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Assessment of estuarine water-quality indicators using MODIS medium-resolution bands: initial results from Tampa Bay, FL Assessment of estuarine water-quality indicators using MODIS medium-resolution bands: initial results from Tampa Bay, FL

Using Tampa Bay, FL as an example, we explored the potential for using MODIS medium-resolution bands (250- and 500-m data at 469-, 555-, and 645-nm) for estuarine monitoring. Field surveys during 21–22 October 2003 showed that Tampa Bay has Case-II waters, in that for the salinity range of 24–32 psu, (a) chlorophyll concentration (11 to 23 mg m−3), (b) colored dissolved organic matter...
Authors
Chuanmin Hu, Zhiqiang Chen, Tonya Clayton, Peter Swarzenski, John Brock, Frank Muller-Karger

Holocene reef development where wave energy reduces accommodation Holocene reef development where wave energy reduces accommodation

Analyses of 32 drill cores obtained from the windward reef of Kailua Bay, Oahu, Hawaii, indicate that high wave energy significantly reduced accommodation space for reef development in the Holocene and produced variable architecture because of the combined influence of sea-level history and wave exposure over a complex antecedent topography. A paleostream valley within the late...
Authors
Eric E. Grossman, Charles H. Fletcher

[Book review] Sea level rise: history and consequences [Book review] Sea level rise: history and consequences

Review of: Sea level Rise: history and consequences. Bruce Douglas, Michael S. Kearney and Stephen P. Leatherman (eds), Sand Diego: Academic Press, 2001, 232 pp. plus CD-RIM, US$64.95, hardback. ISBN 0-12-221345-9.
Authors
Eric E. Grossman

Textures of the soils and rocks at Gusev Crater from Spirit’s Microscopic Imager Textures of the soils and rocks at Gusev Crater from Spirit’s Microscopic Imager

The Microscopic Imager on the Spirit rover analyzed the textures of the soil and rocks at Gusev crater on Mars at a resolution of 100 micrometers. Weakly bound agglomerates of dust are present in the soil near the Columbia Memorial Station. Some of the brushed or abraded rock surfaces show igneous textures and evidence for alteration rinds, coatings, and veins consistent with secondary
Authors
Kenneth Herkenhoff, S. Squyres, R. Arvidson, D.S. Bass, J. Bell, P. Bertelsen, N.A. Cabrol, Lisa Gaddis, A. Hayes, S.F. Hviid, J. Johnson, K.M. Kinch, M.B. Madsen, J.N. Maki, S. McLennan, H.Y. McSween, J. Rice, M. Sims, P. Smith, Laurence Soderblom, Nicole Spanovich, R. Sullivan, A. Wang

Magnetic properties experiments on the Mars Exploration Rover Spirit at Gusev Crater Magnetic properties experiments on the Mars Exploration Rover Spirit at Gusev Crater

The magnetic properties experiments are designed to help identify the magnetic minerals in the dust and rocks on Mars—and to determine whether liquid water was involved in the formation and alteration of these magnetic minerals. Almost all of the dust particles suspended in the martian atmosphere must contain ferrimagnetic minerals (such as maghemite or magnetite) in an amount of ∼2% by...
Authors
P. Bertelsen, W. Goetz, M.B. Madsen, K.M. Kinch, S.F. Hviid, J. Knudsen, H.P. Gunnlaugsson, J. Merrison, P. Nornberg, S. Squyres, J. Bell, Kenneth Herkenhoff, S. Gorevan, A. Yen, T. Myrick, G. Klingelhoefer, R. Rieder, R. Gellert

Using twelve years of USGS refraction lines to calibrate the Brocher and others (1997) 3D velocity model of the Bay Area Using twelve years of USGS refraction lines to calibrate the Brocher and others (1997) 3D velocity model of the Bay Area

Campbell (1983) demonstrated that site amplification correlates with depths to the 1.0, 1.5, and 2.5 km/s S-wave velocity horizons. To estimate these depths for the Bay Area stations in the PEER/NGA database, we compare the depths to the 3.2 and 4.4 km/s P-wave velocities in the Brocher and others (1997) 3D velocity model with the depths to these horizons determined from 6 refraction...
Authors
John Boatwright, Luke Blair, Rufus Catchings, Mark Goldman, Fabio Perosi, Clare Steedman

The Alaska Volcano Observatory - Expanded monitoring of volcanoes yields results The Alaska Volcano Observatory - Expanded monitoring of volcanoes yields results

Recent explosive eruptions at some of Alaska's 52 historically active volcanoes have significantly affected air traffic over the North Pacific, as well as Alaska's oil, power, and fishing industries and local communities. Since its founding in the late 1980s, the Alaska Volcano Observatory (AVO) has installed new monitoring networks and used satellite data to track activity at Alaska's...
Authors
Steven R. Brantley, Robert McGimsey, Christina A. Neal

Topographic mapping of Mars: From hectometer to micrometer scales Topographic mapping of Mars: From hectometer to micrometer scales

We describe USGS topomapping of Mars at resolutions from 100 m to 30 µm with data from the latest spacecraft missions. Analysis of NASA 2001 Mars Odyssey Thermal Emission Imaging System (THEMIS) data combining daytime visible reflected, daytime IR emitted, and nighttime IR emitted images allows us to isolate the physical effects of topography, albedo, and thermal inertia. To a good...
Authors
Randolph Kirk, Steven Squyres, Gerhard Neukum

A new Mars Digital Image Model (MDIM 2.1) control network A new Mars Digital Image Model (MDIM 2.1) control network

The U.S. Geological Survey has recently completed a final revised version of its 231 m/pixel global Viking image mosaic of Mars that has substantially improved geodetic accuracy compared to versions released in 1991 and 2001. This mosaic, known as MDIM 2.1, is currently available in the USGS ISIS file format (see http://astrogeology.usgs.gov/Projects/MDIM21/) and will be formatted and...
Authors
Brent Archinal, Ella M. Lee, Randolph Kirk, T. Duxbury, Robert Sucharski, Debbie Cook, Janet Barrett

A new Mars Digital Image Model (MDIM 2.1) control network A new Mars Digital Image Model (MDIM 2.1) control network

The U.S. Geological Survey has recently completed a final revised version of its 231 m/pixel global Viking image mosaic of Mars that has substantially improved geodetic accuracy compared to versions released in 1991 and 2001. This mosaic, known as MDIM 2.1, is currently available in the USGS ISIS file format and will be formatted and submitted to the NASA Planetary Data System (PDS) in...
Authors
Brent Archinal, Ella M. Lee, Randolph Kirk, T. Duxbury, Robert Sucharski, Debbie Cook, Janet Barrett
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