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Featured researches published by B. C. Bruno.


Journal of Geophysical Research | 1996

Modeling gravity-driven flows on an inclined plane

B. C. Bruno; Stephen M. Baloga; G. Jeffrey Taylor

We develop an exact analytic solution for unconfined flows having an assumed rheology advancing on an inclined plane. We consider the time-dependent flow movement to be driven by gravitational transport and hydrostatic pressure. We examine how these two forces drive flow movement in the downstream and cross-stream directions by adopting a volume conservation approach. Simplifying assumptions reduce the governing equation to the dimensionless form ∂/∂x(αhm) = ∂/∂y(αhm∂h/∂y), where x and y are the downstream and cross-stream directions, respectively; h is the flow depth; and α = α(x) and m are prescribed by the rheology of the fluid. We solve this equation analytically for flows of arbitrary m and α using a similarity transformation. This method involves transforming variables and reducing the governing equation to a nonlinear ordinary differential equation. Our solution determines how flow depth and width change with distance from the source of the flow for different α and m based on known or assumed initial parameters. Consequently, from the traditional geometric dimensions of the deposits, these rhelogical parameters can be inferred. We have applied the model to basaltic lava flows and found m values typically between 1 and 2. This contrasts with Newtonian fluids, for which m = 3. The model of α(x) corresponding to constant viscosity approximates the field data of pahoehoe toes (<5 meters in length), whereas models of α(x) corresponding to linearly increasing and exponentially increasing viscosities better approximate the remote sensing data of longer flows (several kilometers in length).


Geophysical Research Letters | 1992

Lava flows are fractals

B. C. Bruno; G. J. Taylor; Scott K. Rowland; Paul G. Lucey; Stephen Self


Planetary and Space Science | 2009

Mesoscale raised rim depressions (MRRDs) on Earth: A review of the characteristics, processes, and spatial distributions of analogs for Mars

Devon M. Burr; B. C. Bruno; Peter D. Lanagan; Lori S. Glaze; Windy L. Jaeger; Richard J. Soare; Jean-Michel Wan Bun Tseung; James A. Skinner; Stephen M. Baloga


Journal of Geophysical Research | 2007

Nearest‐neighbor analysis of small features on Mars: Applications to tumuli and rootless cones

Stephen M. Baloga; Lori S. Glaze; B. C. Bruno


Geophysical Research Letters | 1995

Morphologic identification of Venusian lavas

B. C. Bruno; G. Jeffrey Taylor


Archive | 1993

Fractal dimensions of rampart impact craters on Mars

Delwyn Ching; G. Jeffrey Taylor; Peter J. Mouginis-Mark; B. C. Bruno


Archive | 1994

Slow Emplacement of Flood Basalts: Evidence from Fractal Properties of Lava Flows

G. Jeffrey Taylor; B. C. Bruno; Stephen Self


Archive | 1995

Morphologic Identification of Venusian Lavas: Implications for Emplacement of Long Lava Flows

B. C. Bruno; G. Jeffrey Taylor


Archive | 1992

The Character of Lava Flow Margins

Stephen M. Baloga; G. Jeffrey Taylor; B. C. Bruno


Archive | 2005

Physical Characteristics and Processes of 100-m-scale raised-rim depressions (RRD's) on Earth: application to Mars

Devon M. Burr; B. C. Bruno; Windy L. Jaeger; Peter Denham Lanagan; Hiroko Miyamoto; Richard J. Soare; J.-M. Wan Bun Tseung

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Stephen M. Baloga

California Institute of Technology

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Lori S. Glaze

Goddard Space Flight Center

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Paul G. Lucey

University of Hawaii at Manoa

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James A. Skinner

United States Geological Survey

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