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Download Volume II Accomplisments (28 Mb pdf). - IRIS

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From an <strong>IRIS</strong> Lecture Tour to a General Audience Book About<br />

Midwest Earthquakes<br />

Seth Stein (Northwestern University)<br />

Following earthquakes of public interest, seismologists<br />

are effective at explaining to the media about<br />

the earthquake’s location, magnitude, and tectonic<br />

setting. However, the underlying research questions<br />

are typically not discussed, in part owing to the challenge<br />

of explaining ongoing and unresolved scientific<br />

questions. As a result, we often do not show the<br />

public the challenges and complexities of earthquake<br />

research. An exception is <strong>IRIS</strong>/SSA Distinguished<br />

Lectures, which give the speaker the motivation and<br />

time to explain earthquake research in some depth.<br />

In 2006 I gave <strong>IRIS</strong>/SSA lectures on "Giant earthquakes:<br />

Why, Where, When, and What We Can<br />

Do” at a number of science museums. Although the<br />

focus was on the largest earthquakes, the lecture also<br />

explained general concepts of plate tectonics, earthquakes,<br />

seismology, and earthquake hazards. Giving<br />

the lectures was interesting and satisfying, and indicated<br />

that the material could be presented using an<br />

approach that focused on the key ideas and unresolved<br />

issues. Based on this experience, I have incorporated<br />

much of this material in a new book written<br />

for a non-technical audience: “Disaster Deferred:<br />

How new science is changing our view of earthquake<br />

hazards in the Midwest” that will be published in fall<br />

2010 by Columbia University Press.<br />

“Disaster Deferred: How new science is changing our view of earthquake hazards in the<br />

Midwest” will be published in fall 2010 by Columbia University Press.<br />

2010 <strong>IRIS</strong> Core Programs Proposal | <strong>Volume</strong> <strong>II</strong> | education and outreach | <strong>II</strong>-29

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