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Affiliate Faculty (Associate Specialist at C-MORE, SOEST)
Email: barb@hawaii.edu
Office: HIG 214
Phone Number: (808) 956-0901
Fax Number: (808) 956-5524
University of Hawai'i at Manoa
Center for Microbial Oceanography: Research and Education
Department of Oceanography-SOEST
1000 Pope Road
Honolulu, HI 96822
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Research Interests:
(C-MORE, SOEST) Science education
Relevant
Links:
Publications
(partial listing):
Bruno B.C., Fagents S.A., Hamilton C., Burr D., Baloga S.D. (2006) Identification of volcanic rootless cones and ice mounds on Earth and Mars: using spatial distribution as a remote sensing tool JGR-Planets (in press)
Baloga S.M. and Bruno B.C. (2005) The origin of transverse ridges on the surfaces of catastrophic mass flow deposits on the Earth and Mars. JGR-Planets 110, E05007, doi:10.1029/2004JE002381.
Bruno B.C., Fagents S.A., Thordarson T., Baloga S.M., and Pilger E.J. (2004) Clustering within rootless cone groups on Iceland and Mars: Effect of nonrandom processes. J. Geophys. Res. 109, doi:10.1029.2004JE002273.
Bruno B.C., Baloga S.M., and Taylor G.J. (1996) Modeling gravity-driven flows on an inclined plane. J. Geophys. Res., 101, No. B5, 11,565-11,577.
Bruno B.C. and Taylor G.J. (1995) Morphologic identification of Venusian lavas. Geophys. Res. Lett.
Bruno B.C., Taylor G.J., Rowland S.K., and Baloga S.M. (1994) Quantifying the effect of rheology and lava-flow margins using fractal geometry. Bull. Volcanol., 56, 193-206.
Bruno B.C., Taylor G.J., Rowland S.K., Lucey P.G., and Self S. (1992) Lava flows are fractals. Geophys. Res. Lett., 19, 3, 305-308.
Bruno B.C. High resolution ultraviolet-visible spectroscopy of lunar red spots, 1990, Masters Thesis, University of Hawaii, December,
Bruno B.C., Lucey P.G. and Hawke B.R. (1991) High resolution UV-visible spectroscopy of lunar red spots, Proc. Lunar Planet. Sci. Conf. XXI, Lunar Planet. Inst., Houston, TX, P. 405-415.
Lucey P.G., Bruno B.C, and Hawke B.R. (1991) Preliminary results of imaging spectroscopy of the Humorum Basin region of the moon. Proc. Lunar Planet. Sci. Conf. XXI, P. 391-403.
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