Journal article
The rupture extent of low frequency earthquakes near Parkfield, CA
- Abstract:
-
The low frequency earthquakes (LFEs) that constitute tectonic tremor are often inferred to be slow: to have durations of 0.2 to 0.5 s, a factor of 10 to 100 longer than those of typical MW 1-2 earthquakes. Here we examine LFEs near Parkfield, CA in order to assess several proposed explanations for LFEs’ long durations. We determine LFE rupture areas and location distributions using a new approach, similar to directivity analysis, where we examine how signals coming from various locations with...
Expand abstract
- Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Accepted Manuscript
Actions
Access Document
- Files:
-
-
(pdf, 3.4MB)
-
- Publisher copy:
- 10.1093/gji/ggy429
Why is the content I wish to access not available via ORA?
Bibliographic data (the information relating to research outputs) and full-text items (e.g. articles, theses, reports, etc.) arrive in ORA from several different sources. Unfortunately we are not able to make available the full-text for every research output.
Please contact the ORA team (
) if you have queries regarding unavailable content OR if you are aware of a full-text copy we can make available.
) if you have queries regarding unavailable content OR if you are aware of a full-text copy we can make available.
Content may be unavailable for the following four reasons
-
Version unsuitable
-
We have not obtained a suitable full-text for a given research output. See this page for more information.
-
Recently completed
-
Sometimes content is held in ORA but is unavailable for a fixed period of time to comply with the policies and wishes of rights holders.
-
Permissions
-
All content made available in ORA should comply with relevant rights, such as copyright. See this page for more information.
-
Clearance
-
Some thesis volumes scanned as part of the digitisation scheme funded by Dr Leonard Polonsky are currently unavailable due to sensitive material or uncleared third-party copyright content. We are attempting to contact authors whose theses are affected.
Alternative access to the full-text
You may be able to access the full-text directly from the publisher's website using the 'Publisher Copy' link in the 'Links & Downloads' box from a research output's ORA record page. This method may require an institutional or individual subscription to the journal/resource.
Authors
Bibliographic Details
- Publisher:
- Oxford University Press Publisher's website
- Journal:
- Geophysical Journal International Journal website
- Volume:
- 216
- Issue:
- 1
- Pages:
- 621–639
- Publication date:
- 2018-10-13
- Acceptance date:
- 2018-10-11
- DOI:
- EISSN:
-
1365-246X
- ISSN:
-
0956-540X
- Pubs id:
-
pubs:929744
- URN:
-
uri:8ba9c4a5-63e3-4642-a779-d96e013d18c9
- UUID:
-
uuid:8ba9c4a5-63e3-4642-a779-d96e013d18c9
- Local pid:
- pubs:929744
Item Description
Terms of use
- Copyright holder:
- Hawthorne et al.
- Copyright date:
- 2018
- Notes:
-
Copyright © 2018 The Authors. Published by Oxford University Press on behalf of The Royal Astronomical Society. This is the accepted manuscript version of the article. The final version is available online from Oxford University Press at: https://doi.org/10.1093/gji/ggy429
If you are the owner of this record, you can report an update to it here: Report update to this record