 2016 Page: 1 Q1. Three point charges are arranged along the x-axis. Charge q 3.0 0 μc 1 is at the origin, and charge q 5.0 0 μc 2 is at x = 0.200 m. Where should a third charge

More information

Large Plasma Device (LAPD)

Large Plasma Device (LAPD) Large Plasma Device (LAPD) Over 450 Access ports Computer Controlled Data Acquisition Microwave Interferometers Laser Induced Fluorescence DC Magnetic Field: 0.05-4 kg, variable on axis Highly Ionized

More information

Thermo-Elastic Distortion Modelling for Drag-Free Satellite Simulations. Draft

Thermo-Elastic Distortion Modelling for Drag-Free Satellite Simulations. Draft IN SUPREMÆ DIGNITATIS 1343 UNIVERSITÀ DI PISA Facoltà di Ingegneria Corso di Laurea in Ingegneria Aerospaziale Thermo-Elastic Distortion Modelling for Drag-Free Satellite Simulations Draft Tesi di laurea

More information

Experiment Design and Performance. G. Catastini TAS-I (BUOOS)

Experiment Design and Performance. G. Catastini TAS-I (BUOOS) Experiment Design and Performance G. Catastini TAS-I (BUOOS) 10 EP and the GRT Einstein s General Relativity Theory Weak Equivalence Principle: all test particles at the same space-time point in a given

More information

Louisiana State University Physics 2102, Exam 2, March 5th, 2009.

Louisiana State University Physics 2102, Exam 2, March 5th, 2009. PRINT Your Name: Instructor: Louisiana State University Physics 2102, Exam 2, March 5th, 2009. Please be sure to PRINT your name and class instructor above. The test consists of 4 questions (multiple choice),

More information

PHY102 Electricity Course Summary

PHY102 Electricity Course Summary TOPIC 1 ELECTOSTTICS PHY1 Electricity Course Summary Coulomb s Law The magnitude of the force between two point charges is directly proportional to the product of the charges and inversely proportional

More information

Maxwell s equations and EM waves. From previous Lecture Time dependent fields and Faraday s Law

Maxwell s equations and EM waves. From previous Lecture Time dependent fields and Faraday s Law Maxwell s equations and EM waves This Lecture More on Motional EMF and Faraday s law Displacement currents Maxwell s equations EM Waves From previous Lecture Time dependent fields and Faraday s Law 1 Radar

More information

EM Simulations using the PEEC Method - Case Studies in Power Electronics

EM Simulations using the PEEC Method - Case Studies in Power Electronics EM Simulations using the PEEC Method - Case Studies in Power Electronics Andreas Müsing Swiss Federal Institute of Technology (ETH) Zürich Power Electronic Systems www.pes.ee.ethz.ch 1 Outline Motivation:

More information

Physics (

Physics ( Question 2.12: A charge of 8 mc is located at the origin. Calculate the work done in taking a small charge of 2 10 9 C from a point P (0, 0, 3 cm) to a point Q (0, 4 cm, 0), via a point R (0, 6 cm, 9 cm).

More information

Consider a point P on the line joining the two charges, as shown in the given figure.

Consider a point P on the line joining the two charges, as shown in the given figure. Question 2.1: Two charges 5 10 8 C and 3 10 8 C are located 16 cm apart. At what point(s) on the line joining the two charges is the electric potential zero? Take the potential at infinity to be zero.

More information

NAME: PHYSICS 6B SPRING 2011 FINAL EXAM ( VERSION A )

NAME: PHYSICS 6B SPRING 2011 FINAL EXAM ( VERSION A ) NAME: PHYSCS 6B SPRNG 2011 FNAL EXAM ( VERSON A ) Choose the best answer for each of the following multiple-choice questions. There is only one answer for each. Questions 1-2 are based on the following

More information

8. (6) Consider the circuit here with resistors R A, R B and R C. Rank the

8. (6) Consider the circuit here with resistors R A, R B and R C. Rank the General Physics II Exam 2 - Chs. 18B 21 - Circuits, Magnetism, EM Induction - Oct. 3, 2013 Name Rec. Instr. Rec. Time For full credit, make your work clear. Show formulas used, essential steps, and results

More information

Introduction)! Electrostatics is the study of stationary electric charges and fields (as opposed to moving charges and currents)

Introduction)! Electrostatics is the study of stationary electric charges and fields (as opposed to moving charges and currents) Higher'Physics'1B Electricity) Electrostatics)) Introduction) Electrostatics is the study of stationary electric charges and fields (as opposed to moving charges and currents) Properties)of)Electric)Charges)

More information

7.Piezoelectric, Accelerometer and Laser Sensors

7.Piezoelectric, Accelerometer and Laser Sensors 7.Piezoelectric, Accelerometer and Laser Sensors 7.1 Piezoelectric sensors: (Silva p.253) Piezoelectric materials such as lead-zirconate-titanate (PZT) can generate electrical charge and potential difference

More information

Lions Mat. Hr. Sec. School, Paramakudi QUARTERLY KEY ANSWERS FOR PHYSICS ( ) 2. Answers written only in black (or) blue should be evaluated

Lions Mat. Hr. Sec. School, Paramakudi QUARTERLY KEY ANSWERS FOR PHYSICS ( ) 2. Answers written only in black (or) blue should be evaluated QUARTERLY KEY ANSWERS FOR PHYSICS (06-07) Note :. For answer in part II, III and IV like reasoning, explaining, narrating, describing and listing the points students may write in their own words but without

More information

Longitudinal Dynamics

Longitudinal Dynamics Longitudinal Dynamics F = e (E + v x B) CAS Bruges 16-25 June 2009 Beam Dynamics D. Brandt 1 Acceleration The accelerator has to provide kinetic energy to the charged particles, i.e. increase the momentum

More information

Gravitational Wave Astronomy Suggested readings: Camp and Cornish, Ann Rev Nucl Part Sci 2004 Schutz, gr-qc/ Kip Thorne WEB course

Gravitational Wave Astronomy Suggested readings: Camp and Cornish, Ann Rev Nucl Part Sci 2004 Schutz, gr-qc/ Kip Thorne WEB course Gravitational Wave Astronomy Suggested readings: Camp and Cornish, Ann Rev Nucl Part Sci 2004 Schutz, gr-qc/0003069 Kip Thorne WEB course http://elmer.caltech.edu/ph237/week1/week1.html L. Bergstrom and

More information

Radiative Processes in Astrophysics

Radiative Processes in Astrophysics Radiative Processes in Astrophysics 11. Synchrotron Radiation & Compton Scattering Eline Tolstoy http://www.astro.rug.nl/~etolstoy/astroa07/ Synchrotron Self-Absorption synchrotron emission is accompanied

More information

UNIVERSITY OF CAMBRIDGE INTERNATIONAL EXAMINATIONS General Certificate of Education Advanced Level

UNIVERSITY OF CAMBRIDGE INTERNATIONAL EXAMINATIONS General Certificate of Education Advanced Level www.xtremepapers.com UNIVERSITY OF CAMBRIDGE INTERNATIONAL EXAMINATIONS General Certificate of Education Advanced Level *9061759643* PHYSICS 9702/41 Paper 4 A2 Structured Questions October/November 2012

More information

Transduction Based on Changes in the Energy Stored in an Electrical Field

Transduction Based on Changes in the Energy Stored in an Electrical Field Lecture 6-1 Transduction Based on Changes in the Energy Stored in an Electrical Field Electric Field and Forces Suppose a charged fixed q 1 in a space, an exploring charge q is moving toward the fixed

More information

Acceleration Feedback

Acceleration Feedback Acceleration Feedback Mechanical Engineer Modeling & Simulation Electro- Mechanics Electrical- Electronics Engineer Sensors Actuators Computer Systems Engineer Embedded Control Controls Engineer Mechatronic

More information

Switched-Capacitor Circuits David Johns and Ken Martin University of Toronto

Switched-Capacitor Circuits David Johns and Ken Martin University of Toronto Switched-Capacitor Circuits David Johns and Ken Martin University of Toronto (johns@eecg.toronto.edu) (martin@eecg.toronto.edu) University of Toronto 1 of 60 Basic Building Blocks Opamps Ideal opamps usually

More information

Mass Analyzers. mass measurement accuracy/reproducibility. % of ions allowed through the analyzer. Highest m/z that can be analyzed

Mass Analyzers. mass measurement accuracy/reproducibility. % of ions allowed through the analyzer. Highest m/z that can be analyzed Mass Analyzers Double Focusing Magnetic Sector Quadrupole Mass Filter Quadrupole Ion Trap Linear Time-of-Flight (TOF) Reflectron TOF Fourier Transform Ion Cyclotron Resonance (FT-ICR-MS) Mass Analyzers

More information

Optics Definitions. The apparent movement of one object relative to another due to the motion of the observer is called parallax.

Optics Definitions. The apparent movement of one object relative to another due to the motion of the observer is called parallax. Optics Definitions Reflection is the bouncing of light off an object Laws of Reflection of Light: 1. The incident ray, the normal at the point of incidence and the reflected ray all lie in the same plane.

More information

Electric_Field_core_P1

Electric_Field_core_P1 Electric_Field_core_P1 1. [1 mark] An electron enters the region between two charged parallel plates initially moving parallel to the plates. The electromagnetic force acting on the electron A. causes

More information

xˆ z ˆ. A second vector is given by B 2xˆ yˆ 2z ˆ.

xˆ z ˆ. A second vector is given by B 2xˆ yˆ 2z ˆ. Directions for all homework submissions Submit your work on plain-white or engineering paper (not lined notebook paper). Write each problem statement above each solution. Report answers using decimals

More information

ELECTRICITY AND MAGNETISM, A. C. THEORY AND ELECTRONICS, ATOMIC AND NUCLEAR PHYSICS

ELECTRICITY AND MAGNETISM, A. C. THEORY AND ELECTRONICS, ATOMIC AND NUCLEAR PHYSICS UNIT 2: ELECTRICITY AND MAGNETISM, A. C. THEORY AND ELECTRONICS, ATOMIC AND NUCLEAR PHYSICS MODULE 1: ELECTRICITY AND MAGNETISM GENERAL OBJECTIVES On completion of this Module, students should: 1. understand

More information

Exam 2 Solutions. ε 3. ε 1. Problem 1

Exam 2 Solutions. ε 3. ε 1. Problem 1 Exam 2 Solutions Problem 1 In the circuit shown, R1=100 Ω, R2=25 Ω, and the ideal batteries have EMFs of ε1 = 6.0 V, ε2 = 3.0 V, and ε3 = 1.5 V. What is the magnitude of the current flowing through resistor

More information

The Engineering of LISA Pathfinder the quietest Laboratory ever flown in Space

The Engineering of LISA Pathfinder the quietest Laboratory ever flown in Space Journal of Physics: Conference Series PAPER OPEN ACCESS The Engineering of LISA Pathfinder the quietest Laboratory ever flown in Space To cite this article: Christian Trenkel et al 2017 J. Phys.: Conf.

More information

ELG4112. Electromechanical Systems and Mechatronics

ELG4112. Electromechanical Systems and Mechatronics ELG4112 Electromechanical Systems and Mechatronics 1 Introduction Based on Electromechanical Systems, Electric Machines, and Applied Mechatronics Electromechanical systems integrate the following: Electromechanical

More information

The free-fall mode experiment on LPF: first results

The free-fall mode experiment on LPF: first results The free-fall mode experiment on LPF: first results Roberta Giusteri on behalf of the LPF collaboration University of Trento and INFN-TIFPA LISA Symposium XI, 5-9 September 2016 1 LPF and actuation control

More information

Radiative Processes in Astrophysics

Radiative Processes in Astrophysics Radiative Processes in Astrophysics 9. Synchrotron Radiation Eline Tolstoy http://www.astro.rug.nl/~etolstoy/astroa07/ Useful reminders relativistic terms, and simplifications for very high velocities

More information

Progress on the Design of the Magnetic Field Measurement System for elisa

Progress on the Design of the Magnetic Field Measurement System for elisa Progress on the Design of the Magnetic Field Measurement System for elisa Ignacio Mateos Instituto de Ciencias del Espacio (CSIC-IEEC) Barcelona 10 th International LISA Symposium University of Florida,

More information

Energetic Particle Influences on the Ozonosphere mediated by the Geomagnetic Field

Energetic Particle Influences on the Ozonosphere mediated by the Geomagnetic Field Energetic Particle Influences on the Ozonosphere mediated by the Geomagnetic Field M.-B. Kallenrode University of Osnabrück, Germany Joachim Vogt, Bertalan Zieger, Int. University Bremen Anja Stadelmann,

More information

PHYS 3446 Lecture #15

PHYS 3446 Lecture #15 PHYS 3446 Lecture #15 Monday, Oct. 30, 2006 Dr. 1. Particle Accelerators Electro-static Accelerators Cyclotron Accelerators Synchrotron Accelerators 2. Elementary Particle Properties Forces and their relative

More information

Class XII Chapter 1 Electric Charges And Fields Physics

Class XII Chapter 1 Electric Charges And Fields Physics Class XII Chapter 1 Electric Charges And Fields Physics Question 1.1: What is the force between two small charged spheres having charges of 2 10 7 C and 3 10 7 C placed 30 cm apart in air? Answer: Repulsive

More information

Chapter 19. Magnetism

Chapter 19. Magnetism Chapter 19 Magnetism Magnetic Fields When moving through a magnetic field, a charged particle experiences a magnetic force This force has a maximum value when the charge moves perpendicularly to the magnetic

More information

Electric Fields Electric charges exert forces on each other when they are a distance apart. The word Electric field is used to explain this action at

Electric Fields Electric charges exert forces on each other when they are a distance apart. The word Electric field is used to explain this action at Electricity & Magnetism Electric Fields Marline Kurishingal Electric Fields Electric charges exert forces on each other when they are a distance apart. The word Electric field is used to explain this action

More information

LESSON 2 PHYSICS NOTES

LESSON 2 PHYSICS NOTES LESSON 2 ELECTROSTATIC POTENTIAL AND CAPACITANCE SECTION I ELECTROSTATIC POTENTIAL ELECTRIC FIELD IS CONSERVATIVE In an electric field work done by the electric field in moving a unit positive charge from

More information

Classical Electromagnetism

Classical Electromagnetism Classical Electromagnetism Workbook David Michael Judd Problems for Chapter 33 1.) Determine the number of electrons in a pure sample of copper if the sample has a mass of M Cu = 0.00250 kg. The molecular

More information

Explanation of dynamical Biefeld-Brown Effect from the standpoint of ZPF field

Explanation of dynamical Biefeld-Brown Effect from the standpoint of ZPF field INTERNATIONAL ACADEMY OF ASTRONAUTICS Missions to the outer solar system and beyond FIFTH IAA SYMPOSIUM ON REALISTIC NEAR-TERM ADVANCED SCIENTIFIC SPACE MISSIONS Aosta, Italy, July -4, 007 Explanation

More information

PHYSICS. Units 3 & 4 Written examination. (TSSM s 2008 trial exam updated for the current study design) SOLUTIONS. TSSM 2017 Page 1 of 1

PHYSICS. Units 3 & 4 Written examination. (TSSM s 2008 trial exam updated for the current study design) SOLUTIONS. TSSM 2017 Page 1 of 1 PHYSICS Units 3 & 4 Written examination (TSSM s 008 trial exam updated for the current study design) SOLUTIONS TSSM 017 Page 1 of 1 SECTION A - Multiple Choice (1 mark each) Question 1 Answer: D Magnetic,

More information

Ground Based Gamma Ray Astronomy with Cherenkov Telescopes. HAGAR Team

Ground Based Gamma Ray Astronomy with Cherenkov Telescopes. HAGAR Team Ground Based Gamma Ray Astronomy with Cherenkov Telescopes HAGAR Team DHEP Annual Meeting, 7-8 April, 2016 Projects : HAGAR Telescope System Development of G-APD based imaging camera Calibration device

More information

Electric Potential in a Uniform Electric Field *

Electric Potential in a Uniform Electric Field * OpenStax-CNX module: m42326 1 Electric Potential in a Uniform Electric Field * OpenStax This work is produced by OpenStax-CNX and licensed under the Creative Commons Attribution License 3.0 Abstract Describe

More information

(1) 2 amp. (2) 1 amp. (3) 0.5 amp. (4) 1.25 amp.

(1) 2 amp. (2) 1 amp. (3) 0.5 amp. (4) 1.25 amp. 1Ω + 4V 8Ω 3Ω 4Ω (1) 2 amp. (2) 1 amp. (3) 0.5 amp. (4) 1.25 amp. 8. Which is correct for inside charged sphere : (1) E 0, V = 0 (2) E=0, V= 0 (3) E 0, V 0 (4) E=0, V = 0 9. The magnetic force experienced

More information

Ultra High Energy Cosmic Rays. UHECRs from Mildly Relativistic Supernovae

Ultra High Energy Cosmic Rays. UHECRs from Mildly Relativistic Supernovae Ultra High Energy Cosmic Rays from Mildly Relativistic Supernovae Tata Institute of Fundamental Research Mumbai, India March 13, 2012 Outline UHECRS Chakraborti, Ray, Soderberg, Loeb, Chandra 2011 Nature

More information

Physics 142 Steady Currents Page 1. Steady Currents

Physics 142 Steady Currents Page 1. Steady Currents Physics 142 Steady Currents Page 1 Steady Currents If at first you don t succeed, try, try again. Then quit. No sense being a damn fool about it. W.C. Fields Electric current: the slow average drift of

More information

PHYSICS Units 3 & 4 Written examination (TSSM s 2009 trial exam updated for the current study design) SOLUTIONS

PHYSICS Units 3 & 4 Written examination (TSSM s 2009 trial exam updated for the current study design) SOLUTIONS PHYSICS Units 3 & 4 Written examination (TSSM s 009 trial exam updated for the current study design) SOLUTIONS TSSM 017 Page 1 of 1 SECTION A - Multiple Choice (1 mark each) Question 1 Answer: D ( ) (

More information

d) (6) If a third charge q = 2.0 µc is now placed 12.0 cm to the left of Q 1, what magnitude electric force will it experience?

d) (6) If a third charge q = 2.0 µc is now placed 12.0 cm to the left of Q 1, what magnitude electric force will it experience? Gen. Phys. II Exam 1 - Chs. 16,17,18A - Electric Fields, Potential, Current Sep. 12, 2013 Name Rec. Instr. Rec. Time For full credit, make your work clear. Show formulas used, essential steps, and results

More information

Current Status of Non-conservative Force Modelling:

Current Status of Non-conservative Force Modelling: Current Status of Non-conservative Force Modelling: Interface to REPRO2 Marek Ziebart, Stuart Grey and Shawn Allgeier Chair, IGS working group on Space Vehicle Orbit Dynamics Space Geodesy and Navigation

More information

Science 30 Unit C Review Outline GCCHS. Negatively charged Positively charged Coulomb Conductor Electric potential difference

Science 30 Unit C Review Outline GCCHS. Negatively charged Positively charged Coulomb Conductor Electric potential difference Science 30 Unit C Review Outline GCCHS Negatively charged Positively charged Coulomb Conductor Electric potential difference volt voltage Insulator Test body Gravitational field Field lines Solar wind

More information

ST-7 gravitational reference sensor: analysis of magnetic noise sources

ST-7 gravitational reference sensor: analysis of magnetic noise sources INSTITUTE OF PHYSICSPUBLISHING Class. Quantum Grav. 20 (2003) S109 S116 CLASSICAL ANDQUANTUM GRAVITY PII: S0264-9381(03)55737-9 ST-7 gravitational reference sensor: analysis of magnetic noise sources John

More information

Study of the very high energy gamma-ray diffuse emission in the central 200 pc of our galaxy with H.E.S.S.

Study of the very high energy gamma-ray diffuse emission in the central 200 pc of our galaxy with H.E.S.S. Study of the very high energy gamma-ray diffuse emission in the central 200 pc of our galaxy with H.E.S.S. Lemière A., Terrier R., Jouvin L., Marandon V, Lefranc V., Viana A. For the H.E.S.S. Collaboration

More information

Internal Magnetic Field Measurements and Langmuir Probe Results for the HIT-SI Experiment

Internal Magnetic Field Measurements and Langmuir Probe Results for the HIT-SI Experiment Internal Magnetic Field Measurements and Langmuir Probe Results for the HIT-SI Experiment (First Evidence of Spheromak Generation and Sustainment) Roger J. Smith Plasma Dynamics Group University of Washington,

More information

MARKING SCHEME SET 55/1/G Q. No. Expected Answer / Value Points Marks Total Marks

MARKING SCHEME SET 55/1/G Q. No. Expected Answer / Value Points Marks Total Marks MARKING SCHEME SET 55//G Q. No. Expected Answer / Value Points Marks Total Marks Set,Q Set2,Q5 Set,Q2 Set,Q2 Set2,Q4 Set,Q5 Set,Q Set2,Q2 Set,Q4 Set,Q4 Set2,Q Set,Q Set,Q5 Set2,Q Set,Q Set,Q6 Set2,Q7 Set,Q0

More information

RESISTIVE WALL MODE STABILIZATION RESEARCH ON DIII D STATUS AND RECENT RESULTS

RESISTIVE WALL MODE STABILIZATION RESEARCH ON DIII D STATUS AND RECENT RESULTS RESISTIVE WALL MODE STABILIZATION RESEARCH ON STATUS AND RECENT RESULTS by A.M. Garofalo1 in collaboration with J. Bialek,1 M.S. Chance,2 M.S. Chu,3 T.H. Jensen,3 L.C. Johnson,2 R.J. La Haye,3 G.A. Navratil,1

More information