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principles and applications of microearthquake networks

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6.1. Determination <strong>of</strong> Origin Time <strong>and</strong> Hypocenter 13 1<br />

tion, <strong>and</strong> the z axis is along the vertical direction pointing downward. Any<br />

position on earth may be specified by latitude 6, longitude A, <strong>and</strong> elevation<br />

above sea level h. If the position is between 70"N <strong>and</strong> 70"s in latitude, it<br />

may be converted to (x, y, z) with respect to the coordinate origin at<br />

latitude bo, longitude A,, <strong>and</strong> elevation at sea level by a method described<br />

by Richter (1958, pp. 701-703, as<br />

(6.2)<br />

x = 60*A(h - A,), y = 60-B($ - 40)<br />

i = -0.001h<br />

where x, y, <strong>and</strong> z are in kilometers, A. A,, 4, <strong>and</strong> 4, are given in degrees,<br />

<strong>and</strong> h is given in meters. Values for A <strong>and</strong> B may be derived from Woodward<br />

(1929)<br />

(6.3)<br />

A ~(1.8553654<br />

+ 0.0062792 sin2@ + 0.0000319 sin4@)cos@<br />

B = 1.8428071 + 0.0187098 sin2@ + 0.0001583 sin4@<br />

where @ = $(+ + 4,) <strong>and</strong> is given in degrees.<br />

In the earthquake location problem, we are concerned with a fourdimensional<br />

space: the time coordinate t, <strong>and</strong> the spatial coordinates x, y,<br />

<strong>and</strong> z. A vector in this space may be written as<br />

(6.4)<br />

x = (t, .Y, y. z)T<br />

where the superscript T denotes the transpose. In Chapter 5, we used x to<br />

denote a vector in an n-dimensional Euclidean space in which the coordinates<br />

are x,. x2, . . . , x,. Since it is common to denote the spatial coordinates<br />

by x, y, <strong>and</strong> i, we have changed our notation here. Furthermore, the<br />

subscript k <strong>of</strong> the coordinates is now used to index the observation made<br />

at the kth station.<br />

To locate an earthquake using a set <strong>of</strong> arrival times 7k from stations at<br />

positions (xk, yk, zk), k = 1, 19 7 . . . . rn. we must first assume an earth<br />

model in which theoretical travel times Tk from a trial hypocenter at<br />

position (x", y* , z* 1 to the stations can be computed. Let us consider a<br />

given trial origin time <strong>and</strong> hypocenter as a trial vector x* in a fourdimensional<br />

Euclidean space<br />

(6.5) x* = (I*. .v*. ),* .-*)'I.<br />

Theoretical arrival time fk from x* to the kth station is the theoretical<br />

travel time Tk plus the trial origin time t", or<br />

(6.6) tk(X*) = Tk(x*) + t*<br />

Strictly speaking, Tk does not depend on t", but we express Tk as ak(x")<br />

for convenience in notation.<br />

for<br />

k = 1, 2. . . . , rn

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