inertial sensor development for a 1 tev linear collider

1
Inertial Sensor Development for a 1 TeV Linear Collider Eric Doyle, Josef Frisch, Linda Hendrickson, Thomas Himel, Thomas Markieweicz, Justin May, Richard Partridge, Andrei Seryi Work Supported by Department of Energy Contract DE-AC03-76SF0515 Requirements Noise: < 1 nanometer integrated above 1Hz. Frequency response: 0.1Hz to 50Hz. Must operate in 1 Tesla magnetic field Compact - ~20×20×10 cm The proposed 1 TeV X-band electron / positron linear collider will produce beams with approximately 1 nanometer vertical sizes at the collision point. The final focusing magnets for this accelerator must be held relative to each other at the nanometer level. Beam – Beam interactions provide a signal for a high gain feedback for frequencies below ~1Hz, but additional stabilization is required at higher frequencies. One option is to use inertial sensors (geophones) to provide a feedback signal. Technology: RF capacitive position sensing Position feedback through DSP Feedback force -> measured acceleration BeCu spring, Ceramic moving parts Parameters Test mass 40 grams Suspension frequency 1.5Hz Mechanical Q >100 Theoretical thermal mechanical noise <1.5×10 -10 M/s 2 /Hz 1/2 . Capacitor Sensor gap ~300 microns Theoretical thermal electronic noise < thermal noise Vacuum <few microns Prototype sensor Technical Issues: Creep Spring must be operated at high stress to maximize unwanted 2 nd mode frequency (from ANSYS simulations) Lifetime of sensor limited by creep of spring. Tests at design 75% of yield stress give creep life >20 years. Creep chart Technical Issues: Magnetic sensitivity Housing, fixed supports : Non-magnetic stainless, Aluminum Motor: (for creep / temperature compensation) Piezoelectric motor (Picomotor TM ), nonmagnetic in final system Cantilever : Prototype uses Aluminum cantilever. (conductor: dB/dt problem) Final version uses Aluminum Oxide cantilever Mass : Tungsten in prototype (magnetic in first prototype!) Final version: HfO 2 9.8g/cc, (heaviest non-radioactive ceramic) Technical Issues: Creak High spring stress can produce creak Also ,early prototype had problems with creak in support components (support position pot) 75% y.p. springs: flat (ch4) & pre-bent (ch6) displ. vs ti compared to max and min predicted rates 0 0.02 0.04 0.06 0.08 0.1 0.12 0.14 0.16 0.18 0.2 0 200 400 600 800 1000 elapsed time (days) pre-bent flat min rate max rate Technical Issues: Temperature Sensitivity Non-magnetic requirement prevents the use of temperature compensated spring materials. Calculated temperature sensitivity ~.01 M/s 2 / °C, 10 nano-degree temperature variation (during measurement time) would limit resolution. Design incorporates multiple thermal filters, gold plating for radiation shielding. Temperature variations probably major noise source below 0.1Hz. Future Work: Test in quiet location Install fully non-magnetic components Try reduced spring stress to reduce crea Add temperature stabilization Preliminary Data – not verified! Initial testing of sensor vs. Strekheisen STS-2. Testing done in noisy lab environment: high Frequency noise (5-100Hz) exceeds sensor feedback actuator strength. Noise floor <~10 -8 m/s 2 /sqrt(Hz) Noise 1/f corner ~0.1Hz.

Upload: cade-mcfadden

Post on 02-Jan-2016

22 views

Category:

Documents


0 download

DESCRIPTION

- PowerPoint PPT Presentation

TRANSCRIPT

Page 1: Inertial Sensor Development for a 1 TeV Linear Collider

Inertial Sensor Development for a 1 TeV Linear Collider

Eric Doyle, Josef Frisch, Linda Hendrickson, Thomas Himel, Thomas Markieweicz, Justin May, Richard Partridge, Andrei SeryiWork Supported by Department of Energy Contract DE-AC03-76SF0515

Requirements

Noise: < 1 nanometer integrated above 1Hz.Frequency response: 0.1Hz to 50Hz. Must operate in 1 Tesla magnetic fieldCompact - ~20×20×10 cm

The proposed 1 TeV X-band electron / positron linear collider will produce beams with approximately 1 nanometer vertical sizes at the collision point. The final focusing magnets for this accelerator must be held relative to each other at the nanometer level. Beam – Beam interactions provide a signal for a high gain feedback for frequencies below ~1Hz, but additional stabilization is required at higher frequencies. One option is to use inertial sensors (geophones) to provide a feedback signal.

Technology:

RF capacitive position sensingPosition feedback through DSPFeedback force -> measured accelerationBeCu spring, Ceramic moving parts

Parameters

Test mass 40 gramsSuspension frequency 1.5HzMechanical Q >100Theoretical thermal mechanical noise <1.5×10-10M/s2/Hz1/2.Capacitor Sensor gap ~300 micronsTheoretical thermal electronic noise < thermal noiseVacuum <few microns

Prototype sensor

Technical Issues: Creep

Spring must be operated at high stress to maximize unwanted 2nd mode frequency (from ANSYS simulations)

Lifetime of sensor limited by creep of spring. Tests at design 75% of yield stress give creep life >20 years.

Creepchart

Technical Issues: Magnetic sensitivity

Housing, fixed supports:Non-magnetic stainless, Aluminum

Motor: (for creep / temperature compensation)Piezoelectric motor (PicomotorTM), nonmagnetic in final system

Cantilever: Prototype uses Aluminum cantilever. (conductor: dB/dt problem)Final version uses Aluminum Oxide cantilever

Mass:Tungsten in prototype (magnetic in first prototype!)Final version: HfO2 9.8g/cc, (heaviest non-radioactive ceramic)

Technical Issues: Creak

High spring stress can produce creak

Also ,early prototype had problems with creak in support components (support position pot)

75% y.p. springs: flat (ch4) & pre-bent (ch6) displ. vs timecompared to max and min predicted rates

00.020.040.060.080.1

0.120.140.160.180.2

0 200 400 600 800 1000

elapsed time (days)

displacement (in)

pre-bent

flat

min rate

max rate

Technical Issues: Temperature Sensitivity

Non-magnetic requirement prevents the use of temperaturecompensated spring materials.

Calculated temperature sensitivity ~.01 M/s2 / °C,10 nano-degree temperature variation (during measurement time) would limit resolution.

Design incorporates multiple thermal filters, gold plating for radiation shielding.

Temperature variations probably major noise source below 0.1Hz.

Future Work:

Test in quiet locationInstall fully non-magnetic componentsTry reduced spring stress to reduce creak.Add temperature stabilization

Preliminary Data – not verified!

Initial testing of sensor vs. Strekheisen STS-2. Testing done in noisy lab environment: high Frequency noise (5-100Hz) exceeds sensor feedback actuator strength.

Noise floor <~10-8m/s2/sqrt(Hz)Noise 1/f corner ~0.1Hz.