Publications
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Digital photogrammetric analysis of the IMP camera images: Mapping the Mars Pathfinder landing site in three dimensions Digital photogrammetric analysis of the IMP camera images: Mapping the Mars Pathfinder landing site in three dimensions
This paper describes our photogrammetric analysis of the Imager for Mars Pathfinder data, part of a broader program of mapping the Mars Pathfinder landing site in support of geoscience investigations. This analysis, carried out primarily with a commercial digital photogrammetric system, supported by our in‐house Integrated Software for Imagers and Spectrometers (ISIS), consists of three...
Authors
Randolph L. Kirk, Elpitha Howington-Kraus, Trent M. Hare, E. Dorrer, D. Cook, Kris J. Becker, K. Thompson, B. Redding, J. Blue, D. Galuszka, E.M. Lee, Lisa R. Gaddis, J. R. Johnson, Laurence A. Soderblom, A. W. Ward, P. H. Smith, D.T. Britt
Aeolian features and processes at the Mars Pathfinder landing site Aeolian features and processes at the Mars Pathfinder landing site
The Mars Pathfinder landing site contains abundant features attributed to aeolian, or wind, processes. These include wind tails, drift deposits, duneforms of various types, ripplelike features, and ventifacts (the first clearly seen on Mars). Many of these features are consistant with formation involving sand-size particles. Although some features, such as dunes, could develop from...
Authors
Ronald Greeley, Michael Kraft, Robert Sullivan, Gregory Wilson, Nathan Bridges, Kenneth E. Herkenhoff, Ruslan O. Kuzmin, Michael Malin, Wes Ward
Ventifacts at the Pathfinder landing site Ventifacts at the Pathfinder landing site
About half of the rocks at the Mars Pathfinder Ares Vallis landing site appear to be ventifacts, rocks abraded by windborne particles. Comparable resolution images taken by the Imager for Mars Pathfinder (IMP) camera and the Viking landers show that ventifacts are more abundant at the Pathfinder site. The ventifacts occur in several forms, including rocks with faceted edges, finger‐like
Authors
N.T. Bridges, R. Greeley, A. F. C. Haldemann, Kenneth E. Herkenhoff, M. Kraft, T. J. Parker, A. W. Ward
Geology of the Upheaval Dome impact structure, southeast Utah Geology of the Upheaval Dome impact structure, southeast Utah
Two vastly different phenomena, impact and salt diapirism, have been proposed for the origin of Upheaval Dome, a spectacular scenic feature in southeast Utah. Detailed geologic mapping and seismic refraction data indicate that the dome originated by collapse of a transient cavity formed by impact. Evidence is as follows: (1) sedimentary strata in the center of the structure are...
Authors
Bryan J. Kriens, Eugene M. Shoemaker, Kenneth E. Herkenhoff
General geology and geomorphology of the Mars Pathfinder landing site General geology and geomorphology of the Mars Pathfinder landing site
The Mars Pathfinder (MPF) spacecraft landed on relatively young (late Hesperian-early Amazonian; 3.1-0.7 Ga) plains in Chryse Planitia near the mouth of Ares Vallis. Images returned from the spacecraft reveal a complex landscape of ridges and troughs, large hills and crater rims, rocks and boulders of various sizes and shapes, and surficial deposits, indicating a complex, multistage...
Authors
A. W. Ward, Lisa R. Gaddis, Randolph L. Kirk, Laurence A. Soderblom, K. L. Tanaka, M.P. Golombek, T. J. Parker, Ronald Greeley, R.O. Kuzmin
Steady-state flow of solid CO2: Preliminary results Steady-state flow of solid CO2: Preliminary results
To help answer the question of how much solid CO2 exists in the Martian south polar cap, we performed a series of laboratory triaxial deformation experiments at constant displacement rate in compression on jacketed cylinders of pure, polycrystalline CO2. Test conditions were temperatures 150 T 190 K, hydrostatic confining pressures 5≤ P ≤40 MPa, and strain rates 4.5×10−8 ≤ ε ≤4.3×10−4 s...
Authors
William B. Durham, Stephen H. Kirby, Laura A. Stern
Stratigraphic constraints on the timing and emplacement of the Alika 2 giant Hawaiian submarine landslide Stratigraphic constraints on the timing and emplacement of the Alika 2 giant Hawaiian submarine landslide
Previous work has found evidence for giant tsunami waves that impacted the coasts of Lanai, Molokai and other southern Hawaiian Islands, tentatively dated at 100 + and 200 + ka by U-series methods on uplifted coral clasts. Seafloor imaging and related work off Hawaii Island has suggested the Alika phase 2 debris avalanche as the source of the ~ 100 ka "giant wave deposits", although its...
Authors
Gary M. McMurtry, Emilio Herrero-Bervera, Maximilian D. Cremer, John R. Smith, Johanna Resig, Clark Sherman, Michael E. Torresan
A physically-based earthquake recurrence model for estimation of long-term earthquake probabilities A physically-based earthquake recurrence model for estimation of long-term earthquake probabilities
A physically-motivated model for earthquake recurrence based on the Brownian relaxation oscillator is introduced. The renewal process defining this point process model can be described by the steady rise of a state variable from the ground state to failure threshold as modulated by Brownian motion. Failure times in this model follow the Brownian passage time (BPT) distribution, which is...
Authors
William L. Ellsworth, Mark V. Matthews, Robert M. Nadeau, Stuart P. Nishenko, Paul A. Reasenberg, Robert W. Simpson
Dark material in the polar layered deposits and dunes on Mars Dark material in the polar layered deposits and dunes on Mars
Viking infrared thermal mapping and bistatic radar data suggest that the bulk density of the north polar erg material is much lower than that of the average Martian surface or of dark dunes at lower latitudes. We have derived a thermal inertia of 245–280 J m−2 s−1/2 K−1 (5.9–6.7×10−3 cal cm−2 s−1/2 K−1) for the Proctor dune field and 25–150 J m−2 s−1/2 K−1 (0.6–3.6×10−3cal cm−2 s−1/2 K−1...
Authors
Kenneth E. Herkenhoff, Ashwin R. Vasavada
Magma migration and resupply during the 1974 summit eruptions of Kilauea Volcano, Hawaii Magma migration and resupply during the 1974 summit eruptions of Kilauea Volcano, Hawaii
The purpose of this paper is to present a complete account of contrasting yet related eruptions, thus filling a gap in the published narratives of recent activity of Kilauea; and to examine their significance within a broader context of regional magmatic and eruptive dynamics. We have gained a historical perspective and can view these three eruptions within a multidecade context of the...
Authors
John P. Lockwood, Robert I. Tilling, Robin T. Holcomb, Fred W. Klein, Arnold T. Okamura, Donald W. Peterson
The Puelche volcanic field: Extensive Pleistocene rhyolite lava flows in the Andes of central Chile The Puelche volcanic field: Extensive Pleistocene rhyolite lava flows in the Andes of central Chile
A remote volcanic field in the rugged headwaters of the Río Puelche and Río Invernada (35.8°S) constitutes the largest cluster of Quaternary rhyolite lava flows yet identified in the Andean Southern Volcanic Zone. The Puelche Volcanic Field belongs to an intra-arc belt of silicic magmatic centers that extends, at least, 140 km north-south and lies well east of the volcanic front but...
Authors
Wes Hildreth, J. Fierstein, E. Godoy, Robert E. Drake, B. Singer
Effect of baseline corrections on response spectra for two recordings of the 1999 Chi-Chi, Taiwan, earthquake Effect of baseline corrections on response spectra for two recordings of the 1999 Chi-Chi, Taiwan, earthquake
Displacements derived from the accelerogram recordings of the 1999 Chi-Chi, Taiwan earthquake at stations TCU078 and TCU129 show drifts when only a simple baseline derived from the pre-event portion of the record is removed from the records. The appearance of the velocity and displacement records suggests that changes in the zero-level of the acceleration are responsible for these drifts...
Authors
David M. Boore