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Journal articles on the topic 'Arizona Meteor Crater'

Author: Grafiati

Published: 4 June 2021

Last updated: 1 February 2022

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1

Bogatikov, O. A., R. V. Boyarskaya, S. V. Soboleva, and D. I. Frikh-Khar. "IMPACT ROCKS OF METEOR CRATER, ARIZONA." International Geology Review 27, no. 3 (1985): 319–26. http://dx.doi.org/10.1080/00206818509466419.

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2

Grant, John A., and Peter H. Schultz. "Erosion of ejecta at Meteor Crater, Arizona." Journal of Geophysical Research 98, E8 (1993): 15033. http://dx.doi.org/10.1029/93je01580.

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3

Nishiizumi, K., C. P. Kohl, E. M. Shoemaker, et al. "In situ10Be-26Al exposure ages at Meteor Crater, Arizona." Geochimica et Cosmochimica Acta 55, no. 9 (1991): 2699–703. http://dx.doi.org/10.1016/0016-7037(91)90388-l.

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4

Roy, S., and R. R. Stewart. "Near-surface Seismic Investigation of Barringer (Meteor) Crater, Arizona." Journal of Environmental & Engineering Geophysics 17, no. 3 (2012): 117–27. http://dx.doi.org/10.2113/jeeg17.3.117.

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5

Sutton, S. R. "Thermoluminescence measurements on shock-metamorphosed sandstone and dolomite from Meteor Crater, Arizona: 2. Thermoluminescence age of meteor crater." Journal of Geophysical Research 90, B5 (1985): 3690. http://dx.doi.org/10.1029/jb090ib05p03690.

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6

Hörz, Friedrich, David W. Mittlefehldt, Thomas H. See, and Charles Galindo. "Petrographic studies of the impact melts from Meteor Crater, Arizona, USA." Meteoritics & Planetary Science 37, no. 4 (2002): 501–31. http://dx.doi.org/10.1111/j.1945-5100.2002.tb00836.x.

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7

Kumar, P. Senthil, James W. Head, and David A. Kring. "Erosional modification and gully formation at Meteor Crater, Arizona: Insights into crater degradation processes on Mars." Icarus 208, no. 2 (2010): 608–20. http://dx.doi.org/10.1016/j.icarus.2010.03.032.

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8

Madden, Megan E. Elwood, David A. Kring, and Robert J. Bodnar. "Shock reequilibration of fluid inclusions in Coconino sandstone from Meteor Crater, Arizona." Earth and Planetary Science Letters 241, no. 1-2 (2006): 32–46. http://dx.doi.org/10.1016/j.epsl.2005.10.008.

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9

Pilon, J. A., R. A. F. Grieve, and V. L. Sharpton. "The subsurface character of Meteor Crater, Arizona, as determined by ground-probing radar." Journal of Geophysical Research: Planets 96, E1 (1991): 15563–76. http://dx.doi.org/10.1029/91je01114.

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10

Myers, S. A., R. T. Cygan, R. A. Assink, and M. B. Boslough. "29 Si MAS NMR relaxation study of shocked Coconino Sandstone from Meteor Crater, Arizona." Physics and Chemistry of Minerals 25, no. 5 (1998): 313–17. http://dx.doi.org/10.1007/s002690050120.

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11

Burt, Jason B., Mike C. Pope, and A. John Watkinson. "Petrographic, X-ray diffraction, and electron spin resonance analysis of deformed calcite: Meteor Crater, Arizona." Meteoritics & Planetary Science 40, no. 2 (2005): 297–306. http://dx.doi.org/10.1111/j.1945-5100.2005.tb00381.x.

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12

Phillips, Fred M., Marek G. Zreda, Stewart S. Smith, et al. "Age and geomorphic history of Meteor Crater, Arizona, from cosmogenic 36Cl and 14C in rock varnish." Geochimica et Cosmochimica Acta 55, no. 9 (1991): 2695–98. http://dx.doi.org/10.1016/0016-7037(91)90387-k.

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13

Cavosie, Aaron J., Nicholas E. Timms, Timmons M. Erickson, Justin J. Hagerty, and Friedrich Hörz. "Transformations to granular zircon revealed: Twinning, reidite, and ZrO2in shocked zircon from Meteor Crater (Arizona, USA)." Geology 44, no. 9 (2016): 703–6. http://dx.doi.org/10.1130/g38043.1.

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14

Racki, Grzegorz, John W. M. Jagt, Elena A. Jagt-Yazykova, and Christian Koeberl. "A Dutch contribution to early interpretations of Meteor Crater, Arizona, USA – Marten Edsge Mulder’s ignored 1911 paper." Proceedings of the Geologists' Association 129, no. 4 (2018): 542–60. http://dx.doi.org/10.1016/j.pgeola.2018.05.005.

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15

Xue, S., G. F. Herzog, G. S. Hall, J. Klein, R. Middleton, and D. Juenemann. "Stable nickel isotopes and cosmogenic beryllium-10 and aluminum-26 in metallic spheroids from Meteor Crater, Arizona." Meteoritics 30, no. 3 (1995): 303–10. http://dx.doi.org/10.1111/j.1945-5100.1995.tb01128.x.

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16

Sutton, S. R. "Thermoluminescence measurements on shock-metamorphosed sandstone and dolomite from Meteor Crater, Arizona: 1. Shock dependence of thermoluminescence properties." Journal of Geophysical Research 90, B5 (1985): 3683. http://dx.doi.org/10.1029/jb090ib05p03683.

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17

Wright, Shawn P., and Michael S. Ramsey. "Thermal infrared data analyses of Meteor Crater, Arizona: Implications for Mars spaceborne data from the Thermal Emission Imaging System." Journal of Geophysical Research: Planets 111, E2 (2006): n/a. http://dx.doi.org/10.1029/2005je002472.

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18

Norwick, Stephen A., and Leland R. Dexter. "Rates of development of tafoni in the Moenkopi and Kaibab formations in Meteor Crater and on the Colorado Plateau, northeastern Arizona." Earth Surface Processes and Landforms 27, no. 1 (2002): 11–26. http://dx.doi.org/10.1002/esp.276.

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19

Yang, Wang-Hong, R. James Kirkpatrick, Norma Vergo, John McHone, Tryggvi I. Emilsson, and Eric Oldfield. "DETECTION OF HIGH-PRESSURE SILICA POLYMORPHS IN WHOLE-ROCK SAMPLES FROM A METEOR CRATER, ARIZONA, IMPACT SAMPLE USING SOLID-STATE SILICON-29 NUCLEAR MAGNETIC RESONANCE SPECTROSCOPY." Meteoritics 21, no. 1 (1986): 117–24. http://dx.doi.org/10.1111/j.1945-5100.1986.tb01230.x.

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20

Verma, Ankit Kumar, and Mary Carol Bourke. "A method based on structure-from-motion photogrammetry to generate sub-millimetre-resolution digital elevation models for investigating rock breakdown features." Earth Surface Dynamics 7, no. 1 (2019): 45–66. http://dx.doi.org/10.5194/esurf-7-45-2019.

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Abstract. We have generated sub-millimetre-resolution DEMs of weathered rock surfaces using SfM photogrammetry techniques. We apply a close-range method based on structure-from-motion (SfM) photogrammetry in the field and use it to generate high-resolution topographic data for weathered boulders and bedrock. The method was pilot tested on extensively weathered Triassic Moenkopi sandstone outcrops near Meteor Crater in Arizona. Images were taken in the field using a consumer-grade DSLR camera and were processed in commercially available software to build dense point clouds. The point clouds wer

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21

Pilon, J. A., R. A. F. Grieve, and V. L. Sharpton. "Correction to “The subsurface character of Meteor Crater, Arizona, as determined by ground-probing radar” by J. A. Pilon, R. A. F. Grieve, and V. L. Sharpton." Journal of Geophysical Research 96, E4 (1991): 20989. http://dx.doi.org/10.1029/91je02290.

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22

Adler, Bianca, C. David Whiteman, Sebastian W. Hoch, Manuela Lehner, and Norbert Kalthoff. "Warm-Air Intrusions in Arizona’s Meteor Crater." Journal of Applied Meteorology and Climatology 51, no. 6 (2012): 1010–25. http://dx.doi.org/10.1175/jamc-d-11-0158.1.

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AbstractEpisodic nighttime intrusions of warm air, accompanied by strong winds, enter the enclosed near-circular Meteor Crater basin on clear, synoptically undisturbed nights. Data analysis is used to document these events and to determine their spatial and temporal characteristics, their effects on the atmospheric structure inside the crater, and their relationship to larger-scale flows and atmospheric stability. A conceptual model that is based on hydraulic flow theory is offered to explain warm-air-intrusion events at the crater. The intermittent warm-air-intrusion events were closely relat

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23

Lehner, Manuela, C. David Whiteman, Sebastian W. Hoch, et al. "The METCRAX II Field Experiment: A Study of Downslope Windstorm-Type Flows in Arizona’s Meteor Crater." Bulletin of the American Meteorological Society 97, no. 2 (2016): 217–35. http://dx.doi.org/10.1175/bams-d-14-00238.1.

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Abstract The second Meteor Crater Experiment (METCRAX II) was conducted in October 2013 at Arizona’s Meteor Crater. The experiment was designed to investigate nighttime downslope windstorm−type flows that form regularly above the inner southwest sidewall of the 1.2-km diameter crater as a southwesterly mesoscale katabatic flow cascades over the crater rim. The objective of METCRAX II is to determine the causes of these strong, intermittent, and turbulent inflows that bring warm-air intrusions into the southwest part of the crater. This article provides an overview of the scientific goals of th

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24

Hoch, Sebastian W., and C. David Whiteman. "Topographic Effects on the Surface Radiation Balance in and around Arizona’s Meteor Crater." Journal of Applied Meteorology and Climatology 49, no. 6 (2010): 1114–28. http://dx.doi.org/10.1175/2010jamc2353.1.

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Abstract The individual components of the slope-parallel surface radiation balance were measured in and around Arizona’s Meteor Crater to investigate the effects of topography on the radiation balance. The crater basin has a diameter of 1.2 km and a depth of 170 m. The observations cover the crater floor, the crater rim, four sites on the inner sidewalls on an east–west transect, and two sites outside the crater. Interpretation of the role of topography on radiation differences among the sites on a representative clear day is facilitated by the unique symmetric crater topography. The shortwave

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25

Lehner, Manuela, C. David Whiteman, and Sebastian W. Hoch. "Diurnal Cycle of Thermally Driven Cross-Basin Winds in Arizona’s Meteor Crater." Journal of Applied Meteorology and Climatology 50, no. 3 (2011): 729–44. http://dx.doi.org/10.1175/2010jamc2520.1.

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Abstract Cross-basin winds produced by asymmetric insolation of the crater sidewalls occur in Arizona’s Meteor Crater on days with weak background winds. The diurnal cycle of the cross-basin winds is analyzed together with radiation, temperature, and pressure measurements at the crater sidewalls for a 1-month period. The asymmetric irradiation causes horizontal temperature and pressure gradients across the crater basin that drive the cross-basin winds near the crater floor. The horizontal temperature and pressure gradients and wind directions change as the sun moves across the sky, with easter

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26

Lehner, Manuela, Richard Rotunno, and C. David Whiteman. "Flow Regimes over a Basin Induced by Upstream Katabatic Flows—An Idealized Modeling Study." Journal of the Atmospheric Sciences 73, no. 10 (2016): 3821–42. http://dx.doi.org/10.1175/jas-d-16-0114.1.

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Abstract Idealized two-dimensional model simulations are performed to study the frequent nocturnal occurrence of downslope-windstorm-type flows in Arizona’s Meteor Crater. The model topography is a simplified representation of the Meteor Crater and its surroundings, with an approximately 1° mesoscale slope upstream and downstream of the crater basin. A strong surface-based inversion and a katabatic flow develop above the mesoscale slope as a result of radiational cooling. The temperature and flow profiles are evaluated against observations over low-angle slopes from two field campaigns, showin

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27

Haiden, Thomas, C. David Whiteman, Sebastian W. Hoch, and Manuela Lehner. "A Mass Flux Model of Nocturnal Cold-Air Intrusions into a Closed Basin." Journal of Applied Meteorology and Climatology 50, no. 5 (2011): 933–43. http://dx.doi.org/10.1175/2010jamc2540.1.

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AbstractObservations made during the Meteor Crater Experiment (METCRAX) field campaign revealed unexpected nighttime cooling characteristics in Arizona’s Meteor Crater. Unlike in other natural closed basins, a near-isothermal temperature profile regularly develops over most of the crater depth, with only a shallow stable layer near the crater floor. A conceptual model proposed by Whiteman et al. attributes the near-isothermal stratification to the intrusion, and subsequent detrainment, of near-surface air from outside the crater into the crater atmosphere. To quantify and test the hypothesis,

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28

Mayer, B., S. W. Hoch, and C. D. Whiteman. "Validating the MYSTIC three-dimensional radiative transfer model with observations from the complex topography of Arizona's Meteor Crater." Atmospheric Chemistry and Physics Discussions 10, no. 5 (2010): 13373–405. http://dx.doi.org/10.5194/acpd-10-13373-2010.

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Abstract. The MYSTIC three-dimensional Monte-Carlo radiative transfer model has been extended to simulate solar and thermal irradiances with a rigorous consideration of topography. Forward as well as backward Monte Carlo simulations are possible for arbitrarily oriented surfaces and we demonstrate that the backward Monte Carlo technique is superior to the forward method for applications involving topography, by greatly reducing the computational demands. MYSTIC is used to simulate the short- and longwave radiation fields during a clear day and night in and around Arizona's Meteor Crater, a bow

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29

Mayer, B., S. W. Hoch, and C. D. Whiteman. "Validating the MYSTIC three-dimensional radiative transfer model with observations from the complex topography of Arizona's Meteor Crater." Atmospheric Chemistry and Physics 10, no. 18 (2010): 8685–96. http://dx.doi.org/10.5194/acp-10-8685-2010.

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Abstract. The MYSTIC three-dimensional Monte-Carlo radiative transfer model has been extended to simulate solar and thermal irradiances with a rigorous consideration of topography. Forward as well as backward Monte Carlo simulations are possible for arbitrarily oriented surfaces and we demonstrate that the backward Monte Carlo technique is superior to the forward method for applications involving topography, by greatly reducing the computational demands. MYSTIC is used to simulate the short- and longwave radiation fields during a clear day and night in and around Arizona's Meteor Crater, a bow

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30

Whiteman, C. David, Manuela Lehner, Sebastian W. Hoch, Bianca Adler, Norbert Kalthoff, and Thomas Haiden. "Katabatically Driven Cold Air Intrusions into a Basin Atmosphere." Journal of Applied Meteorology and Climatology 57, no. 2 (2018): 435–55. http://dx.doi.org/10.1175/jamc-d-17-0131.1.

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AbstractThe interactions between a katabatic flow on a plain and a circular basin cut into the plain and surrounded by an elevated rim were examined during a 5-h steady-state period during the Second Meteor Crater Experiment (METCRAX II) to explain observed disturbances to the nocturnal basin atmosphere. The approaching katabatic flow split horizontally around Arizona’s Meteor Crater below a dividing streamline while, above the dividing streamline, an ~50-m-deep stable layer on the plain was carried over the 30–50-m rim of the basin. A flow bifurcation occurred over or just upwind of the rim,

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31

Whiteman, C. David, Sebastian W. Hoch, Manuela Lehner, and Thomas Haiden. "Nocturnal Cold-Air Intrusions into a Closed Basin: Observational Evidence and Conceptual Model." Journal of Applied Meteorology and Climatology 49, no. 9 (2010): 1894–905. http://dx.doi.org/10.1175/2010jamc2470.1.

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Abstract Observations are analyzed to explain an unusual feature of the nighttime atmospheric structure inside Arizona’s idealized, basin-shaped Meteor Crater. The upper 75%–80% of the crater’s atmosphere, which overlies an intense surface-based inversion on the crater’s floor, maintains a near-isothermal lapse rate during the entire night, even while continuing to cool. Evidence is presented to show that this near-isothermal layer is produced by cold-air intrusions that come over the crater’s rim. The intrusions are driven by a regional-scale drainage flow that develops over the surrounding i

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32

Villagrasa, Daniel Martínez, Manuela Lehner, C. David Whiteman, Sebastian W. Hoch, and Joan Cuxart. "The Upslope–Downslope Flow Transition on a Basin Sidewall." Journal of Applied Meteorology and Climatology 52, no. 12 (2013): 2715–34. http://dx.doi.org/10.1175/jamc-d-13-049.1.

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AbstractThe late afternoon upslope–downslope flow transition on the west inner sidewall of Arizona’s Meteor Crater, visualized by photographs of smoke dispersion, is investigated for 20 October 2006 using surface radiative and energy budget data and mean and turbulent flow profiles from three towers, two at different distances up the slope and one on the basin floor. The bowl-shaped crater allows the development of the upslope–downslope flow transition with minimal influence from larger-scale motions from outside and avoiding the upvalley–downvalley flow interactions typical of valleys. The sl

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33

Wilson, Lionel. "W. G. Hoyt 1987. Coon Mountain Controversies. Meteor Crater and the Development of Impact Theory. xii + 443 pp. Tucson: University of Arizona Press. Price US $40.00 (hard covers). ISBN 0 8165 0968 9. - J. Pohl (ed.) 1987. Research in Terrestrial Impact Structures. v + 142 pp. Braunschweig, Wiesbaden: Vieweg. Price £38.20 (hard covers). ISBN 3 528 08940 7." Geological Magazine 127, no. 1 (1990): 90–91. http://dx.doi.org/10.1017/s0016756800014357.

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34

Whiteman, C. David, Manuela Lehner, Sebastian W. Hoch, et al. "The Nocturnal Evolution of Atmospheric Structure in a Basin as a Larger-Scale Katabatic Flow Is Lifted over Its Rim." Journal of Applied Meteorology and Climatology 57, no. 4 (2018): 969–89. http://dx.doi.org/10.1175/jamc-d-17-0156.1.

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AbstractThe successive stages of nocturnal atmospheric structure inside a small isolated basin are investigated when a katabatically driven flow on an adjacent tilted plain advects cold air over the basin rim. Data came from Arizona’s Meteor Crater during intensive observing period 4 of the Second Meteor Crater Experiment (METCRAX II) when a mesoscale flow above the plain was superimposed on the katabatic flow leading to a flow acceleration and then deceleration over the course of the night. Following an overflow-initiation phase, the basin atmosphere over the upwind inner sidewall progressed

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35

Hoch, Sebastian W., C. David Whiteman, and Bernhard Mayer. "A Systematic Study of Longwave Radiative Heating and Cooling within Valleys and Basins Using a Three-Dimensional Radiative Transfer Model." Journal of Applied Meteorology and Climatology 50, no. 12 (2011): 2473–89. http://dx.doi.org/10.1175/jamc-d-11-083.1.

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AbstractThe Monte Carlo code for the physically correct tracing of photons in cloudy atmospheres (MYSTIC) three-dimensional radiative transfer model was used in a parametric study to determine the strength of longwave radiative heating and cooling in atmospheres enclosed in idealized valleys and basins. The parameters investigated included valley or basin shape, width, and near-surface temperature contrasts. These parameters were varied for three different representative atmospheric temperature profiles for different times of day. As a result of counterradiation from surrounding terrain, night

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36

Kumar, P. Senthil, and David A. Kring. "Impact fracturing and structural modification of sedimentary rocks at Meteor Crater, Arizona." Journal of Geophysical Research 113, E9 (2008). http://dx.doi.org/10.1029/2008je003115.

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37

Ramsey, Michael S. "Ejecta distribution patterns at Meteor Crater, Arizona: On the applicability of lithologic end-member deconvolution for spaceborne thermal infrared data of Earth and Mars." Journal of Geophysical Research 107, E8 (2002). http://dx.doi.org/10.1029/2001je001827.

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38

Fritts, David C., Daniel Goldstein, and Tom Lund. "High-resolution numerical studies of stable boundary layer flows in a closed basin: Evolution of steady and oscillatory flows in an axisymmetric Arizona Meteor Crater." Journal of Geophysical Research 115, no. D18 (2010). http://dx.doi.org/10.1029/2009jd013359.

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