Author: Summer School in Space Physics, Alpbach, Austria, 1963Publisher:
ISBN:
Category : Earth
Languages : en
Pages :
Book Description
Introduction to solar terrestrial relations: proceedings, ed
Author: Summer School in Space Physics, Alpbach, Austria, 1963Publisher:
ISBN:
Category : Earth
Languages : en
Pages :
Book Description
Introduction to Solar Terrestrial Relations
Author: J. OrtnerPublisher: Springer Science & Business Media
ISBN: 9401035903
Category : Science
Languages : en
Pages : 499
Book Description
TO SOLAR TERRESTRIAL RELATIONS PROCEEDINGS OF THE SUMMER SCHOOL IN SPACE PHYSICS HELD IN ALPBACH, AUSTRIA, JULY 1S-AUGUST 10,1963 AND ORGANIZED BY THE EUROPEAN PREPARATORY COMMISSION FOR SPACE RESEARCH (COPERS) Edited by J. ORTNER European Space Research Organisation. Paris and H. MAS ELAND Sterrewacht ' Sonnenborgh' • Utrecht D. REIDEL PUBLISHING COMPANY DORDRECHT-HOLLAND e-ISBN-13:978-94-010-3590-3 IS8N-13:978-94-0 10-3592-7 00110. 1007/978-94-010-3590-3 '96' Softoover reprint of the hardcover 1st edition 1965 All rights reserved No part of this book may be reproduced in any fonn. by print, photoprint, microfilm, or any other means without permission from the publisher FOREWORD The textbook presented in the following is composed of the proceedings of the Summer School in Space Physics held during the summer months of 1963. This Summer School was organized by the Preparatory Commission (COPERS) of the European Space Research Organisation (ESRO). It was the first time that such a summer course was held in Europe on a subject of space physics. Thanks to an invitation from the Austrian Government these lectures were given in the College House of Alpbach, Tyrol. Eight outstanding European scientists each presented five two-hour lectures on topics covering the region between the Sun and the Earth. The courses contained the physics of the Sun, the Interplanetary Medium and Trapped Radiation, the Ionosphere and High Latitude Phenomena. Furthermore, a course on space instrumentation was given. Sixty students were selected to attend the courses.
Introduction to Solar Terrestrial Relations
Author: J. OrtnerIntroduction to Solar Terrestrial Relations
Author: J. OrtnerPublisher:
ISBN:
Category : Atmosphere, Upper
Languages : en
Pages : 534
Book Description
Introduction to Solar Terrestrial Relations
Author: J. OrtnerSolar-Terrestrial Physics/1970
Author: International Symposium on Solar-Terrestial PhysicPublisher: Springer Science & Business Media
ISBN: 9400936931
Category : Science
Languages : en
Pages : 937
Book Description
This volume contains the review papers presented at the International Symposium on Solar-Terrestrial Physics held at the Tavrichesky Palace, Leningrad, U.S.S.R., 11-19 May 1970. The Symposium may be regarded as the most recent member of a series of inter national symposia - for instance, the Symposium on Solar-Terrestrial Physics, Belgrade (1966), the Joint IQSY-COSPAR Symposium on Solar-Terrestrial Physics, London (1967), and the Symposium on the Physics of the Magnetosphere, Washington (1968). Like those earlier symposia, the Leningrad Symposium was sponsored by the International Astronomical Union (IAU), the International Union of Geodesy and Geophysics (IUGG), the International Union of Radio Sciences (URSI), and the ICSU Committee on Space Research (COSPAR). These bodies are all concerned with one or another aspect of solar-terrestrial physics, and all joined in believing that the time was ripe for another comprehensive symposium on all aspects of this very active field of research.
Illustrated Glossary for Solar and Solar-Terrestrial Physics
Author: A. BruzekPublisher: Springer Science & Business Media
ISBN: 9401012458
Category : Science
Languages : en
Pages : 220
Book Description
At the XV. General Assembly of the International Astronomical Union in Sydney 1973, Commission 10 for Solar Activity requested the incoming Organising Committee to establish a small group to recommend a standard nomenclature for solar features and to prepare an illustrated text which would clear the jungle of terms for the benefit of solar physicists as well as of theoreticians and research workers in related fields. The challenge was taken up by the president of Commission 10, Prof. K. O. Kiepenheuer, and his persuasive advocacy has led eventually to the present book. In the course of the work, the declared aim but not the basic purpose was revised. Rather than prepare a list of standard terms, we have preferred to collect together all the terms that appear in current English-language literature. Synonyms and partially overlapping terms are all recorded for the most part without prejudice. Each has been defined as exactly as possible with the hope that in the future they may be used and understood without ambiguity. It would be a step on the road to standardisation if these terms were not re-used for new phenomena. New observations and new theories will lead to reappraisals and redefinitions so the Glossary is intended more as a guide to the present situation than as a rule-book.
Introduction to Astronomical Photometry
Author: M. GolayPublisher: Springer Science & Business Media
ISBN: 9401021694
Category : Science
Languages : en
Pages : 376
Book Description
The material given in this 'Introduction to astronomical photometry' is the subject matter of a lecture at the University of Geneva. It is, therefore, intended for those students, physicists or mathematicians, who have completed their bachelor's degree or diploma, and are intending to work for their Ph.D. in astronomy. We assume then the elementary ideas of astrophysics, magnitude, colour index, spectral classes, luminosity classes, gradient, atmospheric extinction are already known. The student may find it useful to re-read the work of Schatzman [1], Dufay [2] and Aller [254] before embarking upon the study of this 'Introduction to astronomical photometry'. It is not our aim in this book to deal with every aspect of stellar photometry. On the contrary, we shall restriet ourselves to looking at subjects ofwhich knowledge seems to us essential for someone who has to use photometrie quantities in his astronomical research. We are, therefore, keeping the interests of the photometrie measurements user partieularly in mind. We shall only discuss very superficially the technical prob lems and reduction methods for atmospheric extinction. These problems are dealt with very clearly in Astronomical Techniques [3]; the first by A. Lallemand, H. L.
Multivariate Data Analysis
Author: Fionn MurtaghPublisher: Springer Science & Business Media
ISBN: 940093789X
Category : Mathematics
Languages : en
Pages : 225
Book Description
Interest in statistical methodology is increasing so rapidly in the astronomical community that accessible introductory material in this area is long overdue. This book fills the gap by providing a presentation of the most useful techniques in multivariate statistics. A wide-ranging annotated set of general and astronomical bibliographic references follows each chapter, providing valuable entry-points for research workers in all astronomical sub-disciplines. Although the applications considered focus on astronomy, the algorithms used can be applied to similar problems in other branches of science. Fortran programs are provided for many of the methods described.
Effects of Mass Loss on Stellar Evolution
Author: C. ChiosiPublisher: Springer Science & Business Media
ISBN: 9400985002
Category : Science
Languages : en
Pages : 562
Book Description
The IAU Colloquium No. 59, "The effects of mass loss on Stellar Evolution" was held on September 15-19, 1980 at the International Centre for Theoretical Physics, Miramare, Trieste (Italy), under the auspices of the IAU Executive Co~ mittee and the Italian National Council of Research. The planning of this conference began two years ago du ring the IAU Symposium No. 83 "Mass loss and evolution of 0 type stars" (Qualicum Beach, Victoria, Canada) when we felt that mass loss and its effects on the evolution of stars was too broad a subject for being confined to 0 type stars only. Therefore we thought that a conference dealing with the general problem of mass loss across the whole HR diagram would have been of interest to all people working in the field. The main idea was that bringing together Astronomers and Astrophysicists of the widest range of interests and e~ pertize - all in some way related to the problem of mass loss from stars - would have spurred thorough discussions on the many aspects and implications of this topic. We hope this goal has been achieved. Furthermore, the most recent observational and theoreti cal developments on the problem of mass loss from early ty pe stars avoided this meeting to be a simple updating of the Qualicum Beach Symposium as far as this issue is concerned.