Wind as a Geological Process :On Earth, Mars, Venus and Titan ( Cambridge Planetary Science Old )

Publication subTitle :On Earth, Mars, Venus and Titan

Publication series :Cambridge Planetary Science Old

Author: Ronald Greeley; James D. Iversen  

Publisher: Cambridge University Press‎

Publication year: 1987

E-ISBN: 9780511867491

P-ISBN(Paperback): 9780521359627

Subject: P512.1 weathering

Keyword: 自然地理学

Language: ENG

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Wind as a Geological Process

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

1.4.3 Venus

1.4.4 Titan

2 The aeolian environment

2.1 Introduction

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

2.4.1 Turbulence

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

2.4.6 Diffusion

2.5 Windblown particles

2.6 Processes of particle formation

2.6.1 Weathering

2.6.2 Cataclastic processes

2.6.3 Volcanism

2.6.4 Precipitation and biological activity

2.6.5 Aggregation

2.7 Sand and dust sources

3 Physics of particle motion

3.1 Introduction

3.2 Classification of motion

3.3 Threshold of motion

3.3.1 Particle forces

3.3.2 Theoretical expressions for threshold

3.3.3 Wind tunnel experiments

3.3.4 Roughness effects

3.3.5 Effects of moisture and other cohesive forces

3.3.6 Vortex threshold

3.3.7 Threshold predictions for other planets

3.4 Particle trajectories

3.4.1 Particle forces

3.4.2 Saltation trajectories

3.4.3 Predictions of saltation trajectories

3.5 The saltation layer

3.5.1 Particle flux

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

4.1 Introduction

4.2 Aeolian abrasion of rocks and minerals

4.2.1 Mechanics of abrasion

4.2.2 Susceptibility to abrasion

4.3 Ventifacts

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 Yardangs

4.5.1 General characteristics

4.5.2 Yardang localities

4.5.3 Yardang formation

4.5.4 Yardangs on Mars

5 Aeolian sand deposits and bedforms

5.1 Introduction

5.1.1 Sand waves

5.2 Ripples

5.2.1 Ripple morphology

5.2.2 Internal structures in ripples

5.2.3 Ripple formation

5.2.4 'Fluid drag' ripples, 'normal' ripples, and 'mega-ripples'

5.2.5 Ripples on other planets

5.3 Sand dunes

5.3.1 Dune classification and formation

5.3.2 Transverse dunes

5.3.3 Longitudinal dunes

5.3.4 Parabolic dunes

5.3.5 Dome dunes

5.3.6 Star dunes

5.3.7 Other dunes

5.3.8 Internal structures in dunes

5.3.9 Dune migration and control

5.3.10 Clay dunes

5.3.11 Dunes on Mars

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

6.1 Introduction

6.2 Atmospheric motions

6.2.1 General circulation and rotational flows

6.2.2 The vortex

6.3 Topographical effects on surface winds

6.3.1 The effects of mountains

6.3.2 Separated flows

6.4 Wind streaks

6.4.1 Modes of formation

6.4.2 Streaks on Earth

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 Windblown dust

7.1 Introduction

7.2 Dust storms on Earth

7.2.1 Dust storm development and effect on climate

7.2.2 Characteristics of aeolian dust

7.2.3 Erosion of agricultural land

7.2.4 Dust devils

7.2.5 Fugitive dust

7.3 Dust storms on Mars

7.3.1 Martian great dust storms

7.3.2 Martian great dust storms clearing

7.3.3 Local dust storms

7.4 Dust deposits

7.4.1 Loess on Earth

7.4.2 Dust deposits on Mars

Appendix A: Nomenclature and symbols

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

The similitude function

Glossary

References

Index

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