ML20234F443

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Informs That by End of Wk,All Modified Illustrations to Be Completed.Forwards Results on El Centro Analysis,Per Discussion of Resultant Accelerations & Velocities at Last Meeting.Illustrations to Be Included in Final Rept
ML20234F443
Person / Time
Site: 05000000, Bodega Bay
Issue date: 07/10/1963
From: Neumann F
WASHINGTON, UNIV. OF, SEATTLE, WA
To: Bryan R
US ATOMIC ENERGY COMMISSION (AEC)
Shared Package
ML20234A767 List: ... further results
References
FOIA-85-665 NUDOCS 8709230123
Download: ML20234F443 (3)


Text

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dg 121963m Ama July 10, 19 Lf4 j g %rTTGV Dr. Robert H. Bryan, '

Division of Licensing and Regulation, U. S. Atonio Energy Commission, Washington 25, D.C.

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Dear Dr. Bryan:

This is a kind of progress report. By the end of this week I expect to have all of the modified illustrations comt plated; it is a tedious and time consuming job. I have looked further into the magnitude-intensity relationship and, in place I of the simple relationship suggested by Gutenberg-Richter, have come up with a much more informative type of chart which will do as much as anything else to prove that the epicentral intensity in 1906 was n-10 rather than anything less. . ]

1 I have not had time to review the paper {passed out by Hous- ]

nor and Tocher at the Argonne Laboratory but hope to do so as j soon as the illustrations are finished. .

In connection with the discussion of resultant accelerations j and velocities at the last meeting there are onolosed some results l 1

that I published in the 1940 Seismological Report of the Coast j and Geodetic Survey on the El Centro andysis. This solution did 1 l not take into account the fact that there was some permanent dis-placement during the first few seconds of recording but I do not

- think this would make much difference in the over all picture. l Perhaps this illustration should be included in my final report.

Eineerelyyou2s, .

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Frank Neumann.

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ima. of the major displacements rather than details needed to make eparison studw of the various graphs.

W maximum displacement is about 21 centimeters. The period is we shown on the longitudinal component and may be taken as 3.2

-unds. The corresponding velocity would le about 42 cm./sec.

mhich ties in well with the general range of velocities at the start of

} the resultant velocity curw. The corresponding acceleration would be about 80 cm. This is about one. fourth ihe amplitude of the 5  ; euperposed shor/sec."t period accelerations inspection of the acceleration curves. , a ratio which is borne out by

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!2" Fertical motion.-No attempt was made to combine the vertical motion with the horizontal to determine the natun of the vertical 1 - motion relative to the horizontal. An inspection of the noceleration l moord shows little tendency for the period to deviate widely from 0.10 second.. In the early part cf the mcord there are a number of I

turning points indicating periods u low as 0.03 second but they' seem insigmficant. The maximum vertical sooeleration 0.8 second after the start of the moont is about 990 cm.

period of 0.109 second. Freen the res/sec.8, and is,neociated with a ultant horizontal acceleration graph it will be noted that this occum while the horisontal semiera.

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