Description
This book gives an account of geological aspects of windblown material. Aeolian processes play an important role in modifying the surface of the Earth, and they are also active on Mars. Additionally, they are thought to occur on Venus and possibly Titan as well. The authors describe the following aspects: wind as a geological process, the aeolian environment, physics of particle motion, aeolian abrasion and erosion; aeolian sand deposits and bedforms, interaction of wind and topography and windblown dust. A particular strength of the book is that it deals with aeolian processes in a planetary context, rather than as a purely terrestrial phenomenon. In so doing, the authors ably demonstrate how we can gain better understanding of the Earth through comparative planetology. This paperback reissue will enable the book to be used as a text for advanced students in planetary science. Special terms are defined when they are first used. There is a glossary and an exhaustive bibliography.
Chapter
2 The aeolian environment
2.2 Properties of atmospheres
2.2.1 Hydrostatic equilibrium
2.2.2 Adiabatic lapse rate
2.3 Comparisons of planets and their atmospheres
2.3.1 Origin of atmospheres
2.4 The atmospheric boundary layer
2.4.2 Turbulent boundary layer
2.4.3 Effect of non-neutral stability
2.4.4 Pressure gradient and Coriolis forces
2.4.5 Friction forces - the Ekman spiral
2.6 Processes of particle formation
2.6.2 Cataclastic processes
2.6.4 Precipitation and biological activity
2.7 Sand and dust sources
3 Physics of particle motion
3.2 Classification of motion
3.3.2 Theoretical expressions for threshold
3.3.3 Wind tunnel experiments
3.3.5 Effects of moisture and other cohesive forces
3.3.7 Threshold predictions for other planets
3.4 Particle trajectories
3.4.2 Saltation trajectories
3.4.3 Predictions of saltation trajectories
3.5.2 Concentration distribution
3.5.3 Mass transport predictions for Mars and Venus
3.5.4 Effect of saltation on wind speeds near the surface
4 Aeolian abrasion and erosion
4.2 Aeolian abrasion of rocks and minerals
4.2.1 Mechanics of abrasion
4.2.2 Susceptibility to abrasion
4.3.1 Ventifact morphology
4.3.2 Factors involved in ventifact formation
4.3.3 Ventifacts on Mars and Venus
4.4 Rates of aeolian abrasion: Earth and Mars
4.5.1 General characteristics
5 Aeolian sand deposits and bedforms
5.2.2 Internal structures in ripples
5.2.4 'Fluid drag' ripples, 'normal' ripples, and 'mega-ripples'
5.2.5 Ripples on other planets
5.3.1 Dune classification and formation
5.3.8 Internal structures in dunes
5.3.9 Dune migration and control
5.4 Sand shadows and drifts
5.4.1 'Drifts' on Mars and Venus (?)
5.5 Sand sheets and streaks
6 Interaction of wind and topography
6.2.1 General circulation and rotational flows
6.3 Topographical effects on surface winds
6.3.1 The effects of mountains
6.4.3 Wind tunnel streak simulation
6.4.4 Amboy field experiment
6.4.5 Wind streaks on Mars
6.4.6 Wind streaks on Venus and Titan
7.2.1 Dust storm development and effect on climate
7.2.2 Characteristics of aeolian dust
7.2.3 Erosion of agricultural land
7.3.1 Martian great dust storms
7.3.2 Martian great dust storms clearing
7.4.2 Dust deposits on Mars
Appendix A: Nomenclature and symbols
Appendix B: Small-scale modeling of aeolian phenomena in the wind tunnel
Small-scale modeling of aeolian phenomena in wind tunnels
Transport rate similitude
Particle trajectory similitude
Effect of Froude number and density ratio