CaltechAUTHORS
  A Caltech Library Service

Asymmetric P′P′: An alternative to P′dP′ reflections in the uppermost mantle (0 to 110 km)

Whitcomb, James H. (1973) Asymmetric P′P′: An alternative to P′dP′ reflections in the uppermost mantle (0 to 110 km). Bulletin of the Seismological Society of America, 63 (1). pp. 133-143. ISSN 0037-1106. https://resolver.caltech.edu/CaltechAUTHORS:20140812-122837796

[img]
Preview
PDF - Published Version
See Usage Policy.

882kB
[img]
Preview
PDF (Discussion) - Published Version
See Usage Policy.

173kB

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20140812-122837796

Abstract

Precursors to P′P′ (PKPPKP), first interpreted as sub-surface reflections by Gutenberg in 1960 and studied in several later papers by other authors, precede the P′P′ phase by up to 200 sec. This phase, designated P′dP′ where d is the depth of reflection, has unique potential for giving new details of upper-mantle structure. However, as with any newly discovered seismic phase, the uniqueness of its interpretation must be well established. Asymmetric P′P′ phases reflecting from surface or near-surface dipping interfaces pose a challenge to this uniqueness because of their maximum-time nature. Simplified estimates of the amplitudes of asymmetric P′P′ rays are made, including consideration of the relative amplitudes of core phases and the finiteness of the reflecting surfaces of dipping interfaces. These estimates lead to the conclusion that the reading of asymmetric P′P′ at a single station is likely only in the 0- to 30-sec range before the main symmetric P′P′ phase. However, if array beam-forming is used, this range is reduced to 0 to 10 sec. The data indicate that both P′dP′ and asymmetric P′P′ are present at up to 30 sec lead time and array beam-forming is needed to differentiate between the two. A further effect of the maximum-time nature of P′P′ is that, in practice, the geographic location of the reflection point can be determined to within only a few degrees.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://bssa.geoscienceworld.org/content/63/1/133.abstractPublisherArticle
http://bssa.geoscienceworld.org/content/64/3-1/725.full.pdf+htmlPublisherDiscussion
Additional Information:Copyright © 1973, by the Seismological Society of America. Manuscript received May 15, 1972. I am grateful to Paul G. Richards for valuable discussions and to Don L. Anderson for a critical reading of the manuscript. This work was partially supported by the Advanced Research Projects Agency of the Department of Defense and was monitored by the Air Force Office of Scientific Research under Contracts F44620-69-C-0067 and F44620-72-C-0078. During the course of the work, the author was supported by the California Institute of Technology Gutenberg Fellowship.
Funders:
Funding AgencyGrant Number
Advanced Research Projects Agency (ARPA)UNSPECIFIED
Air Force Office of Scientific Research (AFOSR)F44620-69-C-0067
Air Force Office of Scientific Research (AFOSR)F44620-72-C-0078
Caltech Beno Gutenberg FellowshipUNSPECIFIED
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Caltech Division of Geological and Planetary Sciences2179
Caltech Division of Geological and Planetary Sciences2432
Issue or Number:1
Record Number:CaltechAUTHORS:20140812-122837796
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20140812-122837796
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:48391
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:12 Aug 2014 22:50
Last Modified:03 Oct 2019 07:03

Repository Staff Only: item control page