ebook img

Clouds their Formation, Optical Properties, and Effects PDF

501 Pages·1981·38.289 MB·English
Save to my drive
Quick download
Download
Most books are stored in the elastic cloud where traffic is expensive. For this reason, we have a limit on daily download.

Preview Clouds their Formation, Optical Properties, and Effects

CLOUDS THEIR FORMATION, OPTICAL PROPERTIES, AND EFFECTS Edited by PETER V. HOBBS Department of Atmospheric Sciences University of Washington Seattle, Washington ADARSH DEEPAK Institute for Atmospheric Optics and Remote Sensing Hampton, Virginia ACADEMIC PRESS 1981 A Subsidiary of Harcourt Brace Jovanovich, Publishers New York London Toronto Sydney San Francisco COPYRIGHT © 1981, BY ACADEMIC PRESS, INC. ALL RIGHTS RESERVED. NO PART OF THIS PUBLICATION MAY BE REPRODUCED OR TRANSMITTED IN ANY FORM OR BY ANY MEANS, ELECTRONIC OR MECHANICAL, INCLUDING PHOTOCOPY, RECORDING, OR ANY INFORMATION STORAGE AND RETRIEVAL SYSTEM, WITHOUT PERMISSION IN WRITING FROM THE PUBLISHER. ACADEMIC PRESS, INC. Ill Fifth Avenue, New York, New York 10003 United Kingdom Edition published by ACADEMIC PRESS, INC. (LONDON) LTD. 24/28 Oval Road, London NW1 7DX Library of Congress Cataloging in Publication Data Symposium on Clouds: Their Formation, Optical Properties, and Effects and (1980 : Williamsburg, Va.) Clouds, their formation, optical properties, and effects. "Proceedings of Symposium on Clouds: Their Formation, Optical Properties, and Effects, sponsored by Army Atmos­ pheric Sciences Laboratory and Army Research Office, Williamsburg, Virginia, 13-14 May 1980"—Verso t.p. Includes index. Contents: Scales involved in the formation and organi­ zation of clouds and precipitation / Peter V. Hobbs — Techniques for probing cloud microstructure / R. G. Knollenberg — The microstructure of atmospheric clouds and precipitation / H. R. Pruppacher — [etc.] 1. Cloud physics—Congresses. I. Hobbs, Peter Victor, Date. II. Deepak, Adarsh. III. Atmospheric Sciences Laboratory (U. S.) IV. United States. Army Research Office. V. Title. QC921.48.S95 1980 55l.57'6 81-3491 ISBN 0-12-350720-0 AACR2 PRINTED IN THE UNITED STATES OF AMERICA 81 82 83 84 9 8 7 6 5 4 3 2 1 PARTICIPANTS Abdul Alkezweeny, Batteile, Pacific Northwest Laboratory, P. Ο. Box 999, Richland, Washington 99352 Β. Jeffrey Anderson, NASA-Marshall Space Flight Center, ES 83, Marshall Space Flight Center, Alabama 35812 Allan I. Carswell, York University, Department of Physics, 4700 Keele Street, Downs view, Ontario, Canada M3J 1P3 Ronald M. Cionco, Atmospheric Sciences Laboratory, DELAS-BE-C, White Sands Missile Range, New Mexico 88002 Stephen K. Cox, Department of Atmospheric Science, Colorado State University, Fort Collins, Colorado 80524 William E. Cummins II, TRADOC Weather Office, Building P-173, United States Air Force, Fort Monroe, Virginia 23651 M. H. Davis, USRA, P. O. Box 3006, Boulder, Colorado 80307 Adarsh Deepak, Institute for Atmospheric Optics and Remote Sensing, P. O. Box P, Hampton, Virginia 23666 James E. Dye, NC AR, P. Ο. Box 3000, Boulder, Colorado 80303 Usamah O. Farrukh, Institute of Atmospheric Optics and Remote Sensing, P. O. Box P, Hampton, Virginia 23666 B. Richard Fow, Geo-Atmospheric Corporation, Box 117, Lincoln, Maryland 01773 M. Geller, Naval Ocean System Center, Code 813, 271 Catalina Boulevard, San Diego, California 92152 Hermann E. Gerber, Naval Research Laboratory, Washington, D. C. 20375 Richard B. Gomez, Atmospheric Sciences Laboratory, Atten: DELAS-EO-MO, White Sands Missile Range, New Mexico 88002 Andrew Heymsfield, NC AR, P. Ο. Box 3000, Boulder, Colorado 80303 Peter V. Hobbs, Department of Atmospheric Sciences, AK-40, University of Washington, Seattle, Washington 98195 Gerald Hoist, Chemical Systems Laboratory, DRDAR-CLB-PS, Aberdeen Proving Ground, Maryland 21005 vii viii PARTICIPANTS Jim Hudson, Desert Research Institute, P. O. Box 60220, Reno, Nevada 89506 Garry E. Hunt, University College London, Gower Street, London, England WC1E 6BT Edwin C. Hutter, RCA Astro-Electronics, P. O. Box 800, Princeton, New Jersey 08640 Dave Ingram, TRADOC, Fort Monroe, Virginia 23651 Casimir Jachimowski, NASA-Langley Research Center, MS 404B, Hampton, Virginia 23665 Kolf Jayaweera, Geophysics Institute, University of Alaska, Fairbanks, Alaska 99701 James E. Jiusto, Atmospheric Sciences Research Center, State University of New York, 1400 Washington Avenue, Albany, New York 12222 Marvin Kays, Atmospheric Sciences Laboratory, White Sands Missile Range, New Mexico 88002 Geoffrey Kent, Institute for Atmospheric Optics and Remote Sensing, P. O. Box P, Hampton, Virginia 23666 Michael King, NASA-Goddard Space Flight Center, Code 915, Greenbelt, Maryland 20771 Robert G. Knollenberg, Particle Measuring Systems, Inc., 1855 South 57th Court, Boulder, Colorado 80301 Kuo-Nan Liou, Department of Meteorology, University of Utah, Salt Lake City, Utah 84112 John D. Mill, AFGL/OPA, Hanscom AFB, Massachusetts 01731 G. C. Mooradian, Naval Ocean System Center, Code 811, 271 Catalina Boulevard, San Diego, California 92152 C. Martin R. Platt, CSIRO, Division of Atmospheric Physics, P.O. Box 77, Mordialloc, Victoria, Australia 3195 H. R. Pruppacher, Division of Atmospheric Sciences, University of California at Los Angeles, Los Angeles, California 90024 Lary Radke, Department of Atmospheric Sciences, AK-40, University of Washington, Seattle, Washington 98195 G. D. Robinson, The Center for the Environment and Man, Inc., 275 Windsor Street, Hartford, Connecticut 06120 Kenneth Sassen, University of Utah, 819 Browning Building, Salt Lake City, Utah 84112 Michael Starks, USAMSAA, DRXSY-GS, Aberdeen Proving Ground, Aberdeen, Maryland 21005 Graeme Stephens, Department of Atmospheric Sciences, Colorado State Univer­ sity, Fort Collins, Colorado 80523 Z. G. Sztankay, Harry Diamond Laboratories, DELHD-R-CM-NM, 2800 Powder Mill Road, Adelphi, Maryland 20783 Robert Vaglio-Laurin, Department of Applied Sciences, New York University, 23-36 Stuyvesant Street, New York, New York 10003 PARTICIPANTS ιχ Paul Wang, Department of Atmospheric Sciences, University of California, 405 Hilgard Avenue, Los Angeles, California 90024 Pi Wang, Institute for Atmospheric Optics and Remote Sensing, P. O. Box P, Hampton, Virginia 23666 James A. Weinman, Department of Meteorology, University of Wisconsin, Madison, Wisconsin 53706 Christian Werner, DFVLR, 8031 Oberpfoffenhofen, West Germany David Wu, Institute for Atmospheric Optics and Remote Sensing, P. O. Box P, Hampton, Virginia 23666 Man-Li C. Wu, NASA-Goddard Space Flight Center, Code 915, Greenbelt, Maryland 20771 Glenn K. Yue, Institute for Atmospheric Optics and Remote Sensing, P. O. Box P, Hampton, Virginia 23666 FOREWORD The papers contained in this volume present the reader with an excellent assess­ ment and concise summary of our current knowledge and the theoretical and experi­ mental aspects of the microphysical, and optical properties of clouds. This tutorial program on the Symposium on Clouds: Their Formation, Optical Properties, and Ef­ fects was held in Williamsburg, Virginia, May 13-14, 1980. Understanding the physics and radiative properties of clouds and fogs is essential for acquiring the know how for estimating and predicting the effects of the cloudy environments on the per­ formance of various sensor systems deployed in different fields, such as, defense, communications, and weather, and for developing valid models for realistic atmos­ pheric conditions containing clouds, fogs, hazes, rain, snow, etc. I feel that these papers and the follow-up discussions will provide the initiate, the advanced researcher, as well as the program manager, with the concise review of the state of the art and will help identify those areas in which further research efforts are needed in the near future. Richard Β. Gomez xi PREFACE This volume contains the technical proceedings of the Symposium on Clouds: Their Formation, Optical Properties, and Effects, held in Williamsburg, Virginia, May 13-14, 1980. The symposium consisted of a tutorial program of eleven invited review papers on the subject of clouds presented to a select audience of forty-two in­ vited participants from universities, nonprofit institutions, research laboratories, and government agencies in the United States, Canada, West Germany, England, and Australia. The invited papers were grouped under the headings of structure of clouds, interaction of passive radiation with clouds, and interaction of active radiation with clouds. During the past few years, significant advances have been made in our ability to characterize the properties of clouds through detailed in site and remote sensing tech­ niques, and these have led to improvements in our understanding of cloud processes. In the next few years, we should see these techniques and new knowledge applied with increasing effectiveness to many areas of meteorology—weather forecasting, weather modification, climate, atmospheric chemistry, and to many areas of technol­ ogy that interface with the atmosphere—aviation and satellite meteorology, remote sensing, communication systems, to mention only a few. One of the most profound effects of clouds on the meteorology of our planet is in their interactions with radiation. These interactions play crucial roles in determining long-term climatic trends, as well as daily weather. In addition, many important areas of technology involving man-made sources of radiation (for example, lasers) and communication systems are presently limited in their reliability and applications by insufficient understanding of the ways in which they interact with clouds. On the other hand, these same technologies are providing new means of probing clouds which may, in the future, prove as valuable to meteorology as radar. In view of these considerations, it seems particularly opportune at this time to re­ view our knowledge of clouds and their optical properties and to assess the nature and scope of the new research programs that are needed to advance our understanding of these subjects. This was the purpose of this symposium and workshop. xiii xiv PREFACE The symposium was followed by a two-day workshop in which twenty experts on clouds and their optical properties were asked to identify the principal gaps in our knowledge of the optical properties of clouds and the types of research efforts that should be mounted to remove these gaps. The deliberations and recommendations of the workshop participants are contained in a separately published workshop report. In order to ensure that major disciplines involved were properly represented, a Sci­ entific Program Committee composed of the following scientists was set up: Profes­ sor P. V. Hobbs, University of Washington, Chairman; Professor A. I. Carswell, York University, Toronto, Canada; Professor S. Κ. Cox, Colorado State University; Dr. A. Deepak, Institute for Atmospheric Optics and Remote Sensing; and Professor H. Pruppacher, University of California at Los Angeles. The editors wish to acknowledge the cooperation of the authors, members of the Scientific Program Committee, and the participants for making this a successful and valuable symposium. It is a pleasure to acknowledge the valuable assistance of the symposium coordinator, Miss Susan K. Woodfin, Institute for Atmospheric Optics and Remote Sensing, for the smooth organization of the symposium and the typing of the final manuscripts. Special thanks are due to Dr. Richard B. Gomez, U. S. Army Atmospheric Sciences Laboratory, who not only conceived the idea for the sympo­ sium and arranged the financial support, but also participated in various aspects of its organization. Thanks are also due Dr. Leo Alpert, Army Research Office, for the additional financial support that was needed to enhance the scope and quality of the symposium. Peter V. Hobbs Adarsh Deepak SCALES INVOLVED IN THE FORMATION AND ORGANIZATION OF CLOUDS AND PRECIPITATION1 Peter V. Hobbs Atmospheric Sciences Department University of Washington Seattle, WA The spatial and temporal scales involved in the formation and organization of clouds and precipitation range from the micro- physical up to the planetary. This enormous range of scales may be divided into three main categories (macro, meso, and micro) and eleven subcategories. Consideration of scales is important in evaluating cloud and precipitation processes and their effects. The formation and organization of the clouds and precipitation in extratropical cyclones is used to illustrate the role and importance of various scales of phenomena. I. INTRODUCTION The processes involved in the formation and organization of clouds and precipitation range from the very small-scale physical and chemical processes involved in the nucleation and growth of cloud particles up to the very large-scale dynamical processes that are associated with synoptic weather systems. Awareness and ^Research supported by the Atmospheric Research Section of the National Science Foundation (ATM74-14726-A02 and ΆΤΜ77-01344; U. S. Army Research Office (DAAG29-79-G-0005), and the U. S. Air Force Office of Scientific Research (F49620-77-C-0057'). Copyright © 1981 by Academic Press, Inc. Clouds: Their Formation, Optical Properties, and Effects 1 All rights of reproduction in any form reserved. ISBN 0-12-350720-0 PETER V. HOBBS 2 proper consideration of scale is important, not only in deter­ mining the effects of a particular phenomenon but in planning field programs. For example, the areal density of measurements should be at least sixteen times greater than the areal scale of the phenomenon under investigation. II. DISCUSSION Shown on the right-hand side of Fig. 1 is a classification of atmospheric processes based on their horizontal spatial scale (indicated on the left-hand side of Fig. 1). Phenomena with horizontal scales > 1000 km are referred to as macroscale (or synoptic-scale, since they are resolved by synoptic data). Phenomena with horizontal spatial scales ranging from a few kilometers up to about 1000 km are called mesoscale. Smaller scale phenomena (< 1 km) are termed microscale. To provide further refinement, the macroscale may be divided into two subdivisions (a and β), the mesoscale into three subdivisions (a, 3, and γ) and the microscale into six subdivisions (α, β, γ, ό, ξ, and ζ) as shown in Fig. 1. To impress upon the reader the enormous extent of the fifteen orders of magnitude covered by the horizontal spatial scales shown in Fig. 1, it might be noted that the ratio of the linear dimen­ sions of the Milky Way to that of the earth is also about 10"*"^! It is a most remarkable achievement that technological advances over the past decade now allow observations and measurements over this entire size range of atmospheric phenomena to be made. In the remainder of this paper the concept of scales of phenomena are illustrated by considering the organization of clouds and precipitation in extratropical cyclones, which dominate the weather throughout the mid-latitudes of the world. On the macroscale, extratropical cyclones may be viewed as cyclonic circulations embedded within baroclinic waves in the

See more

The list of books you might like

Most books are stored in the elastic cloud where traffic is expensive. For this reason, we have a limit on daily download.