Cookies

We use cookies to ensure that we give you the best experience on our website. By continuing to browse this repository, you give consent for essential cookies to be used. You can read more about our Privacy and Cookie Policy.


Durham Research Online
You are in:

Fan‐surface evidence for debris‐flow avulsion controls and probabilities, Saline Valley, California.

Haas, T. and Densmore, A. L. and Hond, T. and Cox, N. J. (2019) 'Fan‐surface evidence for debris‐flow avulsion controls and probabilities, Saline Valley, California.', Journal of geophysical research : earth surface., 124 (5). pp. 1118-1138.

Abstract

Debris‐flow fans form by shifts of the active channel, termed avulsions. Field and experimental evidence suggest that debris‐flow avulsions may be induced by depositional lobes that locally plug a channel or super‐elevation of the channel bed above the surrounding fan surface, by analogy to fluvial fans. To understand debris‐flow avulsion processes, we differentiate between these controls by quantifying the spatial distribution of debris‐flow lobe and channel dimensions, along with channel‐bed super‐elevation, on nine debris‐flow fans in Saline Valley, California, USA. Channel beds are generally super‐elevated by 2‐5 channel depths above the fan surface, and locally by more than 7 channel depths, thereby substantially exceeding super‐elevation on fluvial fans. Depositional‐lobe thickness and channel depth decrease with distance from the fan apex, although both are highly variable across the fans. Median channel depths roughly correspond to the 50‐75th percentiles of lobe thicknesses, while minimum channel depths roughly correspond to the 10‐25th percentiles. In contrast, the thicknesses of lobes that have triggered avulsions roughly equal local channel depths and are on average twice as thick as the local median lobe thickness. The spatial correspondence between avulsion locations and thick lobe deposits, and the lack of correlation with channel‐bed super‐elevation, leads us to infer that avulsions on these fans are mostly caused by thick lobes forming channel plugs. Although results may vary with climatic and tectonic setting, our findings indicate that avulsion hazard assessment on populated fans should include mapping and monitoring of channel depths relative to typical deposit thicknesses on a given fan.

Item Type:Article
Full text:Publisher-imposed embargo
(AM) Accepted Manuscript
File format - PDF
(37121Kb)
Full text:(VoR) Version of Record
Available under License - Creative Commons Attribution Non-commercial No Derivatives.
Download PDF
(8873Kb)
Status:Peer-reviewed
Publisher Web site:https://doi.org/10.1029/2018JF004815
Date accepted:30 March 2019
Date deposited:09 April 2019
Date of first online publication:07 May 2019
Date first made open access:25 June 2019

Save or Share this output

Export:
Export
Look up in GoogleScholar