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Seismic Design - Gemini Observatory

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<strong>Seismic</strong> <strong>Design</strong><br />

A Structural Engineering Perspective<br />

Mike Sheehan<br />

March 23, 2007<br />

MKO Earthquake Workshop


Overview<br />

• <strong>Seismic</strong> Environment Defined<br />

• <strong>Gemini</strong> Telescope <strong>Seismic</strong> <strong>Design</strong> Process<br />

• <strong>Gemini</strong> Safety Restraint Features<br />

March 23, 2007<br />

MKO Earthquake Workshop


<strong>Seismic</strong> Environment<br />

• <strong>Seismic</strong> <strong>Design</strong> Requirements<br />

– Uniform Building Code<br />

• Plus Hawaii State provisions<br />

– International Building Code<br />

– Other local codes<br />

• UBC and IBC <strong>Design</strong> Choices<br />

– Static Lateral Force Procedure<br />

– Dynamic Analysis<br />

Requirements change over time to reflect new knowledge of the<br />

seismic environments<br />

–Hawaii change from Zone 3 to Zone 4 in the late 90’s<br />

–<strong>Seismic</strong> retrofit should therefore be a big consideration for all<br />

Observatories<br />

March 23, 2007<br />

MKO Earthquake Workshop


<strong>Seismic</strong> Environment<br />

• Static Lateral Force Procedure<br />

– Peak base shear force is calculated by manipulation of loads of<br />

information including:<br />

• Soil profile type<br />

• <strong>Seismic</strong> source classification<br />

• Structural configuration<br />

• Proximity to the source<br />

• Ground response coefficients<br />

• Response spectra<br />

• Redundant load path considerations<br />

• <strong>Seismic</strong> zone factor<br />

• <strong>Seismic</strong> dead load<br />

• Fundamental period of vibration of the structure<br />

March 23, 2007<br />

MKO Earthquake Workshop


<strong>Seismic</strong> Environment<br />

• Static Lateral Force Procedure<br />

– The distribution of the base shear force throughout the structure is based<br />

upon mass and distance from the soil<br />

F 4<br />

NOT VERY GOOD FOR<br />

F<br />

LARGE 3<br />

TELESCOPE DESIGN<br />

F 2<br />

F 1<br />

h<br />

V<br />

March 23, 2007<br />

MKO Earthquake Workshop


Dynamic Analysis<br />

• Dynamic Analysis<br />

– Based upon “Appropriate Ground Motion Representation”<br />

– Performed using “Accepted Principles of Dynamics”<br />

• Ground Motion Definition<br />

– Based upon a seismic event that has a 10% probability of being exceeded<br />

in 50 years<br />

– Characterized by:<br />

• Response spectrum<br />

– Normalized spectrum defined in the codes<br />

– Site-Specific response spectrum<br />

• Representative ground motion time histories<br />

• Analysis<br />

– Three dimensional model required<br />

– Enough modes to describe total structural response<br />

March 23, 2007<br />

MKO Earthquake Workshop


Site-Specific <strong>Seismic</strong><br />

At a specific site –<br />

Hazard Analysis<br />

• The Site-Specific SHA answers the questions<br />

– What is the probability that certain ground motion criteria will occur<br />

within a given period of time?<br />

– What is the likelihood that certain seismic events will occur that will have<br />

an impact on the design of structures at a particular site.<br />

Then - with some set criteria –<br />

The SHA defines the design seismic environment in such terms that a<br />

proper structural analysis and design can proceed.<br />

March 23, 2007<br />

MKO Earthquake Workshop


History<br />

Site-Specific <strong>Seismic</strong><br />

Hazard Analysis<br />

Destructive Earthquakes in Hawaii Since 1868<br />

Date Location Magnitude<br />

28 Mar 1868 Southern Hawaii 7.0<br />

02 Apr 1868 Southern Hawaii 7.9<br />

05 Oct 1929 Hualalai 6.5<br />

21 Aug 1951 Kona 6.9<br />

26 Apr 1973 North of Hilo 6.2<br />

29 Nov 1975 Kalapana 7.2<br />

16 Nov 1983 Ka’oiki 6.7<br />

25 Jun 1989 Kalapana 6.2<br />

15 Oct 2006 Kiholo Bay 6.7<br />

March 23, 2007<br />

MKO Earthquake Workshop


Site-Specific <strong>Seismic</strong><br />

Hazard Analysis<br />

Project the Ground Motion from the Source to the Site<br />

Use of Ground Motion Attenuation Equations<br />

•Source to Site distance<br />

•Source depth<br />

•Geology and Site soil conditions<br />

•Other factors<br />

March 23, 2007<br />

MKO Earthquake Workshop


• Establish your own <strong>Design</strong> Criteria<br />

Site-Specific <strong>Seismic</strong><br />

Hazard Analysis<br />

– Codes requires that you design for the “Survival Event”<br />

• This is defined as an event that has a 10% probability of being exceeded in 50<br />

years.<br />

• In this case, structural elements are required to stay intact.<br />

• Some limited failures are expected.<br />

– At <strong>Gemini</strong>, we have looked at an “Operational Event” as well.<br />

• This was chosen to be an event that produced seismic loads at a level of 80%<br />

of the Survival Event.<br />

• In this environment, the general requirement is that the telescope recover to<br />

full operational capacity within a given (short) period of time.<br />

March 23, 2007<br />

MKO Earthquake Workshop


<strong>Design</strong> levels for Peak Ground Acceleration<br />

Site-Specific <strong>Seismic</strong><br />

Hazard Analysis<br />

Survival Event<br />

10% Probability<br />

of exceeding in 50 years<br />

Average Return Period = 500 years<br />

PGA = 0.40 g<br />

Operational Event<br />

22% Probability<br />

of exceeding in 50 years<br />

Average Return Period = 200 years<br />

PGA = 0.32 g<br />

March 23, 2007<br />

MKO Earthquake Workshop


Site-Specific <strong>Seismic</strong><br />

Hazard Analysis<br />

Horizontal Ground Motion Response Spectrum<br />

Operational Event<br />

March 23, 2007<br />

MKO Earthquake Workshop


Site-Specific <strong>Seismic</strong><br />

Hazard Analysis<br />

Horizontal Ground Motion Response Spectrum<br />

Survival Event<br />

March 23, 2007<br />

MKO Earthquake Workshop


Site-Specific <strong>Seismic</strong><br />

Hazard Analysis<br />

Vertical Ground Motion Response Spectrum<br />

Vertical Ground Motion Response Spectrum<br />

1<br />

Acceleration (g)<br />

0.1<br />

200 yr Event<br />

500 yr Event<br />

•Note that Codes typically scale the vertical<br />

response spectrum at 2/3 the horizontal<br />

spectrum. Here at 10 hz, the vertical and<br />

horizontal spectral values are equal.<br />

0.01<br />

0.01 0.1 1 10<br />

Period (sec)<br />

March 23, 2007<br />

MKO Earthquake Workshop


Site-Specific <strong>Seismic</strong><br />

Hazard Analysis<br />

• Generation of Site-Specific ground motion acceleration time<br />

history records<br />

– Use recorded ground motion records from sensors located near the site.<br />

– Calculate the response spectra based upon the measured data.<br />

– Modify the data as necessary so that the response spectra calculated from<br />

the recorded data matches that calculated for the site in the SHA<br />

March 23, 2007<br />

MKO Earthquake Workshop


Ground Motion Time Histories<br />

Site-Specific <strong>Seismic</strong><br />

Hazard Analysis<br />

Modified Mauna Loa Weather <strong>Observatory</strong> Accelerogram from 11/16/83 Earthquake<br />

D&M Data Set COMP2A<br />

0.4<br />

0.3<br />

300 o Component Acceleration (G)<br />

0.2<br />

0.1<br />

0<br />

-0.1<br />

-0.2<br />

-0.3<br />

-0.4<br />

0 5 10 15 20 25 30 35 40 45<br />

Time (sec)<br />

March 23, 2007<br />

MKO Earthquake Workshop


Comparison of October 15 th Event to <strong>Design</strong><br />

4.00E-01<br />

MK Ground Motion<br />

15 Oct 06 Earthquake<br />

3.00E-01<br />

H Comp 1<br />

Vert Comp<br />

H Comp 2<br />

<strong>Design</strong><br />

2.00E-01<br />

Acceleration (cm/sec^2)<br />

1.00E-01<br />

0.00E+00<br />

-1.00E-01<br />

-2.00E-01<br />

-3.00E-01<br />

-4.00E-01<br />

0.000 5.000 10.000 15.000 20.000 25.000 30.000 35.000 40.000 45.000<br />

Time (sec)<br />

March 23, 2007<br />

MKO Earthquake Workshop


Analysis<br />

Finite Element Model<br />

Modes sufficient to<br />

characterize the<br />

dynamic response<br />

through ~25 hz<br />

Mass and Interface<br />

Stiffness for fragile<br />

Subsystems<br />

Azimuth and Elevation<br />

Interface Stiffness<br />

Modal damping<br />

estimates are important<br />

Pier Mass<br />

Soil Stiffness<br />

March 23, 2007<br />

MKO Earthquake Workshop


Analysis<br />

Response Spectrum Analysis<br />

For each mode or interest –<br />

determine the acceleration response<br />

from the response spectrum design<br />

curve<br />

The response is shown for 5% damping.<br />

In most cases, telescope modal damping<br />

values are far less. Therefore, scale the<br />

acceleration response (up) for the<br />

appropriate level of modal damping.<br />

Combine the peak modal responses in<br />

a rational way (RSS)<br />

March 23, 2007<br />

MKO Earthquake Workshop


0.4<br />

0.3<br />

0.2<br />

0.1<br />

-0.1<br />

-0.2<br />

-0.3<br />

-0.4<br />

0<br />

0 5 1 0 1 5 2 0 2 5 3 0 3 5 4 0 4 5<br />

Analysis<br />

• Transient Analysis<br />

March 23, 2007<br />

MKO Earthquake Workshop


Analysis Results<br />

In General - Response Spectrum and Transient Analysis results<br />

should be similar<br />

• Results of interest<br />

– Global telescope structure response<br />

• High stress areas at risk of permanent deformation<br />

• Uplift<br />

– Telescope Interface Loads<br />

• Bearings, Drives, Brakes, Track & Drive Disk<br />

– Interface Loads to Fragile Subsystems<br />

– Subsystem rigid body (or elastic) response<br />

• Provide seismic design requirements for subsystems<br />

March 23, 2007<br />

MKO Earthquake Workshop


<strong>Seismic</strong> Restraints<br />

• Process<br />

– Identify fragile sub-systems<br />

– Assess Sub-system response in both Survival and Operational <strong>Seismic</strong><br />

Environments<br />

– Address the fragility level of the sub-system to the seismic response<br />

– Define the need for seismic restraints on these subsystems<br />

– <strong>Design</strong> these sub-system restraints<br />

OR<br />

– Calculate the sub-system design environments<br />

– Impose these environments as a part of design specifications<br />

March 23, 2007<br />

MKO Earthquake Workshop


<strong>Seismic</strong> Restraints<br />

M2 Followers<br />

M1 Safety Restraint System<br />

<strong>Seismic</strong> Restraints<br />

on Az and El axes<br />

March 23, 2007<br />

MKO Earthquake Workshop


<strong>Seismic</strong> Restraints<br />

Telescope Overturning Restraints<br />

March 23, 2007<br />

MKO Earthquake Workshop


<strong>Seismic</strong> Restraints<br />

• M1 Restraint System<br />

March 23, 2007<br />

MKO Earthquake Workshop


Conclusion<br />

• Analysis/<strong>Design</strong> Process<br />

– Good for assessment of current design<br />

– <strong>Seismic</strong> retrofit<br />

• Applies to Telescopes in particular, but in general<br />

– Enclosures<br />

– Support Facilities<br />

– Piping systems<br />

– Tanks<br />

– Book cases<br />

Any structure at risk of damage resulting from<br />

being subjected to the effects of a seismic event<br />

March 23, 2007<br />

MKO Earthquake Workshop

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