PREFACE

Previous

Unity is perhaps the keynote of modern science. This means unity in time, for the present is but the outgrowth of the past, and the future of the present. It means unity of process, for there seems to be no sharp dividing line between organic and inorganic, physical and mental, mental and spiritual. And the unity of modern science means also a growing tendency toward coÖperation, so that by working together scientists discover much that would else have remained hid.

This book illustrates the modern trend toward unity in all of these ways. First, it is a companion volume to Earth and Sun. That volume is a discussion of the causes of weather, but a consideration of the weather of the present almost inevitably leads to a study of the climate of the past. Hence the two books were written originally as one, and were only separated from considerations of convenience. Second, the unity of nature is so great that when a subject such as climatic changes is considered, it is almost impossible to avoid other subjects, such as the movements of the earth's crust. Hence this book not only discusses climatic changes, but considers the causes of earthquakes and attempts to show how climatic changes may be related to great geological revolutions in the form, location, and altitude of the lands. Thus the book has a direct bearing on all the main physical factors which have molded the evolution of organic life, including man.

In the third place, this volume illustrates the unity of modern science because it is preËminently a coÖperative product. Not only have the two authors shared in its production, but several of the Yale Faculty have also coÖperated. From the geological standpoint, Professor Charles Schuchert has read the entire manuscript in its final form as well as parts at various stages. He has helped not only by criticisms, suggestions, and facts, but by paragraphs ready for the printer. In the same way in the domain of physics, Professor Leigh Page has repeatedly taken time to assist, and either in writing or by word of mouth has contributed many pages. In astronomy, the same cordial coÖperation has come with equal readiness from Professor Frank Schlesinger. Professors Schuchert, Schlesinger, and Page have contributed so materially that they are almost co-authors of the volume. In mathematics, Professor Ernest W. Brown has been similarly helpful, having read and criticised the entire book. In certain chemical problems, Professor Harry W. Foote has been our main reliance. The advice and suggestions of these men have frequently prevented errors, and have again and again started new and profitable lines of thought. If we have made mistakes, it has been because we have not profited sufficiently by their coÖperation. If the main hypothesis of this book proves sound, it is largely because it has been built up in constant consultation with men who look at the problem from different points of vision. Our appreciation of their generous and unstinted coÖperation is much deeper than would appear from this brief paragraph.

Outside the Yale Faculty we have received equally cordial assistance. Professor T. C. Chamberlin of the University of Chicago, to whom, with his permission, we take great pleasure in dedicating this volume, has read the entire proof and has made many helpful suggestions. We cannot speak too warmly of our appreciation not only of this, but of the way his work has served for years as an inspiration in the preliminary work of gathering data for this volume. Professor Harlow Shapley of Harvard University has contributed materially to the chapter on the sun and its journey through space; Professor Andrew E. Douglass of the University of Arizona has put at our disposal some of his unpublished results; Professors S. B. Woodworth and Reginald A. Daly, and Mr. Robert W. Sayles of Harvard, and Professor Henry F. Reid of Johns Hopkins have suggested new facts and sources of information; Professor E. R. Cumings of Indiana University has critically read the entire proof; conversations with Professor John P. Buwalda of the University of California while he was teaching at Yale make him another real contributor; and Mr. Wayland Williams has contributed the interesting quotation from Bacon on page x of this book. Miss Edith S. Russell has taken great pains in preparing the manuscript and in suggesting many changes that make for clearness. Many others have also helped, but it is impossible to make due acknowledgment because such contributions have become so thoroughly a part of the mental background of the book that their source is no longer distinct in the minds of the authors.

The division of labor between the two authors has not followed any set rules. Both have had a hand in all parts of the book. The main draft of Chapters VII, VIII, IX, XI, and XIII was written by the junior author; his contributions are also especially numerous in Chapters X and XV; the rest of the book was written originally by the senior author.

CONTENTS
I The Uniformity of Climate 1
II. The Variability of Climate 16
III. Hypotheses of Climatic Change 33
IV. The Solar Cyclonic Hypothesis 51
V. The Climate of History 64
VI. The Climatic Stress of the Fourteenth Century 98
VII. Glaciation According to the Solar Cyclonic Hypothesis 110
VIII. Some Problems of Glacial Periods 130
IX. The Origin of Loess 155
X. Causes of Mild Geological Climates 166
XI. Terrestrial Causes of Climatic Changes 188
XII. Post-Glacial Crustal Movements and Climatic Changes 215
XIII. The Changing Composition of Oceans and Atmosphere 223
XIV. The Effect of Other Bodies on the Sun 242
XV. The Sun's Journey through Space 264
XVI. The Earth's Crust and the Sun 285

LIST OF ILLUSTRATIONS
Fig. 1. Climatic changes and mountain building 25
Fig. 2. Storminess at sunspot maxima vs. minima 54
Fig. 3. Relative rainfall at times of increasing and decreasing sunspots 58, 59
Fig. 4. Changes of climate in California and in western and central Asia 75
Fig. 5. Changes in California climate for 2000 years, as measured by growth of Sequoia trees 77
Fig. 6. Distribution of Pleistocene ice sheets 123
Fig. 7. Permian geography and glaciation 145
Fig. 8. Effect of diminution of storms on movement of water 175
Fig. 9. Cretaceous Paleogeography 201
Fig. 10. Climatic changes of 140,000 years as inferred from the stars 279
Fig. 11. Sunspot curve showing cycles, 1750 to 1920 283
Fig. 12. Seasonal distribution of earthquakes 299
Fig. 13. Wandering of the pole from 1890 to 1898 303

TABLES
1. The Geological Time Table 5
2. Types of Climatic Sequence 16
3. Correlation Coefficients between Rainfall and Growth of Sequoias in California 80
4. Correlation Coefficients between Rainfall Records in California and Jerusalem 84
5. Theoretical Probability of Stellar Approaches 260
6. Thirty-Eight Stars Having Largest Known Parallaxes 276, 277
7. Destructive Earthquakes from 1800 to 1899 Compared with Sunspots 289
8. Seasonal March of Earthquakes 295
9. Deflection of Path of Pole Compared with Earthquakes 305
10. Earthquakes in 1903 to 1908 Compared with Departures of the Projected Curve of the Earth's Axis from the Eulerian Position 306
                                                                                                                                                                                                                                                                                                           

Clyx.com


Top of Page
Top of Page